-------------------
27/09/2021 (v16.12)
-------------------
- Add spacecraft 9 and 10 for GOES16 and GOES17

-------------------
22/09/2021 (v16.11)
-------------------
- Correction for bepi_ena

-------------------
21/09/2021 (v16.11)
-------------------
- Add BEPI_MIA lmode moments

-------------------
20/09/2021 (v16.10)
-------------------
- New experiements bepi_ena, bepi_ephemeris, bepi_hk, bepi_mia, bepi_msa
- In Distribution Function plot (Vper1,Vpar) arrow is now the direction of V instead of B

-------------------
22/07/2021 (v16.09)
-------------------
- New products for BEPI-COLOMBO/MPO/MAG with magnetic field in VSO
- New products for SOLAR-ORBITER/PAS with proton and alpha distribution

-------------------
30/06/2021 (v16.08)
-------------------
- Modif for bepi_mmomag and bepi_mmomag
- Modif for SOLAR_PAS proton and alpĥa frame

-------------------
28/06/2021 (v16.07)
-------------------
- Bug correction

-------------------
27/06/2021 (v16.06)
-------------------
- Bug correction

-------------------
26/06/2021 (v16.05)
-------------------
- Correction for FDL

-------------------
26/06/2021 (v16.04)
-------------------
- Change TimeComment in clweb
- Add bepi/mmomag experiment
- Correction for FDL
- Mise à jour de mvn_swe_calib.txt

-------------------
21/06/2021 (v16.03)
-------------------
- Add for SOLAR-ORBITER/PAS 2 products with alpha and proton separation
- Change "data display" max value to 999 in File/Export

-------------------
14/06/2021 (v16.02)
-------------------
- Bug correction

-------------------
10/06/2021 (v16.01)
-------------------
- Change data available for CLWeb MAVEN PDS users
- New product SF00_MOM_FULL for PSP_SPI with proton moments computed in RTN

-------------------
27/04/2021 (v16.00)
-------------------
- Mofifications for GDL and FL
- New modes for CLUSTER_HIA: P40=mode PROM1 in hig G and P42=mode PROM1 in low g
- Modifications of JASON3_AMBRE calibration

-------------------
15/02/2021 (v15.54)
-------------------
- bugs correction

-------------------
11/02/2021 (v15.53)
-------------------
- Bug correction in interpolation of Distribution function
- Bug correction in ACE SWEPAM
- Bug correction in CLUSTER PEACE
- Bug correction in magnetic field of INTERBALL ELECTRON
- Bug correction in MAVEN LPW
- Bug correction in MAVEN STATIC
- Bug correction in PSP_MAG (change pathnames)
- Add RTN info in SOLAR_EPHEMERIS
- Speed optimisation when using FDIST_TO_FDIST, FLUX_TO_FLUX or JE_TO_JE
- Speed optimisation when reading CDF variables

-------------------
15/12/2020 (v15.52)
-------------------
- New experiment PSP_EPHEMERIS
- Add orbit data in SOLAR_EPHEMERIS

-------------------
16/11/2020 (v15.51)
-------------------
- New experiment PSP_FORMAGONLY

-------------------
16/11/2020 (v15.50)
-------------------
- New experiment SOLAR_FORMAGONLY
- Add V_SOLO in (Vr,Vt,Vn) in moments computation in SOLAR_PAS
- Modification for gdl

-------------------
09/11/2020 (v15.49)
-------------------
- Add SOLO VELOCITY in RTN in SOLAR_EPHEMERIS
- Correction for SOLAR_PAS

-------------------
06/11/2020 (v15.48)
-------------------
- bug correction for SOLAR-ORBITER
- add eigenvector EV1, EV2 and EV3 in moments computation

-------------------
28/10/2020 (v15.47)
-------------------
- New product SYS-HSK for BEPI_MEA1 and BEPI_MEA2
- Modif for clweb (XHR.status)

-------------------
21/10/2020 (v15.46)
-------------------
- Correction for SOLAR_PAS
- Correction for clweb

-------------------
19/10/2020 (v15.45)
-------------------
- Add product PROM_1 for CLUSTER_HIA

-------------------
16/10/2020 (v15.44)
-------------------
- Add arrow with B direction in Distribution Function plot
- Bug correction in distribution function plot

-------------------
12/10/2020 (v15.43)
-------------------
- add SOLAR EPHEMRIS with PAS -> RTN matrix
- add SOLAR PAS L2 products: MOM, 1D and 3D

-------------------
05/10/2020 (v15.42)
-------------------
- Add SOLAR MAG data available at soar (5 products)
- New experiment MPOMAG for BEPI-COLOMBO

-------------------
24/07/2020 (v15.41)
-------------------
- New format possible for time_comment: "timetag, type, message" and type can be defined in $HOME/.cl/time_comment.config

-------------------
22/07/2020 (v15.40)
-------------------
- Add SOLAR_MAG data

-------------------
10/07/2020 (v15.39)
-------------------
- Modif for BEPI_MEA if geom_factor is out of range
- Modif for SOLAR_PAS

-------------------
18/06/2020 (v15.38)
-------------------
- New product UNK for TARANIS/XGRE
- Optimisation for SOLAR/PAS

-------------------
15/06/2020 (v15.37)
-------------------
- Bug correction
- Correction for SOLAR-PAS

-------------------
10/06/2020 (v15.36)
-------------------
- Can remove first 1Hz or average of 4hz distributions functions of SOLAR_PAS
- Add products 3DL2 and MOML2 for SOLAR_PAS
- Correction for JASON3_AMBRE

-------------------
20/04/2020 (v15.35)
-------------------
- Modification for SOLAR_PAS and SOLAR_MAG

-------------------
20/04/2020 (v15.34)
-------------------
- Modification for SOLAR_PAS

-------------------
19/04/2020 (v15.33)
-------------------
- New experiment SOLAR_PAS with CDAG data

-------------------
16/04/2020 (v15.32)
-------------------
- Modification for SOLAR_PAS

-------------------
15/04/2020 (v15.31)
-------------------
- Correction for SOLAR_PAS
- Correction for cl -rt

-------------------
13/04/2020 (v15.30)
-------------------
- Add views in BEPI-COLOMBO/MMO/NECP
- Bug correction for BEPI-COLOMBO

-------------------
09/04/2020 (v15.29)
-------------------
- Modification for BEPI_MEA
- Modification for cl -rt

-------------------
07/04/2020 (v15.28)
-------------------
- Correction for PSP_SPE
- Add product Precomputed MOM Burst for STEREO_SWEA
- Modification for cl -rt
- cl can now read csv files

-------------------
01/04/2020 (v15.27)
-------------------
- Modification for SOLAR_PAS commissionning with -rt option
- Modification for TARANIS_IDEE (correction in nanosec)

-------------------
17/03/2020 (v15.26)
-------------------
- Change IHM of cl when rt option is used
- Refresh interval can be changed in General/Expert when -rt option is used
- Raw values of energy, theta and phi can be used for time_energy, time_theta, time_phi and phi_theta spectrogram (variable etp_use_raw_values in Data)
- For SOLAR_PAS: use full E, Az and El tables in moments computation

-------------------
05/03/2020 (v15.25)
-------------------
- New product psp_fld_l2_mag_RTN_4_Sa_per_Cyc pour PSP_MAG
- Better time resolution in timeaxis (nanosec in LONG64 instead of millisec in DOUBLE)
- Modification for TARANIS

-------------------
13/02/2020 (v15.24)
-------------------
- Modification for TARANIS_XGRE

-------------------
12/02/2020 (v15.23)
-------------------
- New experiment PSP_SPI with data from AF00, AF01, SF00, SF01 and SF0A

-------------------
06/02/2020 (v15.22)
-------------------
- Bug correction for CentOS8

-------------------
05/02/2020 (v15.21)
-------------------
- Optimisation
- Bug correction for JASON3_AMBRE
- Modification for TARANIS

-------------------
28/01/2020 (v15.20)
-------------------
- Add the possibility to substract a fraction of background for JUNO_JADEI
- Modif for TARANIS_XGRE
- Modif pour TARANIS EVENT VIEWER

-------------------
16/01/2020 (v15.19)
-------------------
- New object tev to display TARANIS event data
- Path modifications for PSP_MAG and PSP_SPC

-------------------
18/12/2019 (v15.18)
-------------------
- Add the possibility to remove background for JUNO-JADEI
- Bug correction with JUNO-JADEI pitchangle
- New PSP-SPE product psp_swp_spe_sf0_L3_pad

-------------------
04/12/2019 (v15.17)
-------------------
- New product CAL in SOLAR-PAS
- Modification in JUNO-JADEI

-------------------
25/11/2019 (v15.16)
-------------------
- Add "Manual Normalized to mean" in Zmin-Zmax choices

-------------------
19/11/2019 (v15.15)
-------------------
- Bug correction

-------------------
28/10/2019 (v15.14)
-------------------
- Add computation of Energy conversion Rate parameters for MMS

-------------------
27/09/2019 (v15.13)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Modification for BEPI-MEA
- Modification for MAVEN-NGI
- Bug correction

-------------------
16/09/2019 (v15.12)
-------------------
- Add Emin and Emax buttons unsed in NFQE computation for JASON3/AMBRE
- Bug correction

-------------------
14/08/2019 (v15.11)
-------------------
- Add Apply/Unapply TimeComment
- Modifications for gdl 0.9.9
- Modifications for BEPI-MEA (new MDP from Yokota in August 2019)
- Add 2 PAD datasets for PSP/SPE

-------------------
27/06/2019 (v15.10)
-------------------
- Add TimeComment/Properties to change charsize and oientation of characters
- Add calibrations for SOLAR/PAS

-------------------
17/06/2019 (v15.09)
-------------------
- Add PSP SPE experiment with pitch-angle data
- Add Z scale "Normalized to mean"

-------------------
11/06/2019 (v15.08)
-------------------
- Bug correction in MMS ohm law computation

-------------------
04/06/2019 (v15.07)
-------------------
- Add PSP kp data

-------------------
28/05/2019 (v15.06)
-------------------
- Modification of JUNO-JADEE azimuth angle
- Correction in SOLAR-PAS moments computation

-------------------
22/05/2019 (v15.05)
-------------------
- Correction in Distribution Function plot for JUNO-JADEE

-------------------
21/05/2019 (v15.04)
-------------------
- Correction for JUNO-JADEE
- Bug correction in average and interpolation

-------------------
09/05/2019 (v15.03)
-------------------
- When a ".cl" containing a time table is loaded, the time table file is reloaded but not necessarily applied
- Add PSP_MAG product at 15 ms resolution

-------------------
09/05/2019 (v15.02)
-------------------
- Bug correction in PSP_MAG
- Add Refresh time table button
- ".cl" file doesn't contains any more intervalls of time table previously loaded
- When a ".cl" containing a time table is loaded, the time table file is reloaded

-------------------
07/05/2019 (v15.01)
-------------------
- Bug correction for computation of 3D JUNO-JADEE

-------------------
06/05/2019 (v15.00)
-------------------
- Bug correction for JUNO-JADEE and in heat flux computation
- Add Mag for PSP project

-------------------
04/04/2019 (v14.92)
-------------------
- Add the possibility to save a time table with 1 msec resolution (instead of 1 sec)

-------------------
03/04/2019 (v14.91)
-------------------
- Modifications for JUNO-JADEE 3D products

-------------------
29/03/2019 (v14.90)
-------------------
- Modifications for JUNO-JADEE

-------------------
08/03/2019 (v14.89)
-------------------
- bug correction for JUNO/JADEI in LRS mode

-------------------
21/02/2019 (v14.88)
-------------------
- add rtn frame in JUNO/JADEI 3D moments computation

-------------------
19/02/2019 (v14.87)
-------------------
- thBV has been renamed in thBX in get_b_connection
- add JSS frame in JUNO/JADEI 3D moments computation
- add project Parker Solar Proble (PSP) with experiments spa, spb and spc

-------------------
04/02/2019 (v14.86)
-------------------
- Bug correction

25/01/2019 (v14.85)
-------------------
- Remove SOLAR/PAS 3DN, 3DS and 3DB
- Add quantities in MMS ohm law (from Sid calc_lengths.py)
- Modif when plotting text data
- Modif calibrations of MAVEN/SWEA

-------------------
21/12/2018 (v14.84)
-------------------
- Add -rt option in cl command line

-------------------
27/11/2018 (v14.83)
-------------------
- Version for SOLAR-PAS tests in Munich

-------------------
22/11/2018 (v14.82)
-------------------
- Cl can now use VALIDMIN, VALIMAX, SCALEMIN and SCALEMAX in CDF files.

-------------------
09/11/2018 (v14.81)
-------------------
- Bug correction in clweb timer

-------------------
08/11/2018 (v14.80)
-------------------
- Modif timer in clweb

-------------------
07/11/2018 (v14.79)
-------------------
- Bug correction for batch in clweb

-------------------
06/11/2018 (v14.78)
-------------------
- Modif varnames for SOLAR-HSK
- Bug correction in webservice

-------------------
15/10/2018 (v14.77)
-------------------
- Bug correction for 32 bits architecture
- Can plot VALIDMIN and VALIDMAX for SOLAR-PAS HSK

-------------------
20/09/2018 (v14.76)
-------------------
- Modif for SOLAR/PAS
- Bug correction

-------------------
06/08/2018 (v14.75)
-------------------
- Bug correction in clweb
- In title, spacecraft is now at the center and experiement on the left

-------------------
10/07/2018 (v14.74)
-------------------
- Modif for BEPI_MEA
- Modif for MAVEN_SWIA
- Add quantities in MMS ohm law

-------------------
04/07/2018 (v14.73)
-------------------
- Add VENUS_B_CONNECTION for VENUS_EXPRESS

-------------------
21/06/2018 (v14.72)
-------------------
- Modif for SOLAR and BEPI
- Bug correction

-------------------
18/06/2018 (v14.71)
-------------------
- Modif for SOLAR

-------------------
15/06/2018 (v14.70)
-------------------
- Modif for BEPI/MEA
- Modif for SOLAR/PAS
- Bug correction
- Label button now display panels number
- MMS FPI l1b data are now unavailable under clweb

-------------------
05/06/2018 (v14.69)
-------------------
- Modification for Video output for MMS (add millisecond in filename)

-------------------
05/06/2018 (v14.68)
-------------------
- Bug correction 
- Add MOM file for SOLAR-PAS

-------------------
04/06/2018 (v14.67)
-------------------
- Bug correction Ytickv

-------------------
31/05/2018 (v14.66)
-------------------
- Correction in lawohm computation for MMS

-------------------
31/05/2018 (v14.65)
-------------------
- Modif for MMS and BEPI

-------------------
29/05/2018 (v14.64)
-------------------
- Modif for MMS-DES and MMS-DIS
- New parameters in Ohm Law for MMS

-------------------
22/05/2018 (v14.63)
-------------------
- Modifications for SOLAR/PAS

-------------------
14/05/2018 (v14.62)
-------------------
- Add experiment SOLAR/PAS with products HSK and 3D

-------------------
03/05/2018 (v14.61)
-------------------
- Add Agyrotropy terms in Ohm Law for MMS

