Minutes * The SSC presented the baseline plans based on the input from the instrument teams. The baseline plan fits within the allocations, so the only question was what extra telemetry should be added to fill out the residual. * All the instrument teams except SECCHI are recording their beacon telemetry on the SSR. These data also come down during the realtime passes. The actual allocations weren't discussed during the telecon, but appear on the spreadsheet conjunction.xls. * IMPACT presented plans for using the residual telemetry allocations for both side lobes 1 and 2. * It was pointed out that the additional SEPT-NS measurements for side lobe 1 would be the only ones taken out of the ecliptic. * Additional SIT event telemetry for side lobe 1 would improve the composition measurements. * IMPACT data would be produced on the same time scales as currently, which is SEP data within a few days, and HEP data within a month or two. Beacon data would be processed within the SSC as usual, and would be the data used for space weather forecasting. The other realtime data telemetry would be used for after-the-fact data analysis. * The IMPACT proposals for side lobe 2 cover a wide range of telemetry rates. * PLASTIC depends on ApID 0x200 from the IMPACT housekeeping. * PLASTIC would like to see ApID 0x317 to their side lobe 2 telemetry for 2D measurements of protons and Helium. Their calibration monitoring would also be improved with these data. * SECCHI plans to concentrate on EUVI and HI images. Small COR1/2 images would be brought down mainly to monitor the health of the telescopes. * SECCHI is looking into the possibility of saving some images in their own internal RAM to be brought down later during the realtime pass, e.g. with a 12 hour or even 6 hour separation. * SECCHI requests an additional 325 bps during side lobe 2 operations to bring down improved HI images. Images were presented showing the improvement in the images for several image conditions. * The baseline SWAVES plan would bring down only the beacon and housekeeping packets. However, during side lobe 1, they would like to bring down an additional 10.7 packets/minute (~390 bps). This would double their frequency resolution, approximately double their time resolution, and allow them to do direction finding and polarization studies. They estimate that this would be a total increase of a factor of ~16 in their overall science return. SWAVES does not have a way of modifying this additional telemetry rate--it's either all or nothing. * SWAVES is the only instrument that wishes to stay on during the entire solar conjunction period. * It was pointed out that after the spacecraft pass solar conjunction, some of the SEP instruments will no longer be aligned along the Parker spiral. This will tend to mostly affect the initial data from an event. After a few hours, the data become isotropic. * NASA has put a page explaining the situation for the public at http://www.nasa.gov/content/goddard/stereo-entering-new-stage-of-operations/ Decisions * For side lobe 1, it was decided that the spacecraft and instruments would change weekly, alternating between a mode where IMPACT gets more data, and mode where SWAVES gets more data. In both modes, IMPACT should be able to include the additional 36 bps telemetry from the SEPT-NS measurements. This alternating mode of operation will be evaluated after the first period of side lobe 1 operations, during ingress towards solar conjunction, to determine whether this should be used during the second period, during egress. * For side lobe 2, it was decided that SECCHI should receive the extra 325 bps they requested for improved HI images. * It was also decided that PLASTIC should receive some of their ApID 0x317 telemetry, but that this should be reduced in volume within the combined IMPACT/PLASTIC IDPU. The IMPACT and PLASTIC teams will get together and present a combined plan for making use of the additional 262 bps of residual telemetry Action Items * The IMPACT and PLASTIC teams will deliver to the SSC a combined plan for side lobe 2 operations by Tuesday, July 8. * All the instrument teams will deliver to the MOC, with a copy to the SSC, their realtime telemetry requirements for side lobes 1 and 2 by Friday, July 11. These plans will include what ApIDs will be brought down, and what their rates will be.