-------------------
02/05/2018 (v14.60)
-------------------
- Add some terms in Ohm Law for MMS

-------------------
25/04/2018 (v14.59)
-------------------
- Add Ohm Law terms for MMS
- Bug correction

-------------------
27/03/2018 (v14.58)
-------------------
- Modif plot of JASON3 and MAVEN Quicklook

-------------------
23/03/2018 (v14.57)
-------------------
- Modif for JASON3 Quicklook
- Modif for BEPI/MEA

-------------------
20/03/2018 (v14.56)
-------------------
- Add predefined plot mms_manu_fdist_elec_1d.cl and mms_manu_fdist_ions_1d.cl for MMS

-------------------
19/03/2018 (v14.55)
-------------------
- F5 is now a shortcut for "Clean cache and recompute"
- Bug correction

-------------------
07/03/2018 (v14.54)
-------------------
- Add "Remove TT" in Webonly menu
- Optimization

-------------------
28/02/2018 (v14.53)
-------------------
- Modification of MAVEN potential file
- use https instead of http for cdaweb

-------------------
27/02/2018 (v14.52)
-------------------
- New MAVEN potential file format (epoch, potential and method)

-------------------
21/02/2018 (v14.51)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Add MARS_B_CONNECTION in MGS tree
- Current computation: add Curv, Curv[xyz] and new algorithm to compute Rc

-------------------
19/01/2018 (v14.50)
-------------------
- Modification for BEPI-COLOMBO (add RECORD field in each product)
- Bug correction

-------------------
18/01/2018 (v14.49)
-------------------
- Modification for mouse and crosshair in clweb

-------------------
16/01/2018 (v14.48)
-------------------
- Modification for BEPI

-------------------
15/01/2018 (v14.47)
-------------------
- Modification for MMS quicklooks

-------------------
12/01/2018 (v14.46)
-------------------
- Bug correction

-------------------
09/01/2018 (v14.45)
-------------------
- Bug correction in batch mode
- Modif for BEPI-COLOMBO

-------------------
21/12/2017 (v14.44)
-------------------
- Modif for BEPI-COLOMBO

-------------------
20/12/2017 (v14.43)
-------------------
- When plotting epoch field, data is now in type DOUBLE instead of FLOAT

-------------------
19/12/2017 (v14.42)
-------------------
- New Accelerator F4 to quickly add the current time based on mouse position to a TimeComment

-------------------
18/12/2017 (v14.41)
-------------------
- Modif for BEPI/MEA and TARANIS
- Modif of batchfile in order to create output for many plots at different time-intervall
- Modif for TimeComment
- New menu File/Execute batch file

-------------------
07/12/2017 (v14.40)
-------------------
- New button EXP to switch experiment (for example BEPI_MEA1/BEPI_MEA2 and TARANS_IDEEN/TARANIS_IDEEZ)
- New menu TimeComment to display vertical lines with comment (file format is yyyy-mm-ddThh:mm:ss.mscZ comment)
- New experiment TARANIS_EPHEMERIS
- TARANIS A,AP,B,C,D,E files are now in compressed format ".v86"
- New button "Actions/Clean cache and recompute" (useful when data files change in real time)

-------------------
01/12/2017 (v14.39)
-------------------
- Modification for TARANIS

-------------------
30/11/2017 (v14.38)
-------------------
- Modification for TARANIS
- Optimization

-------------------
24/11/2017 (v14.37)
-------------------
- Continents can now be correctly displayed with longitude 0-360 
- Correction in energy_cjf, pitch_cjf and mass_cjf when data are accumulated
- Bug correction

-------------------
17/11/2017 (v14.36)
-------------------
- Bug correction in energy_pitchangle for MMS
- Bug correction in energy_cjf plot with a pitch-angle selection when data are accumulated

-------------------
15/11/2017 (v14.35)
-------------------
- Modification for macOS High Sierra

-------------------
13/11/2017 (v14.34)
-------------------
- cl can create binary files for MAVEN with position, theta and phi angles in MSO

-------------------
06/11/2017 (v14.33)
-------------------
- It's now possible to define up to 5 parameters in a panel composer. A parameter is defined by a mathematical
  expression with plots in different panels. The plot j of panel i is called Pi_j.

  If panel 2 contains Bx (C1), By(C2) and Bz(C3) then parameter sqrt(P2_C1*P2_C1+P2_C2*P2_C2+P2_C3*P2_C3) is the
  amplitude of vector in panel 2.

  These parameters can be selected in SPECIAL branch of tree selection.

-------------------
20/10/2017 (v14.32)
-------------------
- Add File/WAVELET export menu that creates from a timeseries a cef file with wavelet data.

-------------------
18/10/2017 (v14.31)
-------------------
- Add the possibility to export cef file at one microsecond resolution

-------------------
12/10/2017 (v14.30)
-------------------
- Add the possibility to show t1-t2 when accumulate data in Distribution Function
- Modification in time_energy spectrogram with pitchangle selection

-------------------
04/10/2017 (v14.29)
-------------------
- Add IMAP3 INTERBALL-AURORAL data

-------------------
02/10/2017 (v14.28)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Bug correction
- Modif for GDL

-------------------
05/07/2017 (v14.27)
-------------------
- Bug correction in orbito panel 
- Add JUNO magnetic field data from PDS

-------------------
29/06/2017 (v14.26)
-------------------
- Modif for new clweb computer (CentOS-7, IDL 8.4, 256G RAM)
- Default cache size for each clweb user is now 10 Gbytes

-------------------
20/06/2017 (v14.25)
-------------------
- Modification in Average or Max bins used in 'Distribution Function', 'energy_pitchangle' and 'phi_theta' plots
- New products time_pitchangle for MMS_FEEPSE and MMS_FEEPSI
- Modification of MAVEN_SWEA clibrations

-------------------
07/06/2017 (v14.24)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Modification for JASON3_AMBRE (there is now 3 configurations)
- Modification of quality wording in MAVEN_NGIMS

-------------------
16/05/2017 (v14.23)
-------------------
- New widget in Time tab: Type ("Average" ou "Max") to display Average or Max of bins used in Distribution Function plot
- Number of energies in MMS_HPCA srvy is now 16 instead of 64

-------------------
11/05/2017 (v14.22)
-------------------
- Add computation of N, F, Q and E in JASON3_AMBRE
- Add predefined plots for MMS
- Bug correction

-------------------
03/05/2017 (v14.21)
-------------------
- Modification of JASON3_AMBRE electron and ion energy table
- Modification for JUNO and BEPI
- Bug correction

-------------------
28/04/2017 (v14.20)
-------------------
- Modification for BEPI-COLOMBO and MAVEN/NGI

-------------------
14/04/2017 (v14.19)
-------------------
- Add some predefined plots for BEPI-COLOMBO
- Bug correction in time_pitchange output

-------------------
11/04/2017 (v14.18)
-------------------
- Correction for MMS/EDI and MMS/EPD-EIS
- Modif of CDAWeb tree

-------------------
24/03/2017 (v14.17)
-------------------
- Add orbit IRAP in JASON3 ephemeris

-------------------
23/03/2017 (v14.16)
-------------------
- Bug correction in MMS-EDP
- Modification for BEPI-COLOMBO

-------------------
15/03/2017 (v14.15)
-------------------
- Correction for BEPI-COLOMBO

-------------------
14/03/2017 (v14.14)
-------------------
- Bug correction
- Add "Reduce high" widget in Z spectrogram to reduce or not color palette when panels are superimposed

-------------------
13/03/2017 (v14.13)
-------------------
- Bug correction

-------------------
06/03/2017 (v14.12)
-------------------
- Change data available for CLWeb MAVEN PDS users

-------------------
01/03/2017 (v14.11)
-------------------
- Modification in MAVEN_SWEA calibrations
- Modification in time table obj.xml created with constraints

-------------------
28/02/2017 (v14.10)
-------------------
- Correction in MMS pressure tensor gradient
- Add computation of IMF_cone_angle_GSE, IMF_clock_angle_GSE and IMF_clock_angle_GSM in OMNI 1 and 5 mn resolution data

-------------------
23/02/2017 (v14.09)
-------------------
- Correction in MMS pressure tensor gradient

-------------------
22/02/2017 (v14.08)
-------------------
- Add B magnitude in JUNO-MAG
- Add Pt = Pp + Pm in 3D moments computation
- Add fields (par/perr) computed with fgm in pressure tensor gradient for MMS DES and DIS
- Modification in calibration file of MAVEN/SWEA

-------------------
14/02/2017 (v14.07)
-------------------
- add computation of pressure tensor gradient for MMS DES and DIS

-------------------
07/02/2017 (v14.06)
-------------------
- For MMS: new products (srvy and brst) for FGM with jmax at 5 mn resolution
- For JUNO_EPHEMERIS: XJ2000, YJ2000 and ZJ2000 are now in Rj unit (1 Rj = 71492.0 km)

-------------------
03/02/2017 (v14.05)
-------------------
- Bug correction introduced in CLUSTER and MMS current computation

-------------------
02/02/2017 (v14.04)
-------------------
- Modification for BEPI-COLOMBO
- Modif in interpolation used in current computation

-------------------
01/02/2017 (v14.03)
-------------------
- Modification for BEPI-COLOMBO
- Modif in current computation for MMS (orbit is now read all the time in srvy data)

-------------------
30/01/2017 (v14.02)
-------------------
- Modification for BEPI-COLOMBO

-------------------
27/01/2017 (v14.01)
-------------------
- Modification for BEPI-COLOMBO and MMS

-------------------
26/01/2017 (v14.00)
-------------------
- Modification for BEPI-COLOMBO
- Bug correction in time_phi spectro

-------------------
24/01/2017 (v13.84)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Modif for BEPI-COLOMBO
- Modif in MMS_FGM
- Correction in MMS current computation with FGM data

-------------------
20/01/2017 (v13.83)
-------------------
- Correction in MMS current computation with FGM data

-------------------
19/01/2017 (v13.82)
-------------------
- Correction in 'energy_pitchangle' spectro
- Add a new system plot for JASON3_AMBRE

-------------------
18/01/2017 (v13.81)
-------------------
- Correction in 'energy_pitchangle' spectro

-------------------
13/01/2017 (v13.80)
-------------------
- Modif for BEPI

-------------------
12/01/2017 (v13.79)
-------------------
- Add META DATA "EXPERIMENT", "START_TIME" and "END_TIME" in exported files when possible

-------------------
11/01/2017 (v13.78)
-------------------
- Modification of theta angles for INTERBALL-AURORAL
- Add META DATA "SC_ID" in exported files for multispacecraft project

-------------------
10/01/2017 (v13.77)
-------------------
- Add "Data display" widget in ASCII and CEF export to export for example distribution function over a time range

-------------------
09/01/2017 (v13.76)
-------------------
- Add MAVEN_SWEA calibrations until end of 2019
- Modifications for BEPI-COLOMBO MEA
- Change filename when exporting data with "data display" different than 1

-------------------
04/01/2017 (v13.75)
-------------------
- For MAVEN_SWEA: new products SVY3D, ARC3D, SVYPAD, ARCPAD and SVYSPEC in JE physical values
- For MAVEN_SWEA: huge modification in calibrations
- Modification in vector plot (automatic scale, arrow)

-------------------
24/11/2016 (v13.74)
-------------------
- Modification of quality wording in MAVEN_NGIMS

-------------------
23/11/2016 (v13.73)
-------------------
- MAVEN_SWEA calibrations uses now cc (SWEA/SWIA cross-calibration), ke (Electron suppression correction) and ff (flatfield correction)

-------------------
18/11/2016 (v13.72)
-------------------
- CDFLIB upgraded to version 3.6.3 to include Dec 31 2016 leapsecond

-------------------
16/11/2016 (v13.71)
-------------------
- Bug correction in JASON3_AMBRE
- Bug correction in JUNO_JADEE
- Correction of axes in AITOFF projection

-------------------
15/11/2016 (v13.70)
-------------------
- Modification of quality wording in MAVEN_NGIMS
- Bug correction in time_phi and phi_theta spectrogram for JUNO_JADEE
- Bug correction in time_phi spectrogram for MAVEN_SWIA and MAVEN_STATIC

-------------------
28/10/2016 (v13.69)
-------------------
- New product in MAVEN_KP: insitu_helcats at one minute resolution
- Modification for JUNO_JADEE HRS products

-------------------
26/10/2016 (v13.68)
-------------------
- JUNO_JADEE: new 3D products dynamically computed with 2D products and magnetic field

-------------------
24/10/2016 (v13.67)
-------------------
- Bug correction in moments computation for MMS_DES, MMS_DIS and JUNO_JADEE
- Optimization

-------------------
20/10/2016 (v13.66)
-------------------
- Correction for MMS_DES and MMS_DIS
- Correction for JUNO_JADEE and JUNO_JADEI
- Modification for MMS_EDI

-------------------
14/10/2016 (v13.65)
-------------------
- Modification for MMS
- Bug correction for JUNO_JADEE in background removal

-------------------
12/10/2016 (v13.64)
-------------------
- Add LONG, MLAT and IO_PHASE in JUNO_EPHEMERIS orbit files
- Add geometrical factor in JUNO_JADEE
- Bug correction for MMS_DES and MMS_DIS in 64 energies interpolation
- Add the possibility to plot JUNO_JADEE spectrogram as a fonction of LONG, MLAT or IO_PHASE

-------------------
06/10/2016 (v13.63)
-------------------
- Modification of JUNO_JADEE and JUNO_JADEI
- Correction for MMS

-------------------
03/10/2016 (v13.62)
-------------------
- Correction in JUNO_JADEE
- New format V3 for MMS_DES ans MMS_DIS (energy table are now in data files)

-------------------
21/09/2016 (v13.61)
-------------------
- Modification for MMS DES and DIS (structure of brst l2 moms)

-------------------
15/09/2016 (v13.60)
-------------------
- Modifications for JUNO JADEE and JADEI
- Bug correction

-------------------
13/09/2016 (v13.59)
-------------------
- Change data available for CLWeb MAVEN PDS users
- Modification calib of MAVEN SWEA
- Modification structure of MMS EDP files
- Modification for JUNO JADEE and JADEI

-------------------
01/08/2016 (v13.58)
-------------------
- Background can be removed for JUNO JADEE (count from one energy band)
- Add 2 widgets for magnetic field in order to average B on N sec (MAVEN/SWEA, MAVEN/SWIA, MMS/DES and MMS/DIS)
- Modification of MMS/FEEPSE and MMS/FEEPSI data files

-------------------
30/06/2016 (v13.57)
-------------------
- Add CONVECTION in AITOFF spectrogramm (symbols * for +Beam and -Beam). Parameters can be changed in Type.
- Change wording of MAVEN/SWIA L1 moments
- Bug correction

-------------------
24/06/2016 (v13.56)
-------------------
- Bug correction in MMS_DES and MMS_DIS

-------------------
23/06/2016 (v13.55)
-------------------
- Add MARS_B_CONNECTION in MAVEN tree. The 4 parameters can be changed in Type of panel composel.

-------------------
20/06/2016 (v13.54)
-------------------
- Correction of phi_theta_rotate for experiment with theta=anode (CLUSTER and MMS)
- Correction missing widgets in phi_theta for MEX/IMA and VEX/IMA
- Modifications for JASON3/AMBRE
- Modifications for JUNO/JADEE and JUNO/JADEI

-------------------
13/06/2016 (v13.53)
-------------------
- Correction in MMS DES/DIS/HPCA
- add product name in experiment for MAVEN/STATIC, MAVEN/SWIA, JASON3/AMBRE and JUNO/JADEI
- Add dynamic computation of SH in MAVEN/EPHEMERIS
- Add dynamic computation of SZA, LT and SH in MGS/EPHEMERIS

-------------------
10/06/2016 (v13.52)
-------------------
- Add widgets phi_theta_rotate and phi_theta_show_blocked_bins in Type to rotate MAVEN-SWEA phi_theta spectrogram and show blocked bins values
- Add widgets to choose velocity and potential in MAVEN-SWEA pitch_cjf plot
- Add dynamic computation of SZA_deg and LT_h in MARS-EXPRESS ephemeris
- Modifications for JASON3-AMBRE

-------------------
02/06/2016 (v13.51)
-------------------
- Change data available for CLWeb MAVEN PDS users
- New project JASON3 with EPHEMERIS and AMBRE
- New particule spectrogram energy_pitchangle
- Particle plot energy_cjf can be done for a pitchangle selection
- Modification in JUNO_EPEHEMRIS, JUNO_JADEE, JUNO_JADEI and JUNO_MAG
- Bug correction in MAVEN_SEP

-------------------
13/05/2016 (v13.50)
-------------------
- Last month of MMS data is not public in CLWeb
- Modification of MAVEN_NGIMS quality wording

-------------------
11/05/2016 (v13.49)
-------------------
- Modifcation of timeaxis in order to plot interval up to 1 millisecond (useful for MMS burst mode)
- all MMS data is now public in CLWeb

-------------------
06/05/2016 (v13.48)
-------------------
- Bug correction for MMS and CLweb

-------------------
03/05/2016 (v13.47)
-------------------
- Bug correction in dynamic computation of field abundance_total in MAVEN_NGIMS ion-abund product

-------------------
02/05/2016 (v13.46)
-------------------
- Modification for MMS_FEEPSE, MMS_FEEPSI and MMS_EIS: it's now possible to change unit: flux, JE, ...
- Correction in wording of MAVEN_NGIMS csn-abund and cso-abund: ion has been replaced by neutral
- if a super-constraint is provided then the time-table "obj.xml" is automatically created

-------------------
26/04/2016 (v13.45)
-------------------
- Add dynamic computation of field abundance_total in MAVEN_NGIMS ion-abund product
- Correction of unit (FLUX) in MMS_FEEPSE and MMS_FEEPSI
- Speed optimization when CL uses a lot of memory

-------------------
25/04/2016 (v13.44)
-------------------
- Correction of bugs introduced in v13.43 (Cluster and WebServices)

-------------------
22/04/2016 (v13.43)
-------------------
- Modification for INTERBALL
- Products of experiments are now created dynamically (only when necessary) so CL starts faster
- Modification of MAVEN_NGI (quality factor)
- Modification for MMS_HPCA (it's now possible to change unit: flux, JE, ...)
- New products MMS_HPCA burst l2 ion and moments
- Modification for MMS_DES and MMS_DIS (taking in account variation of phi angles, FGM can be used as magnetic field)
- MMS_FGM can now be used in current computation (Curlometer and fpi_nq(vi-ve))
- Magnetic field models for MAVEN is now computed for altitude lower than 3000 km
- Bug correction for MAVEN_SWEA with manual potential

-------------------
08/04/2016 (v13.42)
-------------------
- New experiments for MMS: ASPOC, DSP, EIS, FEEPSE, FEEPSI, FGM, HPCA and SCM
- Add products in MMS_EDI, MMS_EDP, MMS_MEC
- Modification for CSA: https and cookies are now used to download data

-------------------
16/03/2016 (v13.41)
-------------------
- Change data available for CLWeb MAVEN PDS users
- add JUNO_EPEHEMERIS and JUNO_MAG
- Modif in JUNO_JADEE and JUNO_JADEI to read only L3 data

-------------------
09/03/2016 (v13.40)
-------------------
- Change data available for CLWeb MAVEN PDS users
- MAVEN SWEA bias adjustment

-------------------
07/03/2016 (v13.39)
-------------------
- Add fast l2 products (dist and moms) for MMS DES and DIS

-------------------
01/03/2016 (v13.38)
-------------------
- Change data available for CLWeb MAVEN PDS users

-------------------
29/02/2016 (v13.37)
-------------------
- Add position in GSE/GSM and DIST in MMS_DFG and MMS_MEC
- Add carrington rotation number 2173-2300

-------------------
26/02/2016 (v13.36)
-------------------
- Change data available for CLWeb MAVEN PDS users

-------------------
25/02/2016 (v13.35)
-------------------
- Change products priority of MMS DES and DIS
- Change field names of MMS EDP products
- Change data available for CLWeb MAVEN PDS users

-------------------
23/02/2016 (v13.34)
-------------------
- Modif for MMS (currentie and scpot)

-------------------
19/02/2016 (v13.33)
-------------------
- New experiment MAVEN EUV

-------------------
18/02/2016 (v13.32)
-------------------
- Add l2 data files for MMS DES and DIS

-------------------
17/02/2016 (v13.31)
-------------------
- Add current computation for MMS with electron, ion and mag data

-------------------
15/02/2016 (v13.30)
-------------------
- bug correction for MAVEN_SWEA energy_cjf between T1 and T2 when Spacecraft potential is Automatic

-------------------
11/02/2016 (v13.29)
-------------------
- Correction in MAVEN_SWEA moments computation
- Add field scpot_v with spacecraft potential used in moments computation
- Energies used in 'energy_cjf' plot are automatically shifted by potential if spacecraft_potential is 'Automatic'

-------------------
10/02/2016 (v13.28)
-------------------
- Modification in potential used in MAVEN_SWEA moments computation

-------------------
09/02/2016 (v13.27)
-------------------
- FILLVAL value modification for MAVEN_LPW CDF files
- Wording correction in MAVEN_EPHEMERIS

-------------------
08/02/2016 (v13.26)
-------------------
- New experiment MAVEN NGIMS
- Bug correction in AITOFF plot
- Introduce blocked angular bins for MAVEN_SWEA
- Modification in SWEA_MAVEN 1D moments computation

-------------------
03/02/2016 (v13.26)
-------------------
- New products lpnt, l2_wspecact and l2_wspecpas for MAVEN_LPW
- New product scpot fast l2 for MMS_EDP
- For MMS: use scpot from fast_l2 if burst_l2 is unavailable
- New experiment MAVEN_SEP
- New experiment MAVEN_KP

-------------------
28/01/2016 (v13.25)
-------------------
- New experiment MAVEN_LPW
- Spacecraft potential can be use in time_energy spectro and energy_cjf plot for MAVEN_SWEA
- New products fast data (moms, dist and disterr) for MMS_DES and MMS_DIS
- Add photoelectron_correction_factor in MMS_DES 3Dmoments computation
- Bug correction when reading multiple MMS SITL CDF files

-------------------
21/01/2016 (v13.24)
-------------------
- Correction bug in Distribution function plot of MMS_DES and MMS_DIS
- New plot in MMS/TIME: mms_time_burst_all with time of burst for all spacecrafts

-------------------
20/01/2016 (v13.23)
-------------------
- Correction of a bug introduced in CLUSTER Distribution function plot
- Modification of algorithm used in time_pitchangle in Bulk frame

-------------------
19/01/2016 (v13.22)
-------------------
- Add spacecraft_potential widget in time_pitchangle for MAVEN_SWEA, MAVEN_SWIA, MMS_DES and MMS_DIS
- Bug correction (density in MAVEN_SWEA_ENGY, time_pitchangle in MAVEN_SWEA_PAD)

-------------------
14/01/2016 (v13.21)
-------------------
- Bug correction for MMS

-------------------
13/01/2016 (v13.20)
-------------------
- For MMS_DES and MMS_DIS: MAG data "dfg_brst_l2pre" or "dfg_brst_ql" can now be used in 3D moments or time_pitchangle

-------------------
08/01/2016 (v13.19)
-------------------
- Change "http://stereo.cesr.fr" by "http://clweb.irap.omp.eu" for data, calibration and software update
- Spacecraft potential can be changed in 3D moments computation of THEMIS_EESA and THEMIS_IESA

-------------------
23/12/2015 (v13.18)
-------------------
- New experiment MMS_EDP with spacecraft potential data
- New products P16 and P17 for MMS_DFG with l2pre brst data
- Current for MMS can now also be computed with l2pre brst data
- Precision of MMS data inside cl is now one micro second (instead of one milli second)
- Moments computation for MMS_DES and MMS_DIS can now use spacecraft potential from MMS_EDP

-------------------
09/12/2015 (v13.17)
-------------------
- Change clweb.cesr.fr by clweb.irap.omp.eu
- Unit correction in MMS current computation

-------------------
26/11/2015 (v13.16)
-------------------
- Evaluation of 0/x is now equal to 0 (without evaluation of x)
- Extension of start time and end time of intervals computed with constraint
- New product disterr in MMS_DES and MMS_DIS
- Correction of parameters used in 3D moments computation of MMS_DES and MMS_DIS
- Add "Produced by CLWeb" in CLWeb output

-------------------
16/11/2015 (v13.15)
-------------------
- Add plot in MAVEN/SWEA/PRODUCTS and MAVEN/SWIA/PRODUCTS
- Correction plotting data with time_table
- Set end of VENUS-EXPRESS data to 2014/12/31
- Add moments computation for MAVEN/STATIC modes CE/CF/D0/D1
- Files downloaded by WebServices are now valid only 6 days
- New experiment MMS/EDI
- Correction when reading CDF files with WARNING (ex: MMS)

-------------------
05/11/2015 (v13.14)
-------------------
- New plot available ind Add/MAVEN and Add/MMS
- Warning correction when some fields of orbit data contains STRING (ex: MMS)
- for MAVEN_MODELS: residual is now computed with MAG3 instead of MAG1
- Constraint can now be used with ".v86" files
- "Map export" is now available under CLWeb
- CLWeb ready for MAVEN_PDS users
- Bug correction in distribution function plot

-------------------
30/10/2015 (v13.13)
-------------------
- New compressed file format ".v86" for MMS_DES and MMS_DIS dist: contains only non zero values and direct access to any record is possible
- Correction in Distribution Function for MMS
- C code corrected to remove gcc warning
- Increase quality image in Postscript output
- Bug correction for phi_theta spectrogram in Postscript and CLWeb
- Reduction of character size by 25% in Postscript and CLWeb output (see Preferences/General/General Expert/Postscript charsize reduction)
- Start time with duration can now be used in CLWeb (ex: 1 10 2015 /1d)
- Start time with duration can now be used in default_start_time in Preferences/General
- Z normalized can now be used in spectrogram with time on Xaxis to normalize data at each time

-------------------
22/10/2015 (v13.12)
-------------------
- Correction in TRIANGULATE
- Correction plotting data with time_table
- Correction plotting Distribution function with TRIGRID
- Next time and Previous time depend now of "Data accumulation"
- Correction of MMS/DES energy table
- log0value and log0use widget in count3d are now invisible and automatically used with TRIGRID interpolation
- Zauto can now be used with Distribution function interpolated with TRIGRID
- Bug correction distribution function in Bulk frame

-------------------
15/10/2015 (v13.11)
-------------------
- Pitchangle in Bulk frame can be done in physical unit FLUX, JE, FDIST and FLUX_INTEGRAL

-------------------
14/10/2015 (v13.10)
-------------------
- Minor corrections

-------------------
13/10/2015 (v13.09)
-------------------
- Add some parameters in 3D moments computation for MMS DES and DIS

-------------------
13/10/2015 (v13.08)
-------------------
- Optimization for pitchangle computation in Bulk frame
- cl is now definitively unsupported under Windows 32 bits

-------------------
09/10/2015 (v13.07)
-------------------
- Add Bavg in MAG3 MAVEN MAG
- Add quality_index_2 in 3D moments MAVEN SWEA (SC_POT available or not)
- MAVEN SWIA pitch-angle are now done in Bulk frame
- Pitchangle in Bulk frame can be done only for fdist unit

-------------------
08/10/2015 (v13.06)
-------------------
- Bug correction in MMS DIS energy table
- Bug correction for time_pitchangle in Bulk frame

-------------------
07/10/2015 (v13.05)
-------------------
- Bug correction for time_pitchangle in Bulk frame

-------------------
06/10/2015 (v13.04)
-------------------
- New product for MAVEN MAG: MAG3 at 1 sec (calibrated) or 2 sec (uncalibrated) resolution
- Add pitchangle for MAVEN SWIA and MAVEN STATIC
- Add some predefined plots in Add/MMS/OTHER

-------------------
02/10/2015 (v13.03)
-------------------
- CDFLIB upgraded to version 3.6 to include June 30 2015 leapsecond
- Add data files with time of burst in dist and moms for MMS_DES and MMS_DIS
- Add predefined plot mms_des_time and mms_dis_time in Add/MMS
- Add widget Amin and Amax to select pitchangle in time_energy spectrogram
- Add current computation for MMS
- Add unit of fields computed in current
- Add srvy l2pre data in MMS_DFG
- All files for MMS_DES, MMS_DIS and MMS_DFG are now in uncompressed binary format (".x86") in /DATA/MMS/DATA/CL
- Bug correction when seeking files larger than 4G on Windows

-------------------
25/09/2015 (v13.02)
-------------------
- Plots are available in Add/JUNO
- Possible bug correction with THETA and PHI angles

-------------------
23/09/2015 (v13.01)
-------------------
- Server defined in General "HTTP server" is now used for data and software update
  (The value "aspera.cesr.fr" is automatically replaced by "stereo.cesr.fr")
- Bug correction in pitchangle in bulk frame for MMS (energies in ascending order)
- Use electron bulk-velocity vector GSE from des-moms to compute MMS_DES brst pitchangle in bulk frame
- Use ion bulk-velocity vector GSE from dis-moms to compute MMS_DIS brst pitchangle in bulk frame

-------------------
22/09/2015 (v13.00)
-------------------
- Add unit "fdist->flux", "fdist->integral_flux", "fdist->fdist" and "fdist->JE" for MMS_DES and MMS_DIS (computed from fdist)
- Modification for MMS_DES and MMS_DIS
- Modifcation of timeaxis in order to plot interval less than 1 seconde (useful for MMS burst mode)
- Bug correction in Distribution Function plot (energies in ascending order for MMS)
- Add the possibility to use spacecraft potential in CLUSTER-HIA 3D moments computation
- Add experiments MMS_MEC and MMS_FPI
- MMS burst data files for DES, DIS and DFG are now in ".X86" format (uncompressed binary files)
- Add interpolated 64E product (computed from 32E product) for MMS_DES and MMS_DIS
- Informs at startup Windows and Mac users if a new cl is available

-------------------
10/09/2015 (v12.48)
-------------------
- Bug correction when reading SWIA moments
- Bug correction in DMETER_IDP 3 energy band definition
- Add experiments DES, DIS and DFG for MMS

-------------------
22/07/2015 (v12.47)
-------------------
- Add the possibility to export 2D Distribution function data

-------------------
09/07/2015 (v12.46)
-------------------
- bug correction

-------------------
08/07/2015 (v12.45)
-------------------
- bug correction

-------------------
08/07/2015 (v12.44)
-------------------
- MAVEN_SWIA and MAVEN_STATIC: add export "map" for phi_theta spectrogram to obtain a phi_theta in MSO coord
- MAVEN_SWIA and MAVEN_STATIC: phi_theta spectrogram display theta and phi angle in MSO at mouse position
- MAVEN_SWIA and MAVEN_STATIC: variable cjf in data is automatically changed when a new product is selected
- MAVEN_STATIC: new plot mass_cjf (can also be used between t1 and t2)
- MAVEN_EPHEMERIS: new product STATIC_MSO with transformation matrix from MAVEN_STATIC to MAVEN_MSO frame (1 sec resolution)
- MAVEN_EPHEMERIS: new product SWIA_MSO with transformation matrix from MAVEN_SWIA to MAVEN_MSO frame (1sec resolution)
- MAVEN_SWIA: deflection angle in 3D data file is now a fonction of time, energy and deflection number
- MAVEN_STATIC: 4D data file are now in binary format, header in ascii (reading is much faster)
- MAVEN_SWIA: 3D data file are now in binary format, header in ascii (reading is much faster)
- Add schematics for MAVEN_STATIC and MAVEN_SWIA
- MAVEN_SWIA: 3D moments computation and distribution function use deflection angle as a function of time, energy and deflection number

-------------------
24/06/2015 (v12.43)
-------------------
- Bug correction when loading time_table
- Bug correction when plotting time_theta, time_phi, time_mass and time_pitchangle spectrogram with time_table

-------------------
23/06/2015 (v12.42)
-------------------
- Modif experiment data right access for Clweb
- Update of MAVEN_SWEA calibration file
- Compute B magnitude for MAVEN PC SS and PL files
- MAVEN_SWEA: export "map" in phi_theta spectrogram to obtain a phi_theta in MSO coord
- energy_cjf plots: can now be used between t1 and t2
- MAVEN_SWEA: correction to obtain correct JE (cross-correlation SWEA/SWIA)
- MAVEN_SWEA: phi_theta spectrogram display theta an phi angle in MSO at mouse position
- MAVEN_SWIA: new products for SWICS, SWICA, SWIFS, SWIFA and SWIS with all Energies, Deflections and Anodes in different physical units (idem MAVEN_STATIC)

-------------------
16/06/2015 (v12.41)
-------------------
- FOR MAVEN_MAG: add 3 products at 1 sec resolution MAGPC1SEC, MAGSS1SEC and MAGPL1SEC

-------------------
15/06/2015 (v12.40)
-------------------
- Add some plots for SWEA under Add/MAVEN/SWEA
- bug correction

-------------------
12/06/2015 (v12.39)
-------------------
- Add spacecraft_potential and bulk_velocity widget in time_pitchangle for MAVEN SWEA (uses Bulk frame now)
- Bugs correction

-------------------
10/06/2015 (v12.38)
-------------------
- Add experiments jadee060, jadee180, jadee300, jadei and all for JUNO
- Bug correction when printing

-------------------
04/06/2015 (v12.37)
-------------------
- For MAVEN_MAG: add 3 high resolution products MAGPCFULL, MAGSSFULL and MAGPLFULL
- Add schematic for MAVEN_SWEA

-------------------
01/06/2015 (v12.36)
-------------------
- Modif X,Y,Z axes of MAVEN_SWEA in the code
- Bug correction in mass_energy plot of MAVEN_STATIC

-------------------
29/05/2015 (v12.35)
-------------------
- Modif for MAVEN_STATIC: add plots "mass_energy", "phi_theta" and "distribution function"

-------------------
17/05/2015 (v12.34)
-------------------
- Modif for MAVEN_STATIC:
  * MASS and DEFLECTION are now time dependant in data files
  * Add products (except for QL) in physical units: c/s, flux, JE and fdist
- Modif for MAVEN_MODELS: add Br in map

-------------------
07/05/2015 (v12.33)
-------------------
- Correction loop intervall timetable
- Modification tree MAVEN STATIC

-------------------
06/05/2015 (v12.32)
-------------------
- MAVEN MAG MODEL Purucker has been replaced by Morschhauser
- Correction for MAVEN STATIC

-------------------
04/05/2015 (v12.31)
-------------------
- Correction for compilation under Solaris

-------------------
30/04/2015 (v12.30)
-------------------
- Add definitions for product MAVEN/STATIC mvn_sta_C6_P1D

-------------------
28/04/2015 (v12.29)
-------------------
- Modification of MAVEN/SWEA counts 19 to 8 bits decompression (middle of each range)
- Add for MAVEN/SWEA bias adjustment (2500 -> 2600 V) after 2014-10-17/2:26:41 (efficencies have to be multiplied by 1.5)

-------------------
27/04/2015 (v12.28)
-------------------
- Removal of check for software update stable

-------------------
24/04/2015 (v12.27)
-------------------
- Add Br, Bt, Bp in MAVEN_MAG and MAVEN_MODELS
- Modifications in MAVEN SWEA 3D moments

-------------------
10/04/2015 (v12.26)
-------------------
- Modificaions for MAVEN SWIA

-------------------
09/04/2015 (v12.25)
-------------------
- Correction for IMPEX FMI_GUMICS

-------------------
08/04/2015 (v12.24)
-------------------
- New product P12 for MAVEN_SWIA (on board moments)
- Use VSWIA in SWEA coord in SWEA 3D moments computation
- Correction for IMPEX

-------------------
27/03/2015 (v12.23)
-------------------
- corrections

-------------------
25/03/2015 (v12.22)
-------------------
- cl now runs under windows 64 bits

-------------------
20/03/2015 (v12.21)
-------------------
- memory usage optimization for MAP export

-------------------
18/03/2015 (v12.20)
-------------------
- Add option MAP export to create "map.x86" with epoch, lat, long and the field plotted in one panel
- Use by default spacecraft potentiel in moments computation of MAVEN SWEA
- New product P7 for MGS: omnidirection flux for ER experiment
- RLONG_RLAT spectrogram can be used for MAVEN, MGS et "map.x86"

-------------------
06/02/2015 (v12.19)
-------------------
- Add experiment rosina rtof
- Add fields MARS, MPB and BS in MAVEN EPHEMERIS ORBIT
- Add plot maven_ephemeris_orbitXY

-------------------
26/01/2015 (v12.18)
-------------------
- Add local time computation in MAVEN EPHEMERIS
- MSO components are now in MAVEN MAG data files
- Add quality_flag and decom_flag for MAVEN SWIA
- Modif for Cef ROSINA files

-------------------
21/01/2015 (v12.17)
-------------------
- Add matrix file to transfer SWEA to MSO frame
- Add longitude and latitude for MAVEN in orbit file
- Add dynamic computation of B in MSO for MAVEN
- Use 3389.1km for Mars radius for MAVEN
- Add wording for MAVEN STATIC

-------------------
14/01/2015 (v12.16)
-------------------
- New experiments IDEEZ, IDEEN and XGRE for TARANIS
- Correction for EPOCH16 and TT2000 in CDF
- If necessary precision of time on cl can be microsecond instead of millisecond (but it's impossible to get nano and pico second)

-------------------
04/12/2014 (v12.15)
-------------------
- Bug correction

-------------------
26/11/2014 (v12.14)
-------------------
- Removing right access to ASPERA4-MAG 1sec resolution because these data are available at ftp://psa.esac.esa.int

-------------------
25/11/2014 (v12.13)
-------------------
- 6 last months of data for guest account are now blocked by default for MARS-EXPRESS, VENUS-EXPRESS
- 9 last months of data for guest account are now blocked by default for CLUSTER

-------------------
18/11/2014 (v12.12)
-------------------
- Modification in cl auto-install for Unix

-------------------
13/11/2014 (v12.11)
-------------------
- Bug correction in MAVEN data tree

-------------------
07/11/2014 (v12.10)
-------------------
- Change USERNAME in CSA data streaming request

-------------------
06/11/2014 (v12.9)
-------------------
- CAA tree removal
- Implementation of CSA data streaming with generic user ccl
- Bug correction in installation of new version of cl
- Duration of intervall can now be added at the end of start time (ex: ' /1d' for one day). Usage: /n[smhd], not case sensitive

-------------------
03/11/2014 (v12.8)
-------------------
- Modification for MAVEN-STATIC

-------------------
23/10/2014 (v12.7)
-------------------
- Add STATIC for MAVEN

-------------------
20/10/2014 (v12.6)
-------------------
- Add SWIA for MAVEN
- Optimization execution time for spectrogram in cef format

-------------------
14/10/2014 (v12.5)
-------------------
- Add ephemeris/orbit for MAVEN

-------------------
13/10/2014 (v12.4)
-------------------
- Add attributs "size" and "display" for spectrogram in clweb tree (for AMDA)
- NCDF output of webservice for vector contains now a vector instead of components (for AMDA)

-------------------
09/10/2014 (v12.3)
-------------------
- Add MEA1 and MEA2 for BEPI-COLOMBO
- Modification for MAVEN-SWEA
- Modif for IMPEX

-------------------
23/06/2014 (v12.2)
-------------------
- Modification for MAVEN-SWEA.

-------------------
27/05/2014 (v12.1)
-------------------
- Modif plugin_caa
- Add plugin_csa

-------------------
26/05/2014 (v12.0)
-------------------
- Modif for MAVEN-SWEA
- Add VEX MAG 1sec resolution

-------------------
18/04/2014 (v11.31)
-------------------
- Bug correction in profiler output

-------------------
08/04/2014 (v11.31)
-------------------
- Bug correction

-------------------
07/04/2014 (v11.31)
-------------------
- Remove unused declarations in IDL and C code.

-------------------
20/03/2014 (v11.31)
-------------------
- Bug correction for RLONG_RLAT plot for "c/s_TARANIS"
- Bug correction auto install cl

-------------------
19/03/2014 (v11.31)
-------------------
- Bug correction

-------------------
17/03/2014 (v11.31)
-------------------
- Modification for IMPEX

-------------------
13/03/2014 (v11.31)
-------------------
- Add "c/s_tararnis" in cjf for DEMETER-IDP

-------------------
07/03/2014 (v11.30)
-------------------
- For non Windows plateform: "Help/Check for software update" can now download and install new release in /DATA/CLUSTER/SOFT

-------------------
05/03/2014 (v11.29)
-------------------
- Bug correction for ASPERA3-ELS in mode 32 energies (bug in energy table)

-------------------
03/03/2014 (v11.28)
-------------------
- cl Web Service now produces files "data".extension instead of parameter.extension
- Add orbit for all experiment in WebService
- New experiment "MAVEN-SWEA"
- Metadata modifications

-------------------
10/02/2014 (v11.27)
-------------------
- Bug correction (XML,Webservice,gse->gsm(),IMPEX tree)
- Metadata correction
- Cookies used by dynatree in CLWeb are now destroyed at the beginning of the session

-------------------
06/02/2014 (v11.26)
-------------------
- Add CLUSTER in webservice
- Correction for STEREO/SEPT
- Bug correction

-------------------
04/02/2014 (v11.25)
-------------------
- Add DOUBLESTAR1 in webservice

-------------------
03/02/2014 (v11.24)
-------------------
- Add SACC, INTERBALL-AURORAL, SACC and STEREO in webservice
- Correction special character in xml files

-------------------
31/01/2014 (v11.23)
-------------------
- Add WIND tree in webservice
- Correction for WIND WI_H1_SWE

-------------------
30/01/2014 (v11.22)
-------------------
- Correction for GEOTAIL spectrogram
- Add GEOTAIL tree in webservice
- Add target in clweb_tree.xml
- gse_to_gsm() works now for data before 2000

-------------------
29/01/2014 (v11.21)
-------------------
- It's no longer possible to use CLUSTER magnetic field at 1 sec resolution (this dataset is not produced since end 2009)
  All configs with this resolution will automatically use 4 sec resolution.
- "impex://" has been removed in filename for master and data file

-------------------
23/01/2014 (v11.20)
-------------------
- New spectro available X="Day of CR" and Y="Carrington Rotation" for a field found a a timeseries file (ex: Qr in STEREO-SWEA precomputed MOM file)

-------------------
15/01/2014 (v11.19)
-------------------
- cl can now read CDF files with time in CDF_TIME_TT2000 type (ex: GOES15 and RBSP in CDAWeb)
  In case of pb please install CDF Patch for IDL 6.2 and later at http://cdf.gsfc.nasa.gov/html/cdf_patch_for_idl.html

-------------------
10/01/2014 (v11.18)
-------------------
- bug correction (not necessary for CLUSTER) in some vector components computed in 3Dmoments in GSE, GSM, RTN frame (ex: Qrtn for STEREO-SWEA)
- components of vector selected in tree will be red-green-blue, even for 3D moments object

-------------------
11/12/2013 (v11.17)
-------------------
- add LESIA dataset in IMPEX tree
- add <DESCRIPTION> tag of VOTABLE in wording of each field
- add CSA tree

-------------------
12/11/2013 (v11.16)
-------------------
- bug correction for bulk_speed in 'Distribution Function'

-------------------
28/10/2013 (v11.15)
-------------------
- bug correction (Xaxis in HEADER)
- first implementation of SINP calculateDataPointValue_Spacecraft for IMPEX

-------------------
25/10/2013 (v11.14)
-------------------
- bug correction
- new IMPEX trees
- output files for DEMETER are created with energy table in meta data

-------------------
19/09/2013 (v11.13)
-------------------
- Correction of Methods_CLWEB.wsdl
- Correction of exp_plugin_caa

-------------------
27/08/2013 (v11.12)
-------------------
- Bug correction

-------------------
08/08/2013 (v11.11)
-------------------
- New experiment LIGHTNING
- Add POES and LIGHTNING data in tree
- Use method getDataPointValue_Spacecraft for FMI/IMPEX

-------------------
15/07/2013 (v11.10)
-------------------
- New plot velocity_cjf_hia_low_g.cl
- Use method getDataPointValue_Spacecraft for LATMOS
- Add experimental TARANIS data in tree
- Add type CDF_INT8
- Correction when reading AMDA VOTABLE files in WebService

------------------
01/07/2013 (v11.9)
------------------
- Add option in general/Expert for STEREO-SWEA to compute efficencies below 50 eV

------------------
26/06/2013 (v11.8)
------------------
- Add Xaxis button with 'E' our 'V' in energy_cjf plot to obtain velocity_cjf or energy_cjf plot
- Correction for DEMETER-IDP mode with 3 energies

------------------
11/06/2013 (v11.7)
------------------
- Add DEMETER in WebService getParameter

------------------
03/06/2013 (v11.6)
------------------
- Bug correction with superimposed panels and Yleft 'Automatic'

------------------
30/05/2013 (v11.6)
------------------
- Shortcuts available in CLWeb

------------------
29/05/2013 (v11.5)
------------------
- Panels with Yleft 'Automatic' are now correctly superimposed

------------------
15/05/2013 (v11.4)
------------------
- Integration of webservice GetFileURL for IMPEX LATMOS

------------------
06/05/2013 (v11.3)
------------------
- Correction for THEMIS IESA modes 'peif_176x16' and 'peir_176x16'
- bug correction for DEMETER spectro L_energy

------------------
02/04/2013 (v11.2)
------------------
- Export possible for SPECTRO in VOTABLE format
- Read possible in compressed VOTABLE format

------------------
25/03/2013 (v11.1)
------------------
- New data POESN17
- Read possible in VOTABLE and NCDF
- Export possible in NCDF
- Export possible in VOTABLE (not for spectrogram)
- Data downloaded from CAA, AMDA and CLWEB are considered valid one week only
- AMDA tree now availaible in cl
- INTERBALL-TAIL data available in CL WebService
- Continents can be plotted with isocontours
- News files ".x86" contains natif binary data created under x86 Linux
- Bug correction with values of energy,theta and phi in Tools

----------------
19/02/2013 (v11)
----------------
- New experiments SWIDA and SWIDB from Chang'E-2 spacecraft

- Background contamination of THEMIS_IESA can be removed (with 4 parameters in Data)

- Data tree contains datasets available for plotting at CDAWeb and CAA, and some mirror datasets available at IRAP.
  For each dataset, variables are inside "Timeseries", "Particle spectrogram" and "Particle plot" (and "Orbit" for ephemeris).

  Panel spacecraft number for these datasets can be changed for CLUSTER, THEMIS and STEREO.

  Data files are downloaded in "$LOCAL_DIRECTORY/downloads_cl" (if this directory can be created) or "$HOME/downloads_cl"
  $LOCAL_DIRECTORY is defined in Preferences/General.
  Please use $LOCAL_DIRECTORY/downloads_cl in order to share files files between different users (mode of this directory must be "o+w" under Unix)

- Data tree branch 'SPECIAL' offers the possibility to display an external ASCII, CEF or CDF file in a panel Timeseries,
  Particle spectrogram, Particle plot or Orbit

- Yleft of each panel: Wording and Unit can be used to display on Y axis wording and unit

- Data of each panel: Wording and Unit can be used to display on top of the panel wording and unit

- New "Label" button: to display/undisplay wording and unit on top of each panels

- Correction for THEMIS_EESA and THEMIS_IESA: on board moments can be used in VB objects (see new entries in CL/THEMIS tree)

- For filename in ASCII_CEF_CDF, it's possible to use:
   $YEAT		=> year on 2 digits
   $MONTS		=> month replaced by month 01 or 07 (before or after july)
   {MULTIDAY:xxx}	=> if filename can contains xxx days of data

- Read more efficiently Rvar of CDF files (eg: old CDAWeb datasets)

- Bug correction for CEF files larger than 2GB

- No longer forces 32 bits compilation under MacOS

- Uses CDF library v3.4.1

- CDF output is possible for spectrogram. So it's possible to export in ".asc", ".cef" and ".cdf"

- Mouse middle click writes on terminal X position, Y position and YMIN, YMAX and YAVG of each plots

- Button "T1T2": it's possible to select "start time"+"end time" or a "carrington rotation number"

- Buttons "TIME->" and "<-TIME":
    - change panels to next/previous month if interval time is exactly one month
    or change panels to next/previous year if interval time is exactly one year
    or change panels to next/previous carrington rotation number if "start time" and "end time" is exactly a carrington rotation period
    or change panels to next/previous time intervall
    - can be used on a panel composer even if "start time" and "end time" are not in global properties

- For batch mode, it's possible to specifiy output in ASCII, CEF or CDF in batch file with the following options:
	* for ASCII with " Ascii           =       1"
	* for CEF   with " Cef             =       1"
	* for CDF   with " Cdf             =       1"

- New product for INTERBALL-TAIL-ELECTRON: 2D16E with data from Mode 8 (only one anode, 16 energies, 16 phis)

- Bug correction for B components in GSE in 3D moments computation.

------------------
03/09/2012 (v10.6)
------------------
- Modifications for DEMETER IDP Proton

------------------
24/07/2012 (v10.5)
------------------
- Modifications for TimeTable

------------------
12/07/2012 (v10.4)
------------------
- New widget "Use Eproton" for DEMETER-IDP in count2d and count3d (to use Proton energy table and calibration)

------------------
11/07/2012 (v10.4)
------------------
- New physical unit: integral flux
- Bug correction

------------------
02/07/2012 (v10.3)
------------------
- Bug correction in some Mars-Express predefined plots
- Add widget 'one count level' in count3d and 'count2d' to force all raw count to 1

------------------
22/06/2012 (v10.2)
------------------
- Bug correction in Postscript Distribution Function output using contour

------------------
21/06/2012 (v10.1)
------------------
- Bug correction
- Widgets modifications
- Add some plots in the tree
- Add Eproton for DEMETER IDP in time_energy count3d

------------------
07/06/2012 (v10.0)
------------------
- New tree selection
- Modification for CLWeb

------------------
30/03/2012 (v9.04)
------------------
- New "ACE" products: "ac_ko_mfi" and "ac_h3_mfi"
- New "WIND" products: "w1_h2_mfi", "w1_k0_swe" and "wi_elpd_3dp"

------------------
14/03/2012 (v9.03)
------------------
- bug correction

------------------
21/02/2012 (v9.02)
------------------
- bug correction
- Add experiments ION1CH1 ION1CH2 ION2CH1 and ION2CH2 for INTERBALL-AURORAL

------------------
20/12/2011 (v9.01)
------------------
- bug correction
- Add orbit product for experiments ELEC1CH1, ELEC1CH2, ELEC2CH1 and ELEC2CH2 of INTERBALL-AURORAL

------------------
06/12/2011 (v9.00)
------------------
- New experiments ELEC1CH1, ELEC1CH2, ELEC2CH1 and ELEC2CH2 for INTERBALL-AURORAL
- New mass positions and energy table for IMA MARS-EXPRESS
- New 'experimental' button in IHM to check and correct the plot
- New 'experimental' button in IHM to show in the plot why there is no data in some panel
- New 'experimental' button in IHM to display meta-data, search data and plot them
- New spacecraft available in SC BUTTON (used GOES13 GOES14 GOES15)
- New 'Loop interval' menu for time-table to successively plot data for each interval found in time-table
- Meta data in cef files:
  * header/count2d time-series plot: meta-data Name and Unit are used to label Yaxis (only if 'Wording' and 'Unit' are checked in Yleft menu)
  * count3d spectrogram: meta-data are used to label Yaxis (Name + Unit) and Zaxis (Name)
- Can read and display cef/cdf files with 5D variable (time,theta,phi,energy,masse). This is necessary for IMA experiment
- Add cross-correlation button in timeseries plot
- SC button can now be used all the time on any panel
- Yellow color is not any more in the 8 default colors used in timeseries plot
- The last directory used when loading file is now memorised
- Correction in Ascii export:
  * 'selection asc':  used for timeseries and 'old format' for spectrogram
  * 'selection cef':  write displayed spectrogram of type time_theta, time_phi, time_energy or time_pitchangle data in cef format
  * 'selection mini': idem in a more simple ascii format
  * 'all cef':        write all spectrogram data of type 'time_energy' or 'time_pitchangle' (for each theta/phi/energy/mass or pitchangle/energy) in cef format
  * 'all mini':       idem in a more simple ascii format

------------------
07/06/2011 (v8.24)
------------------
- New menu "Actions/Clean cache" available in clweb

------------------
01/06/2011 (v8.23)
------------------
- bug correction
- new plot 'aspera3_ima_clean' and 'aspera4_ima_clean'
- Modification of ZLIB symbols names because IDL8.0 redefines incorrectly some zlib functions()

------------------
28/04/2011 (v8.22)
------------------
- For imported ASCII/CEF/CDF: PROPERTY, FIELDNAM and UNITS can be used to label axis
	- in Header, Ascii and Cdf timeseries plot: FIELDNAM and UNITS can be displayed in Yleft axis (see checkboxes Wording,Unit)
	- in count2d plot (of type 'time_cjf' or 'energy_cjf'): FIELDNAM and UNITS can be displayed in X and Yleft axis and Legend
	- in count3d plot (of type 'time_energy', 'time_theta' or 'phi_theta'): PROPERTY can be displayed in color palette, FIELDNAM and UNITS can be used in X and Yleft axis
- NEW experiment: Omni data from cdaweb at 1hr, 5min and 1min resolution
- Bug correction in Yleft/Wording and Yleft/Unit
- cl now manages files that change every month or year (eg: one file per month for Omni data)
- Bug correction in ascii files plot (color, load/save, ...)

------------------
18/03/2011 (v8.21)
------------------
- Correction in MacOSX library creation

------------------
11/03/2011 (v8.20)
------------------
- Bug correction
- New product STEREO-SWEA P30: precomputed MOM files in CEF format

------------------
02/03/2011 (v8.19)
------------------
- Bug correction
- New product STEREO-SWEA P29: magnetic field 1mn resolution

------------------
25/02/2011 (v8.18)
------------------
- silence option in get_http_file
- bug correction in export ascii file for a panel with constraint
- New version of MAGLIB used inside cl (includes coefficients for 2010-1014)

------------------
25/01/2011 (v8.17)
------------------
- Optimization for Help/Check for data update, display number of files incorrectly downloaded

------------------
20/01/2011 (v8.16)
------------------
- New product for WIND: P17="H5_SWE     Electron moments 6-15 sec resolution"

------------------
19/01/2011 (v8.15)
------------------
- New unit 'flux_algo' for DEMETER-IDP (flux correction by Thomas Moreau)

------------------
06/01/2011 (v8.14)
------------------
- Add and compute GSM magnetic field components when reading CAA FGM cef files
- New product for WIND: P16=magnetic field 3sec resolution
- To build cl under MacOSX: "genere.sh -gcc -m32 all" works fine now

------------------
23/12/2010 (v8.13)
------------------
- Correction for MacOs compilation (compilation ok for 32 bits)
- PNG output is possible in batch mode (Nomps = PNGval, PNG100 for example)
- Correction for STEREO-PLASTIC spectrogram with 'FACTOR' product

------------------
09/12/2010 (v8.12)
------------------
- When STEREO-SWEA is in test mode (janv_fen 2009), physical values are not computed
- 'PNG video' can be used to generate any plot of duration sec between t1 and t2
- Bug correction for STEREO 'SC3' and 'SC4' 

------------------
01/12/2010 (v8.11)
------------------
- Bug correction in PAD spectrogram
- New option 'PNG Video' in Print menu (to obtain for example all distributions function plots between t1 and t2)
- Virtual spacecraft SC3 and SC4 can also be used for PLASTIC data

--------------------
11/10/2010 (v8.10.2)
--------------------
- New virtual spacecraft for STEREO:
  * SC3 = Behind at Ahead position
  * SC4 = Ahead at Behind position

--------------------
05/10/2010 (v8.10.1)
--------------------
- Add On-Board moments for THEMIS EESA and IESA
- Bug correction for clweb

------------------
07/09/2010 (v8.10)
------------------
- Skip moments computation when STEREO-SWEA is in test mode
- user "clweb.." can use clweb with reduced dataset

-------------------
26/08/2010 (v8.9)
---------------------
- New mode for THEMIS ESA: 'eef_088x15', 'eif_176x16' and 'eib_176x16'
- Correction for STEREO-SEPT: description of spectro are not the same for Ahead and Behind spacecraft

-------------------
11/06/2010 (v8.8)
---------------------
- STEREO PLASTIC Spectrogram

-------------------
01/04/2010 (v8.7.2)
---------------------
- Correction for STEREO SEPT
- New experiment STEREO SIT
- Cleanup in STEREO SWEA products

---------------------
18/03/2010 (v8.7.1)
---------------------
 - A mathematical expression function of TABY can now be used in count2d object (ex: TABY/300)
 - sol7 is now all the time used for STEREO SWEA
 - new products for STEREO_SWEA: P26(core cal), P27(core13ev) and P28(core13ev cal)

---------------------
15/03/2010 (v8.6.9)
---------------------
 - Bug correction for CO2+ and H+ particule line position of ASPERA3 (lines not displayed)

---------------------
10/03/2010 (v8.6.8)
---------------------
 - cl can now plot time_pitchangle spectrogram for IMA/VEX

---------------------
08/03/2010 (v8.6.7)
---------------------
 - cl now uses STEREO magnetic field files 'L1_MAG_SC' and 'L1_MAGB_SC' found in l1data directory
 - moments computation now includes 'B' in different frame used in this routine

---------------------
04/03/2010 (v8.6.6)
---------------------
 - bug correction when plotting ascii file

---------------------
02/02/2010 (v8.6.5)
---------------------
 - bug correction when reading ascii file created under Linux and transfered under Windows by ascii ftp

---------------------
19/01/2010 (v8.6.4)
---------------------
 - theta angles correction in Double-Star distribution function plot

---------------------
22/12/2009 (v8.6.3)
---------------------
 - Yleft: more than one value can now be specified in 'Line for X=' (number of second since start time)
 - PEACE CAA_CDF: use new files '3DRH' and '3DRL' instead of old files 'CP3DRH' and 'CP3RDL'
 - bug correction

---------------------
10/12/2009 (v8.6.2)
---------------------
 - Amelioration in wget.pro

---------------------
20/11/2009 (v8.6.1)
---------------------
 - Optimization when plotting several months of ELS data (for both MEX and VEX)
 - bug correction

---------------------
15/10/2009 (v8.5.9)
---------------------
 - Z_axis can be "Normalized". Normalization is done for each record. Usefull for STEREO/PAD
 - bug correction when plotting several years of IMA data

---------------------
14/09/2009 (v8.5.8)
---------------------
 - STEREO/SWEA MAG: cl uses now only V03 of 'new' short format and computes components in rtn frame
 - bug correction in file_http_copy: directory listing is sometimes chunked by http server so some files were skipped

---------------------
19/08/2009 (v8.5.7)
---------------------
 - NPI for ASPERA3 and ASPERA4: bug correction in validity duration of the data
 - STEREO/MAG: cl uses now new format without values in Rtn frame

---------------------
25/06/2009 (v8.5.6)
---------------------
 - STEREO/SWEA: new plot SPIN/PAD in bulk frame
 - STEREO/SWEA: new plot moments3d_andrea_correction (core)
 - STEREO/PLASTC: one plot added

---------------------
18/06/2009 (v8.5.5)
---------------------
 - Check for data update: bug correction in base64 source code for login/password
 - Check for data update: use now protocol HTTP/1.1 instead of HTTP/1.0
 - STEREO/SWEA uses old energy table from April 16 2009

---------------------
02/06/2009 (v8.5.4)
---------------------
 - New MAG files for ASPERA4 (with new filenames)
 - bugs correction

---------------------
19/05/2009 (v8.5)
---------------------
  - ready to create plots on CESR STEREO SWEA web server
  - clweb ready

---------------------
12/03/2009 (v8.4)
---------------------
  - load INCLUDE files defined in metadata of CEF-2.0 files
  - bug correction for SWEA and INTERBALL (plot compressed count in count/energy plot)

---------------------
11/03/2009 (v8.4)
---------------------
  - bug correction with get data by http
  - cl produces similar header in CEF-2.0 output for both timeseries and count3d
  - sol7 for STEREO-SWEA

---------------------
10/03/2009 (v8.4)
---------------------
  - rtn components computed for SWEA3D  moments
  - Qpar and Qper computed in 3D moments
  - bug correction in heat flux computation in 3D moments
  - cef export produces now ascii file in CEF-2.0 format insted of CEF-1.0

---------------------
20/02/2009 (v8.4)
---------------------
  - bug correction
  - New menu Time_Table (time_table in xml format)
  - New keyword Time_Table in batch file to loop for each time interval of time table
  - 3D Moments: computation of (Ppar_b,Pper1_b,Pper2_b) and (Tpar_b,Tper1_b,Tper2_b) in MAG frame
  - 3D Moments fields depend on experiment (add RTN frame for STEREO_SWEA)

---------------------
22/01/2009 (v8.4)
---------------------
  - correction for wildcard in animation filename
  - add views for themis_thg

---------------------
16/01/2009 (v8.4)
---------------------
  - bug correction
  - reads STEREO KHP in L1_CDF directory instead of l1data

---------------------
15/01/2009 (v8.4)
---------------------
  - TABY in 3D moments: it's possible to compute for example TPar/Tper1
  - header and ascii object can now read both CEF and CDF files and
    $YYYYMMDD, $YEAR, $MONTH, $DAY, $DOY, $HOUR, $MINUTE, $SECOND, $SC can be used to plot more than one day
  - optimization for (phi,theta) spectrogram
  - 64 bits ready
  - NEW CLUSTER_PEACE experiment (data from CAA in CDF format)
  - Theta and Phi have been added to Tools menu
  - Can plot data before 1958
  - Datation correction for STEREO-SWEA and THEMIS
  - VB object can now be used for THEMIS
  - ACE: new product pitchangle
  - STEREO-SWEA: distribution function in Bulk frame
  - STEREO-SWEA: new products distribution 1Ax88E and HK
  - Magnetic field for VEX: compute now Pm_nPa
  - cl can produce 1D, 2D, 3D ascii output in standard or CEF-2.0 format
  - Inside cl, data and calibration can be downloaded at http://aspera.cesr.fr (login/password required)
  - cl can quickly read any CEF-2 files (as timeseries and spectrogram)
  - cl can be installed in $CL_ROOT (by default, $CL_ROOT=$CIS_ROOT/SOFT/CLL3)
  - New experiment 'plugin_caa' using description file resource/plugin_caa.txt
  - In time_pitchangle, Emin and Emin can be specified as i[0..nbenergies-1] (ex: i0 and i1 to select the 2 higher energies)
  - Compute 3Dmoments in MSO for MEX and VSO for VEX
  - New geometrical factor for MEX (H+ and not H+)
  - Experimenent are now alphabetically sorted in General and Add menu
  - New theta angles for STEREO-SWEA (0.625 deg error)
  - For Win32, read './cl.cfg' instead of '/cl.cfg' (because of Windows Vista security)
  - Bug correction for ASCII and CDF panel with global 'Experiment' or 'Products'
  - Bug correction for the last energy step of CODIF RPA mode
  - cl.exe -> cl.ivm
  - Bug correction with cef RPA CIS file
  - check for new cl version available on http://interball2.cesr.fr:8001/software
  - cl nows auto-backup each plot in 'cl_autobackup_*.cl' files and destroy them at the end of the session (usefull in case of crash)
  - Number of PAD bins for time_pitchangle can be now choosen in Type menu (8 by default, instead of 180)
  - New products 'ser_006' and 'seb_064' for THEMIS-ESST and 'sir_006' for THEMIS-ISST
  - New experiment STEREO_PLASTIC with 2 products Proton_Bulk at 1mn and 10mn resolution
  - Coefficient sin(65) in density computation for STEREO-SWEA
  - New energies table for STEREO-SWEA in Feb 2008
  - New STEREO-SWEA plot for Web server
  - Spacecraft_potential in moments computation can be manual or automatic
  - Can create ascii files for spectro (Vpar,Vperp)
  - Nasa Themis spacecraft names
  - Magnetic field for Stereo: read V03 only
  - Write now Zvariables in CDF output
  - Bugs correction

---------------------
04/03/2008 (v8.1)
---------------------
  - Moments computation for Themis: uses spacecraft_potential, longitude=f(E), GSE frame
  - phi selection in time_phi plot and theta selection in time_theta plot
  - cl can reads only scalar and array in cdf
  - Themis eesa, iesa, esst, isst
  - cache size max = 2Gbytes
  - new option "cl -int module" to use module.pro
  - cl try to read similar fields when user change product
  - RLONG_RLAT: ascii file output and re-computes if necessary only
  - read correctly ascii files created with Notepad.exe

------------------
20/11/2007 (v8.0a)
------------------

  - Insert new Time-table widget
  - Bug correction for HIA energy table
  - l2_esa themis
  - l2_sst themis
  - l2_fbk

------------------
22/07/2007 (v7.9n)
------------------

  - bug correction

  - For MEX-IMA: use Andrei Fedorov MEX-IMA geometrical factor
  - For VEX-IMA: use same geometrical factor than MEX-IMA
  - For VEX-ELS: use engineering mode to determine ELS energy table

  - Clean cache now clean all filenames reference in cache: if a data file is modified, added or removed, there is no need to re-launch cl,
    clean cache must be enough.
  - cl can create ascii file greather than 2 G (gcc Linux and Solaris)
  - For MEX/ELS: cl use a special energy table (<1eV) when engineering data are incorrect.
  - For MEX/IMA:             display angle in MSO frame on (theta,phi) spectrogram with ATTITUDE file
  - For VEX/IMA and VEX/ELS: display angle in VSO frame on (theta,phi) spectrogram with ATTITUDE file

------------------
05/06/2007 (v7.6a)
------------------

  - For STEREO:
    * Change 'Bx_HGRTN_nT', 'By_HGRTN_nT', 'Bz_HGRTN_nT' by 'Bx_SC_nT', 'By_SC_nT', 'Bz_SC_nT' in magnetic field
    * Add P16 and P17: magnetic field in GSE frame
    * Add experiment LET and SEPT
    * Implementation of SWEA geometrical factor

  - For MEX: 
    * correction noise matrix e_mex
    * for PAC7, force Mass channel 30 and 31 for lower energies to contains H+
    * Use old and new energy table for IMA
    * Use engineering mode to determine ELS energy table

  - For MEX and VEX:
    * modify number of mass channel used in mass selection
    * Introduce Heavy Ion
    * introduce Noise level2
    * Introduce All Ion
    * Introduce remove Hghost with k1 and k2 constants


------------------
23/02/2007 (v7.4a)
------------------

  - New experiment: Themis
  - Orbit file for Stereo
  - New filename for VEX Magnetic filed


------------------
30/01/2007 (v7.3a)
------------------

  - New experiment: IMP8 and ISEE
  - New experiment: INTERBALL-ELECTRON, INTERBALL-FM3I, INTERBALL-MIFM


------------------
13/09/2006 (v7.10)
------------------

  - New constraint widget
  - Constraint time interval can be determinated directly in C langage (by default) or in IDL
  - cl can read data in one big array when reading more than one day (by default)
  - cl can read data directly in C langage (by default) or in IDL
  - cl can use Zlib to directly read ascii and binary ".gz files (by default)
  - New experiment GOES, WIND and INDICES
  - Moments computation for ASPERA3
  - New calibration for ASPERA3 and ASPERA4
  - Plot VENUS, MPB and BS for ASPERA4
  - Correction correction in HIA moments computation (thanks Giuseppe PALLOCCHIA)


------------------
11/01/2006 (v7.05)
------------------

  - New experiment SACC and XMM

------------------
25/07/2005 (v7.01)
------------------

 - New plots for DEMETER:
   - demeter_ondes_puissance_critere.cl: plot ICE for a selection on Longitude (RLONG) and Latitude (RLAT)
   - demeter_RLONG_RLAT.cl: Longitude_Latitude flux spectrogram for IDP


------------------
25/07/2005 (v7.00)
------------------

  - New experiment DSP-OTH with magnetic field data for DOUBLE-STAR in CDF format (CDF_PP_FGM) and
    plot using magnetic field in DOUBLE_STAR (Pad, fdist)
  - New experiments taking in account: DEMETER-ICE and DEMETER-IMSC
  - Add "Undo time" button in main window.
  - No needs to define CIS_ROOT, DSP_ROOT and Path. By default, /DATA/CLUSTER
    and /DATA/DOUBLE_STAR are used.
  - Some bugs correction.
  - Ascii output file is now created in distribution function even if magnetic field
    is not available (3D has to be choosen).
  - New plot: Distribution function 1D-Vpar and 1D-Vperp (ascii output is supported)
              Distribution function 2D-Vpar-Vperp (no ascii output)
  - Time series plot: it's possible to plot values as a function of one row. This
    row has to be selected in the widget Xaxis in Data menu.
  - Cl can read ascii file without time in the first row. In this case, the datation
    of the first line is set to 1/1/1950 at 00:00:00.000. The interval between lines
    is one second.
  - Cl runs more quickly!
  - Add widget Spacecraft_potential in data menu (this value is added one time to energy table
    for all particules and two times for He++).
  - Support for CESR spectrogram in CEF-2.0 format.
  - Bug correction in HIA moments computing after November 2003 (thanks to Giuseppe PALLOCCHIA).

  - Explanations on cl configuration:

    - In Preferences/Cache, put a cache size equal at maximum at the middle of your PC memory size.
      Under Unix, 256 Mbytes seems to be a a good value.

    - In Preferences/General, check the values of the following variables:

      Variable         LOCAL Path           LOCAL Compression   LOCAL Source    NFS Path               NFS Compresssion

      CLUSTER         /DATA/CLUSTER/DATA       .co or Yes*         hard disk    "path"/CLUSTER/DATA       Yes
      ORBITO_CLUSTER  /DATA/CLUSTER/ORBITO     -                   -            "path"/CLUSTER/ORBITO     -
      CDF_CLUSTER     /DATA/CLUSTER/CDF        -                   -            "path"/CLUSTER/CDF        -
      ACE             /DATA/ACE/DATA           -                   -            "path"/ACE/DATA           -
      ASPERA3         /DATA/ASPERA3/DATA       Yes                 hard disk    "path"/ASPERA3/DATA       Yes
      MGS             /DATA/MGS/DATA           -                   -            "path"/MGS/DATA           -
      DSP             /DATA/DOUBLE_STAR/STAR   .co or Yes*         -            "path"/DOUBLE_STAR/DATA   Yes
      DEMETER         /DATA/DEMETER/DATA       Yes                 -            "path"/DEMETER/DATA       Yes
      DSP_CDF         /DATA/DOUBLE_STAR/CDF    -                   -            "path"/DOUBLE_STAR/CDF    -
 
      * put 'Yes' for standard files (cl will compress counts in real time in memory).
        Put '.co' for special CESR data files using special compression for 3D counts files (files with extension .co or .co.gz).

    - Put the variable Use to 'LOCAL' if you want to use local path (files on your hard disk).
      Put this variable to 'NFS' if you want to use the alternative NFS path:
        - Under Windows: data from a Samba server seen on a mounted drive (ex path=Z:)
        - Under Unix: data from au Unix NFS server on a mounted path (ex path=/nfs)





-----------------
10/02/2005 (v6.7)
-----------------

  - Description of DEMETER data files.

	Each file contains an array of record written in the Sun FORMAT.
	Each record has a fixed length. The field date is the datation of
	the record and contains the number of milliseconds since
	01/01/1958 00:00:00.000.

	in YYYYMMDD, YYYY=Year, MM=Month and DD=day


	DEMETER_IDP_HKxxxx_YYYYMMDD_V01.bin
	-----------------------------------
		double		date
		float		Discri_level_keV
		float		Polar_voltage_Volt
		float		Temperature_deg
		float		Gene_test


	DEMETER_IDP_CNTxxx_YYYYMMDD_V01.bin
	-----------------------------------
		double		date
		unsigned char	table
		unsigned int	coup[0..2]


	DEMETER_IDP_BURSTx_YYYYMMDD_V01.bin
	-----------------------------------
		double		date
		unsigned char	burst
		unsigned int	coup[0..255]


	DEMETER_IDP_SURVEY_YYYYMMDD_V01.bin
	-----------------------------------
		double		date
		unsigned char	burst
		unsigned int	coup[0..127]


	DEMETER_IDP_ORBITO_YYYYMMDD_V01.bin
	-----------------------------------
		double		date
		short		orbit_number
		short		orbit_subnumber
		float		X_geo_m
		float		Y_geo_m
		float		Z_geo_m
		float		VX_geo_m_sec
		float		VY_geo_m_sec
		float		VZ_geo_m_sec
		float		X_VEIS_m
		float		Y_VEIS_m
		float		Z_VEIS_m
		float		VX_VEIS_m_sec
		float		VY_VEIS_m_sec
		float		VZ_VEIS_m_sec
		float		geocentric_latitude_deg
		float		geocentric_longitude_deg
		float		altitude_km
		float		local_time_of_the_first_point_of_the_data_array_hour
		float		Xsolar_geo
		float		Ysolar_geo
		float		Zsolar_geo
		float		Geomagnetic_latitude_deg
		float		Geomagnetic_longitude_deg
		float		Magnetic_local_time_of_the_first_point_hour
		float		Invariant_latitude_deg
		float		Mc_Ilwain_parameter_L
		float		Geocentric_latitude_of_the_conjugate_point_at_the_satellite_altitude_deg
		float		Geocentric_longitude_of_the_conjugate_point_at_the_satellite_altitude_deg
		float		Geocentric_latitude_of_North_conjugate_point_at_altitude_100km_deg
		float		Geocentric_longitude_of_North_conjugate_point_at_altitude_100km_deg
		float		Geocentric_latitude_of_South_conjugate_point_at_altitude_100km_deg
		float		Geocentric_longitude_of_South_conjugate_point_at_altitude_100km_deg
		float		Bx_nT
		float		By_nT
		float		Bz_nT
		float		B_nT
		float		DB_nT
		float		Proton_gyrofrequency_at_satellite_point_Hz
		float		S
		float		F
		float		pitchangle_deg

		The Values of S and F are computed with the expression:

                	S = L * ( sqrt (3.0*x*x + x) + 1/sqrt(3.0) * log (sqrt(3.0*x) + sqrt (3.0*x + 1)));
                	F = 1.0 / (S * S);

			with	L = Mc_Ilwain_parameter_L
                		x = sin(Geomagnetic_latitude_deg*M_PI/180.) * sin(Geomagnetic_latitude_deg*M_PI/180.)




-----------------
06/12/2004 (v6.6)
-----------------

 - In menu Panel of object Panel Composer, you can specify a constraint for
   a specific panel. Just enter the panel number in 'Constraint panel'
   (value between 1 and total number of panel) and a mathematic expression
   constituded of fields found in this panel and mathematic operators. The
   expression is not case sensitive. The 'Contraint panel' must be of class
   HEADER, COUNT2D, ASCII or CDF. cl will determine to time intervals
   where constraint equal 1 and then apply these time intervals to all panels.

   You can use the following operators:

        +:              addition
        -:              subtraction
        *:              multiplication
        /:              division
        &&:             logical and
        ||:             logical or
        <:              inferior
        <=:             inferior or equal
        >:              superior
        >=:             superior or equal
        ==:             equal
        !=:             different
        >>:             right shift
        <<:             left shift

        m_pi:           3.1415926535897932385

        abs (x):        absolute value of x
        atan (x):       inverse tangent of x
        cosh (x):       hyperbolic cosine of x
        exp (x):        exponential of x
        frac (x):       floating point of x
        int (x):        integer part of x
        log (x):        natural logarithm of x
        sinh (x):       hyperbolic sine of x
        sqrt (x):       square root of x
        sqr (x):        square of x
        acos (x):       inverse cosine of x
        asin (x):       inverse sine of x
        atan2 (y,x):    inverse tangent of y/x
        cos (x):        cosine of x
        log10 (x):      base 10 logarithm of x
        pow (x,y):      x raised to the exponent y
        sin (x):        sine of x
        tanh (x):       hyperbolic tangent of x
        tan (x):        tangent of x


   For example, if you have a panel composer with

     Panel 1: title
     Panel 2: header with the following fields:
                date
                B_nT
                Bx_sr2_nT
                By_sr2_nT
                Bz_sr2_nT
                Bx_gse_nT
                By_gse_nT
                Bz_gse_nT
                Bx_gsm_nT
                By_gsm_nT
                Bz_gsm_nT
     Panel 3: orbito

     you can specify 'Constraint panel' 2 
                     'Constraint value' Bx_gse_nT > -95
     to obtain the plot only when Bx_gse_nT is greather than -95.

 - New spectrogram (time, L) for DEMETER data averaged each orbit.

-----------------
04/11/2004 (v6.5)
-----------------

 - GSE to GSM transformation works now fine under Windows, Solaris, Linux
   without any FORTRAN source code.

 - New experiment taking in account: DEMETER-IDP

   For DEMETER ORBITO, the following parameters can be displayed:

               'orbit'              orbit_number
               'suborb'             orbit_subnumber
               'XGEO'               X_geo_m
               'YGEO'               Y_geo_m
               'ZGEO'               Z_geo_m
               'VXGEO'              VX_geo_m_sec
               'VYGEO'              VY_geo_m_sec
               'VZGEO'              VZ_geo_m_sec
               'XVEIS'              X_VEIS_m
               'YVEIS'              Y_VEIS_m
               'ZVEIS'              Z_VEIS_m
               'VXVEIS'             VX_VEIS_m_sec
               'VYVEIS'             VY_VEIS_m_sec
               'VZVEIS'             VZ_VEIS_m_sec
               'RLAT'               geocentric_latitude_deg
               'RLONG'              geocentric_longitude_deg
               'ALT'                altitude_km
               'LTI'                local_time_of_the_first_point_of_the_data_array_hour
               'XSUN'               Xsolar_geo
               'YSUN'               Ysolar_geo
               'ZSUN'               Zsolar_geo
               'MLAT'               Geomagnetic_latitude_deg
               'MLON'               Geomagnetic_longitude_deg
               'MLT'                Magnetic_local_time_of_the_first_point_hour
               'ILAT'               Invariant_latitude_deg
               'L'                  Mc_Ilwain_parameter_L
               'RLATC'              Geocentric_latitude_of_the_conjugate_point_at_the_satellite_altitude_deg
               'RLONC'              Geocentric_longitude_of_the_conjugate_point_at_the_satellite_altitude_deg
               'RLATNC100'          Geocentric_latitude_of_North_conjugate_point_at_altitude_100km_deg
               'RLONNC100'          Geocentric_longitude_of_North_conjugate_point_at_altitude_100km_deg
               'RLATSC100'          Geocentric_latitude_of_South_conjugate_point_at_altitude_100km_deg
               'RLONSC100'          Geocentric_longitude_of_South_conjugate_point_at_altitude_100km_deg
               'BX'                 Geographic_Bx_nT_model
               'BY'                 Geographic_By_nT_model
               'BZ'                 Geographic_Bz_nT_model
               'B'                  B_nT_model
               'DB'                 Difference_between_Bmodel_and_Bdipole_nT
               'Pf'                 Proton_gyrofrequency_at_satellite_point_Hz
               'S'                  Lenght_dipolar_field_lines
               'F'                  1_over_S_square
               'PI'                 Pitch_angle_IDP_deg

 - In Panel Composer, N objects can be superposed: the N-1 last objects must have Data_size equal to 0.
   In this case, color palettes and legends are now correctly positioned.

-----------------
02/07/2004 (v6.4)
-----------------

 - ppi can be choosen in TIFF file creation in DEVICE menu

 - More than on horizontal line can be plotted in HEADER object

 - Correct print under Windows

 - For batch mode (cl -batch filename), new parameter:
                 Supprimer_image_vide     =       1
   The value can be 0 or 1 (0 by default). Use 1 if you want cl to suppress
   postscript file with spectrogram all empty

 - Ascii export: it's possible to suppress comma and to put header in separate file

 - Time-energy Spectrogram: choosing a value different than 1 in "Y addition" cause cl to
   increase statistic in Y

 - Correction NPD/ASPERA3 for RAW, BIN AND PHD mode

 - New plot PH and TOF for NPD/ASPERA3

 - Correction PAC determination for IMA

 - HIA and DOUBLE-STAR moments computation: if necessary, it's possible to choose a mass
   different than proton (default)


-----------------
23/04/2004 (v6.3)
-----------------

 - TIFF format

 - DSP 3D Moments computations in GSE frame

 - New plot massQ_energy for ASPERA3

 - Optimization for ASPERA3-IMA 3D files

 - ASPERA3 ALTITUDE-ENERGY spectrogram

 - Bug corrections

 - Ascii output create ascii file for Distribution Function

 - DOUBLE STAR 3D moments in GSE frame


-----------------
03/12/2003 (v6.2)
-----------------

- take into account the new mode definitions for CODIF mode 12 and 14 
  after 2003-11-02T00:00:00.000Z: sweeps 6-21 use truncated energy table,
  sweeps 0-5 and 22-31 use normal energy table.

- New experiment taking in account: MGS

- New experiment taking in account: DSP (DOUBLE_STAR_PROJECT)

- Values in ORBITE and ORBITO objects are now writen with FORMAT F8.2 instead of F7.2

- Both ORBITE and ORBITO objects can plot any object that contains ORBITO or ORBITE data

- Ascii SPECTROGRAM: it's possible to load an ascii file in COUNT3D object, choose ASCII experiment
  and then plot a spectrogram.

  If you have M lines of data containing N Flux for N energies, the format of the Ascii file must be:

  EMIN value1 value2 ... valueN
  EMOY value1 value2 ... valueN
  EMAX value1 value2 ... valueN
  [DT   value]
  [Start_variable = Name1
  End_variable   = Name1
  Start_variable = Name2
  End_variable   = Name2
  ...
  ...
  Start_variable = NameN
  End_variable   = NameN]
  Datatation1 Flux1 Flux2 ... FluxN
  Datatation2 Flux1 Flux2 ... FluxN
  ...
  ...
  DatatationM Flux1 Flux2 ... FluxN

  - The symbol [xxx] means that xxx is optionnal.
  - EMIN, EMOY and EMAX is the Energies Table in eV (Minimum, Average and Maximum values)
  - DT is the number of seconds of validity of each lines
  - Name1, Name2 ... NameN contains the name of each Flux
  - Datation contains UT time in one of the following format:
      YYYY-MM-DDTHH:MM:SS.MSCZ
      YYYY-MM-DDTHH:MM:SSZ
      YYYY MM DD HH MM SS[.MSC]
      DD MM YYYY HH MM SS[.MSC]
  - Flux is the flux in part/(sec.cm2.sr.keV)

- Title Object: you can put your own text for Experiment, Spacecraft and Time


-----------------
20/10/2003 (v6.1)
-----------------

- time_energy spectrogramm: can create ascii file with energy, theta, phi for
  maximum value encountered (c, c/s, flux, ...) between Emin and Emax.

- can superpose N objects (a plot and a spectrogram for example): the N-1 last objects
  must have Data_size equal to 0.



-----------------
11/09/2003 (v6.0)
-----------------

- ASPERA3 plot support for ELS, NPI, NPD, IMA and HOUSEKEEPING.

- Spectrogram plot with ILAT (invariant latitud) on X axis.

- Plot 2 components of a vector.

- Plot contourfill and isocontour on the same plot

- Creation of CDF output except for spectrogram.

- Possibility to plot 2 CDF files in the same CDF object.

- For batch mode (cl -batch filename), new parameter:
                Jour_unique     =       1
  The value can be 0 or 1 (0 by default). Use 1 if you are sure that you plot data for one
  day only and if you want to optimize the computation time.



-----------------
03/02/2003 (v5.4)
-----------------

- IDL v5.6 support.

- CLUSTER Housekeeping plot with wording support.

- Cache improvement for ascii files. Before plotting ascii data of an ASCII object, cl
  determines if the corresponding ascii file has change since the last reading. If necessary,
  the file is read a another time.

- Check more strict for CODIF and HIA ACCUMULATION SPIN. If necessary, the message
  "WARNING: Use accumulation=1 for ..." is displayed.

- Bugs fixed.

- Cl launch optimization.

- Error computation modification in pitch-angle plot.

- Alfven velocity computation in COUNT2D and VB objects.

- New configuration "vue_flux.cl".

- 2 ascii files can be plotted in an single ASCII object: the second file
  is interpoled for the time found in the first file.



-----------------
25/10/2002 (v5.3)
-----------------

- Bug correction when reading a ".cl" file that contains 'HIA low g'.

- Inversion of Qx, Qy and Qz in 3D moment computations.

- Ascii output now contains units of each field.

- Unit correction in 'orbito' and 'orbite' object for ascii output.

- New option -batch in cl.

  Use: cl [-D] [-true] [-batch] [filename]

      -D : force compilation of ".pro" modules

      -true: use 24 bits per color

      -batch: batch mode

   filename: cl file (interactive mode) or command file (batch mode) to load


   So, for batch mode, use cl -batch filename. The syntax of filename is:

		Nomcl           =       filename.cl
		Nomps           =       filename
		Satellite       =       3
		Temps_debut     =       2002-09-30T00:00:00.000Z
		Temps_fin       =       2002-10-01T00:00:00.000Z
		Nombre_de_vues  =       1
		Orientation     =       Portrait
		Ascii           =       1

   In this example, cl will open the cl file "filename.cl" and realize one plot
   (Nombre_de_vues=1), between Temps_debut and Temps_fin, for spacecraft 3 (Satellite=3,
   value 0 is equivalent to None in interactive mode) in the Postscript file "filename_1.ps". 
   If Nombre_de_vues (number of plots) is greather than 1, cl will create filename_1.ps, 
   filename_2.ps, ...

   The orientation is Portrait (other value is Landscape). cl will also generate obj*.asc ascii 
   output files (0 means no ascii output).

- Explanations on distribution function

  For the distribution function depending on B, cl uses two vector:

  - Vboard: velocity in GSE frame from the onboard moments
  - B: from FGM in GSE frame (resolution 1 sec or 4 sec). If the resolution
  is 1 sec, cl compute the average.

  Theses 2 vectors defines a plane. We define V2 as B^Vboard.
  If T is the signed angle between Vboard and B, the vector V1 is
  define as Vboard rotated of pi/2-T around V2. 

  So, now:
  - Vpar is B
  - Vperp1 is V1
  - Vperp2 is V2

  After, cl represents the distribution function in the plane defines
  by the vectors V1 and V2.

  So, for "2D Vperp1 Vpar", cl uses the plane containing V1 and B.
      for "2D Vperp1 Vperp2", cl uses the plane containing V1 and V2 at Vpar=Vpar
      (widget near PT).
    
   
  If you choose width=0, cl makes a projection of the distribution function
  in this plane.

  If you choose a value for width, cl computes an averaged cut of the distribution
  function in the plane += width/2.



-----------------
26/09/2002 (v5.1)
-----------------

- Bug correction for HIA low g introduced in the last version. Now, the
  field 'hvtbl' is used to determine the number energy table used.

- Information on parameter 'Cjf' (found in Data Menu):

	'count':	raw counts per sample
	'count/spin':	raw counts per spin
	'count/s':	raw counts per second
	'c/s':		corrected counts per sec
	'flux':		flux (in part/(sec.cm2.sr.keV))
	'fdist':	distribution function (in sec3/km6)
	'JE':		flux*energy (in keV/(sec.cm2.sr.keV))

- New object 'orbite' similar to 'orbito' object. The binary file
  /DATA/CLUSTER/ORBITO/CLUSTERi/C1_L3_CISxxx_yyyymmdd_Vvv_ORBITExxxx.sdd contains
  the orbite parameters with
	yyyy:	Year
	mm:	Month
	dd:	Day
	vv:	Version
	i:	Spacecraft number (1..4)

  The following parameters can be displayed:

	'XGR'           'YGR'           'ZGR'           Position satellite repere geographique              (rt)
	'XGSE'          'YGSE'          'ZGSE'          Position satellite repere GSE                       (rt)
	'XGSM'          'YGSM'          'ZGSM'          Position satellite repere GSM                       (rt)
	'R'                                             Distance radiale satellite                          (rt)
	'DPP'                                           Distance a la plasmasphere                          (rt)
	'DMP'                                           Distance a la magnetopause                          (rt)
	'DBS'                                           Distance a la magnetopause ou onde de choc          (rt)
	'DZNSH'                                         Distance a la couche neutre                         (rt)
	'DZPSN'                                         Distance a la couche de plasma nord                 (rt)
	'DZPSS'                                         Distance a la couche de plasma sud                  (rt)
	'DSH'                                           Indicateur satellite dans l'ombre de la terre
	'VXGR'          'VYGR'          'VZGR'          Vitesse satellite repere geographique               (km)
	'VGR'                                           Module vitesse satellite repere geographique        (km)
	'BXGSM'         'BYGSM'         'BZGSM'         Composante B repere GSM
	'BGSM'                                          Module de B repere GSM
	'L'                                             Parametre L de Mac Ilain
	'ILAT'                                          Latitude invariante                                 (rad)
	'MLTS'                                          Temps local geomagnetique satellite
	'LATGRS'                                        Latitude  geographique  satellite
	'LONGRS'                                        Longitude geographique  satellite
	'MLTC'                                          Temps local geomagnetique point conjugue
	'LATGRC'                                        Latitude  geographique  point conjugue              (deg)
	'LONGRC'                                        Longitude geographique  point conjugue              (deg)
	'LATGMC'                                        Latitude  geomagnetique point conjugue              (deg)
	'LONGMC'                                        Longitude geomagnetique point conjugue              (deg)

-----------------
09/07/2002 (v5.0)
-----------------

- Bug correction for HIA high G, CODIF high g and CODIF low g in Solar 
  Wind mode. Now, I hope that only valid counts comming from valid phi, 
  theta and energy are taking in acount!

- New line objet.

- In 3D moments computation, if matrix file SR2_to_GSE is missing, the fields
  normaly expressed in GSE frame are now expressed in PSEUDO-GSE frame
  (and not in SR2 frame).


-----------------
05/06/2002 (v4.2)
-----------------

- Bug correction for high G of HIA in Solar Wind Mode. Now, all counts
  comming from Sun direction are used (in previous cl versions, the two
  spectrums looking in Sun direction were unused).

- True color images in GIF, BMP or PNG format can be displayed in IMAGE 
  object.
  

-----------------
17/05/2002 (v4.1)
-----------------

- Bug correction for high G and low g of CODIF in Solar Wind Mode
  in energy spectrogram with all phi addition: the counts under 2 Kev
  were too high. But the spectrograms was correct for Sun, Dusk, Tail and
  Dawn direction.
  Now, the counts for energy lower than 2 Kev when high G looks the
  Solar Wind (also when low g looks anti Solar Wind) are not used.

- Thick of labels of time axis can now be changed.


-----------------
03/05/2002 (v4.0)
-----------------
- New object 'cdf'. Like 'ascii' object, you can now read and plot a
cdf file. cl automatically found variables inside the CDF file.
The GUI is similar to 'ascii' or 'header' object.

- cl can directly plot some other experiments data in CDF format: depending
of time intervall and spacecraft number, cl automatically opens the(s) 
necessary file(s).

ACE: /DATA/ACE/DATA/AC_K0_EPM_yyyymmdd_Vvv.CDF
     /DATA/ACE/DATA/AC_K1_MFI_yyyymmdd_Vvv.CDF
     /DATA/ACE/DATA/AC_K0_SIS_yyyymmdd_Vvv.CDF
     /DATA/ACE/DATA/AC_K0_SWE_yyyymmdd_Vvv.CDF
     /DATA/ACE/DATA/AC_H0_SWE_yyyymmdd_Vvv.CDF

CIS: /DATA/CLUSTER/CDF/CIS/CLUSTERi/Cs_PP_CIS_yyyymmdd_Vvv.cdf (onboard moments file
     produced by CNES)

EFW: /DATA/CLUSTER/CDF/EFW/CLUSTERi/Cs_PP_EFW_yyyymmdd_Vvv.cdf

FGM: /DATA/CLUSTER/CDF/FGM/CLUSTERi/Cs_PP_FGM_yyyymmdd_Vvv.cdf (4 sec resolution)

with yyyy: Year
     mm:   Month
     dd:   Day
     vv:   Version
     i:    Spacecraft number (1..4)
The directories /DATA/ACE/DATA and /DATA/CLUSTER/CDF can be changed in Preferences/General.


- Ground 3D Moments: many bugs correction (low g in Solar Wind Mode, Energy band to be used). Now, the 
values in GSE are not in SR2 but in real GSE coordinate system (using the file 'SR2_GSE' in L3 
directory).

- Magnetic field data: cl can plot data with 1 sec resolution (P3 CIS3) and data with 4 sec
resolution (P5 CIS3).

- GSM coordinate system: for each vector in GSE, the corresponding vecteur in GSM is computed by 
cl. If necessary, the module is also computed. The computation is done for:
  . PSDS FGM magnetic field (P3 CIS-OTH)
  . CODIF onboard moments (P50 and P51 for CIS-CODIF)
  . HIA   onboard moments (P50 and P51 for CIS-HIA)
  . PPD CODIF and HIA onboard moments (P2 for CIS-OTH)
  . CDF CODIF and HIA onboard moments (P4 for CIS-OTH)

- Multi spacecraft plot: for header and count2d object, it's possible to plot data from
different spacecraft. If 'Yes' is selected for parameter 'Multi Spacecraft' in 'Multi' menu, then:
 . For header object, the 'Plot' parameter in 'Data' menu displays the fields found in each selected 
   products for spacecraft 1 to 4.
 . For count2d object, the parameter 'Sc' will appear in 'Data' menu (each plot is defined for 
   a specific spacecraft).

- Multi experiment plot: for header and count2d object, it's possible to plot data from
different experiment. If 'Yes' is selected for parameter 'Multi Experiment' in 'Multi' meny, then:
 . For header object, the 'Plot' parameter in 'Data' menu displays the fields found in each selected
   products for experiment  CIS1 (CODIF), CIS2 (HIA), CIS3 (CIS-OTH) and CIS6 (ACE). For example, if
   P50 and P51 is selected, it's possible to plot onboard moments for CODIF and HIA.
 . For count2d object, the parameter 'Experiment' will appear in 'Data' menu (each plot is defined for
   a specific experiment)

- Multi product plot: for header and count2d object, it's possible to plot data from
different product. If 'Yes' is selected for parameter 'Multi Product' in 'Multi' meny, then:
 . For header object, the 'Plot' parameter in 'Data' menu displays the fields found in each selected
   products. If a field is present in 2 products, the 2 lines will be present. For example, for CIS3,
   if P3 and P5 are selected, it's possible to plot Bx_gse_nT from P3 (1 sec resolution) and P5
   (4 sec resolution) on the same panel.
 . For count2d object, the parameter 'Products' will appear in 'Data' menu (each plot is defined for
   a specific group of products). For example, it's possible to plot density for hig G HIA and
   density for low g HIA in the same panel.

- B resolution in phi_theta, distribution function, VB in 3D moments and onboard moments.
  It's possible to choose for B resolution '1 sec' or '4 sec'.

 . phi_theta: in both cases, the B values found in the 4 sec after Start Time are displayed.

 . distribution function: in both cases, the averaged values of B found in the 4 sec after 
   Start Time is used to compute vector Vpar, Vperp1 and Vperp2 (Vperp2 = Vpar ^ Vperp1).

 . VB in 3D moments and onboard moments:
   - for '1 sec': in each spin, the B used is the averaged values of B found in the
     validity duration of the spin (depends on accumulation value).
   - for '4 sec': in each spin, the B used is the interpolated values of B in the
     middle of the spin (depends on accumulation valued).

- 3D moments field description:
 . N_cm3: density
 . Vx_km_sec, Vy_km_sec, Vz_km_sec: 3 components of velocity in experiment frame
 . V_km_sec: module of velocity
 . Vx_gse_km_sec, Vy_gse_km_sec, Vz_gse_km_sec: 3 components of velocity in gse frame
 . Vx_gsm_km_sec, Vy_gsm_km_sec, Vz_gsm_km_sec: 3 components of velocity in gsm frame
 . Ppar_eV_cm3
 . Pper1_eV_cm3
 . Pper2_eV_cm3
 . Tpar_eV
 . Tper1_eV
 . Tper2_eV
 . Qx_erg_sec_cm2, Qy_erg_sec_cm2, Qz_erg_sec_cm2: 3 components of heat flux in experiment frame
 . Q_erg_sec_cm2: module of heat flux
 . Qx_gse_erg_sec_cm2, Qy_gse_erg_sec_cm2, Qz_gse_erg_sec_cm2: 3 components of heat flux in gse frame
 . Qx_gsm_erg_sec_cm2, Qy_gsm_erg_sec_cm2, Qz_gsm_erg_sec_cm2: 3 components of heat flux in gsm frame
 . Pxx_eV_cm3
 . Pxy_eV_cm3
 . Pxz_eV_cm3
 . Pyy_eV_cm3
 . Pyz_eV_cm3
 . Pzz_eV_cm3
 . Ei_eV_cm3
 . Ti_eV
 . Ex
 . Ey
 . Ez
 . Ex_gse
 . Ey_gse
 . Ez_gse
 . Ex_gsm
 . Ey_gsm
 . Ez_gsm
 . Vxpar_gse_km_sec
 . Vypar_gse_km_sec
 . Vzpar_gse_km_sec
 . Vpar_gse_km_sec
 . Vxpar_gsm_km_sec
 . Vypar_gsm_km_sec
 . Vzpar_gsm_km_sec
 . Vxper_gse_km_sec
 . Vyper_gse_km_sec
 . Vzper_gse_km_sec
 . Vper_gse_km_sec
 . Vxper_gsm_km_sec
 . Vyper_gsm_km_sec
 . Vzper_gsm_km_sec
 . Elx_gse_mV_m
 . Ely_gse_mV_m
 . Elz_gse_mV_m
 . El_gse_mV_m
 . Elx_gsm_mV_m
 . Ely_gsm_mV_m
 . Elz_gsm_mV_m
 . Pp_nPa
 . Pm_nPa
 . Beta


---------
21/7/2001
---------
Time Format

         FORMAT = format string.  Allows output date to be customized.
         The default format string is 'Y$ n$ d$ h$:m$:s$ w$'
            The following substitutions take place in the format string:
         Y$ = 4 digit year.
         y$ = 2 digit year.
         N$ = full month name.
         n$ = 3 letter month name.
         0n$= month as a 2 digit number.
         d$ = day of month number.
         0d$= 2 digit day of month number.
         doy$= 3 digit day of year (see DDECIMAL below).
         W$ = full weekday name.
         w$ = 3 letter week day name.
         h$ = hour.
         m$ = minute.
         s$ = second.
         f$ = fraction of second (see DECIMAL, DENOMINATOR below).
         I$ = time interval in days to 2 decimal places.
         i$ = time interval in days as an integer.
         H$ = time interval in integer hours.
         sam$ = Time in seconds after midnight (DECIMAL works here).
         @  = Carriage Return.
         !  = Line feed.                                                                 

         Some examples: 'h$:m$:s$' -> 09:12:04,
                        'd$ n$ Y$' -> 12 Jan 1991
                        'd$D h$h' -> 3D 2h, ...


---------
20/7/2001
---------
New object 'Ascii'. Now, it's possible to read an timeseries ascii file
and plot it directly with cl. The format of the ascii file is compatible 
with the ascii output generated by cl. But, some informations can be
missing. The minimal informations is:

[Start variable = epoch
 End varaible   = epoch] -> OPTIONAL definition of the field "Universal Time" ('date' by default)

[Start variable = Name1
 End   variable = Name1] -> OPTIONAL definition of the field nb 1 ('Field1' by default)

[Start variable = Name2
 End   variable = Name2] -> OPTIONAL definition of the field nb 2 ('Field2' by default)

         ...
 
[Start variable = Namen
 End   variable = Namen] -> OPTIONAL definition of the field nb n ('Fieldn' by default)

date1[,] FIELD1[,] FIELD2[,] ... FIELDn[,] -> data record nb 1 (',' is OPTIONAL)
date2[,] FIELD1[,] FIELD2[,] ... FIELDn[,] -> data record nb 2 (',' is OPTIONAL)
         ...
datem[,] FIELD1[,] FIELD2[,] ... FIELDn[,] -> data record nb m (',' is OPTIONAL)

date format: you can use one of the follzing format
 - "YYYY-MM-DDTHH:MM:SS.MSCZ"
 - "YYYY MM DD HH MM SS.MSC"
 - "DD MM YYYY HH MM SS.MSC"


----------
29/01/2001
----------
New object animation 
New format ".bmp" et "png"


---------
23/1/2001
---------
Correction of Qx, Qy, Qz


----------------------
Distribution functions
----------------------
- Start Time: the soft looks for the first spin greater or equal than this time

- End Time: not used but must be greather than Start Time!

- spin accumulation: with the value one, the software takes the data for the
first spin contained after Start time and compute the corrresponding count according
with the spin accumulation described in the calibration file. With the value N,
the software do the same for N successives spins and just compute the addition of the count.

- time intervall: used with spin accumulation, if you ask N spin accumulation,
the soft looks for N successives spins found starting at Start time and
ending at Start time + time interval.

- for a specific cut, using TRIGRID interpolation, I give to IDL TRIGRID
functions all the points and IDL compute an interpolated picture (so with
interpolation between pixel). Using "None" for interpolation, cl doesn't
interpolate anything!

- specific cut: Choose in "Distribution" box the value "2D V1 V2 at PT", 
"3D V1 V2 at PT" or "3DANIM V1 V2 at PT". You must the specify the values for
V1 V2 and PT. You will obtain a cut from the plane defined with the 2 vectors
V1 and V2 and the point PT:
 V1 is a vector in the frame (Vx, Vy, Vz)
 V2 is a vector in the frame (Vx, Vy, Vz)
 PT is a point in the frame (Vx, Vy, Vz)


---------------------------------
Energy sweeps that stop at ~ 2keV
---------------------------------
In solar wind modes, for Codif, for some phi direction, of course, I know that
many sweeps contains data for the same energy band (~ 2keV).

At this time, for time-energy spectrogram, the soft handles energy sweeps that
stop at 2 keV only for Sun direction with high g and for Tail direction with
low g.
If you select a specific phi direction, the soft uses the Magnetospheric energy
table. The problem is not so simple because it's possible to select many phi:
- if you select only phi in Sun direction: SW table must be used
- if you don't select any phi in Sun direction: MAG table must be used
- in other case, what table has to be used?
Perhaps I could correct this problem in the future but, at this time, the
problem has not been corrected.


----------
GIF format
----------
I have now add the PNG format

----------------
c/s and Counts/s
----------------
Counts/s : count per second corrected by the spin accumulation without using
anods efficiencies.

c/s: same but using the anods efficiencies!


--------------
Date selection
--------------
The format is DD MM YYYY HH MM SS.MSC
 or           DD MM YYYY HH MM SS
 or           DD MM YYYY HH MM
 or           DD MM YYYY HH
 or           DD MM YYY
 (missing values mean 0)


--------------------------------------------------------------------------
To see what data of what day and what spacecraft are available on the disk
--------------------------------------------------------------------------
 1) Select the menu Infos/Data: specify 2 days
 2) Wait for the list of files between Start files and End files
 For each day you will have for each spacecraft 3 columns with
  1th column: COD (data for CODIF) or ... (No data for codif)
  2th column: HIA (data for HIA) or ... (No data for HIA)
  3th column: OTH (data for Orbit PPD) or ... (No data for OTH)

-------------------------
In order to obtain a plot
-------------------------
 CASE 1
 1) In the menu Preferences/General: specify Start Time + End Time + Spacecraft and OK to validate
 2) In the menu Add: select a predefined plot (CNES  ESOC  ...  HOME)
 3) Click OK in the window (Start End Spacecraft = default and Full screen object)
 4) Wait until the end of plot
 Defaut spacecraft must be None if the plot contains more than one spacecraft (eg esoc 34)

 CASE 2
 1) In the menu Add: select a predefined plot (CNES  ESOC  ...  HOME)
 2) In the window: choose Select values for Start End Spacecraft and OK to validate
 3) Enter Start time + End Time + Spacecraft in the console

------------------
Duration of a plot
------------------
It's possible to plot more than one day. In this case just specify two differents day
