SPECIES: H_summed
BEGIN HEADER
STEREO LET Level 1 Combined proton intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   1.8 -  3.6 MeV proton intensity (1/(cm^2 s sr MeV/nuc))
Column 8:   4.0 -  6.0 MeV proton intensity (1/(cm^2 s sr MeV/nuc))
Column 9:   6.0 - 10.0 MeV proton intensity (1/(cm^2 s sr MeV/nuc))
Column 10: 10.0 - 15.0 MeV proton intensity (1/(cm^2 s sr MeV/nuc))
Column 11 - 14: 4 proton counts , same energy ranges as above (counts/minute)
Column 15 - 18: 4 proton statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity.
     U(I) is the uncertainty in the calculated average intensity.
     Ii is the intensity for minute i in one of the energy bins.
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins.
     M is the number of good 1-minute records in the averaging interval.
The total number of counts in each hour is also provided.
BEGIN DATA
END HEADER

SPECIES: He3_summed
BEGIN HEADER
STEREO LET Level 1 Combined 3He intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc 3He intensity (1/(cm^2 s sr MeV/nuc))
Column 8:   6.0 - 10.0 MeV/nuc 3He intensity (1/(cm^2 s sr MeV/nuc))
Column 9:  10.0 - 15.0 MeV/nuc 3He intensity (1/(cm^2 s sr MeV/nuc))
Column 10 - 12: 3 3He counts , same energy ranges as above (counts/minute)
Column 13 - 15: 3 3He statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: He4_summed
BEGIN HEADER
STEREO LET Level 1 Combined 4He intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   1.8 -  3.6 MeV/nuc 4He intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   4.0 -  6.0 MeV/nuc 4He intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:   6.0 - 10.0 MeV/nuc 4He intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 10.0 - 15.0 MeV/nuc 4He intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 4He counts , same energy ranges as above (counts/minute)"
Column 15 - 18: 4 4He statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: He_summed
BEGIN HEADER
STEREO LET Level 1 Combined Helium intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc He intensity (1/(cm^2 s sr MeV/nuc))
Column 8:   6.0 - 10.0 MeV/nuc He intensity (1/(cm^2 s sr MeV/nuc))
Column 9:  10.0 - 15.0 MeV/nuc He intensity (1/(cm^2 s sr MeV/nuc))
Column 10 - 12: 3 He counts , same energy ranges as above (counts/minute)
Column 13 - 15: 3 He statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: C_summed
BEGIN HEADER
STEREO LET Level 1 Combined carbon intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc carbon intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc carbon intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc carbon intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc carbon intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 carbon counts, same energy ranges as above (counts/minute)"
Column 15 - 18: 4 carbon statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: N_summed
BEGIN HEADER
STEREO LET Level 1 Combined nitrogen intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc nitrogen intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc nitrogen intensity (1/(cm^2 s sr MeV/nuc))"
Column 9: 10.0 - 15.0 MeV/nuc nitrogen intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc nitrogen intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 nitrogen counts, same energy ranges as above (counts/minute)"
Column 15 - 18: 4 nitrogen statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: O_summed
BEGIN HEADER
STEREO LET Level 1 Combined oxygen intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc oxygen intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc oxygen intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc oxygen intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc oxygen intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 oxygen counts, same energy ranges as above (counts/minute)"
Column 15 - 18: 4 oxygen statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Ne_summed
BEGIN HEADER
STEREO LET Level 1 Combined neon intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc neon intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc neon intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc neon intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc neon intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 neon counts, same energy ranges as above (counts/minute)"
Column 15 - 18: 4 neon statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Na_summed
BEGIN HEADER
STEREO LET Level 1 Combined sodium intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:  10.0 - 15.0 MeV/nuc sodium intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:  15.0 - 27.0 MeV/nuc sodium intensity (1/(cm^2 s sr MeV/nuc))"
Column 9 - 10: 2 sodium counts, same energy ranges as above (counts/minute)"
Column 11 - 12: 2 sodium statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Mg_summed
BEGIN HEADER
STEREO LET Level 1 Combined magnesium intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc magnesium intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc magnesium intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc magnesium intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc magnesium intensity (1/(cm^2 s sr MeV/nuc))"
Column 11 - 14: 4 magnesium counts, same energy ranges as above (counts/minute)"
Column 15 - 18: 4 magnesium statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Al_summed
BEGIN HEADER
STEREO LET Level 1 Combined aluminum intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   6.0 - 10.0 MeV/nuc aluminum intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:  10.0 - 15.0 MeV/nuc aluminum intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  15.0 - 27.0 MeV/nuc aluminum intensity (1/(cm^2 s sr MeV/nuc))"
Column 10 - 12: 3 aluminum counts, same energy ranges as above (counts/minute)"
Column 13 - 15: 3 aluminum statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Si_summed
BEGIN HEADER
STEREO LET Level 1 Combined silicon intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc silicon intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc silicon intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc silicon intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc silicon intensity (1/(cm^2 s sr MeV/nuc))"
Column 11: 27.0 - 40.0 MeV/nuc silicon intensity (1/(cm^2 s sr MeV/nuc))"
Column 12 - 16: 5 silicon counts, same energy ranges as above (counts/minute)"
Column 17 - 21: 5 silicon statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: S_summed
BEGIN HEADER
STEREO LET Level 1 Combined sulfur intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc sulfur intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc sulfur intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc sulfur intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc sulfur intensity (1/(cm^2 s sr MeV/nuc))"
Column 11: 27.0 - 40.0 MeV/nuc sulfur intensity (1/(cm^2 s sr MeV/nuc))"
Column 12 - 16: 5 sulfur counts, same energy ranges as above (counts/minute)"
Column 17 - 21: 5 sulfur statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Ar_summed
BEGIN HEADER
STEREO LET Level 1 Combined argon intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc argon intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc argon intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc argon intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc argon intensity (1/(cm^2 s sr MeV/nuc))"
Column 11: 27.0 - 40.0 MeV/nuc argon intensity (1/(cm^2 s sr MeV/nuc))"
Column 12 - 16: 5 argon counts, same energy ranges as above (counts/minute)"
Column 17 - 21: 5 argon statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Ca_summed
BEGIN HEADER
STEREO LET Level 1 Combined calcium intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc calcium intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc calcium intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc calcium intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc calcium intensity (1/(cm^2 s sr MeV/nuc))"
Column 11: 27.0 - 40.0 MeV/nuc calcium intensity (1/(cm^2 s sr MeV/nuc))"
Column 12 - 16: 5 calcium counts, same energy ranges as above (counts/minute)"
Column 17 - 21: 5 calcium statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Fe_summed
BEGIN HEADER
STEREO LET Level 1 Combined iron intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:   4.0 -  6.0 MeV/nuc iron intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:   6.0 - 10.0 MeV/nuc iron intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  10.0 - 15.0 MeV/nuc iron intensity (1/(cm^2 s sr MeV/nuc))"
Column 10: 15.0 - 27.0 MeV/nuc iron intensity (1/(cm^2 s sr MeV/nuc))"
Column 11: 27.0 - 40.0 MeV/nuc iron intensity (1/(cm^2 s sr MeV/nuc))"
Column 12 - 16: 5 iron counts, same energy ranges as above (counts/minute)"
Column 17 - 21: 5 iron statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

SPECIES: Ni_summed
BEGIN HEADER
STEREO LET Level 1 Combined nickel intensities for ahead spacecraft, for 2022
Verified Data - OK to distribute
File created: INSERTDATEHERE
Created by: Caltech Space Radiation Lab
Hourly-averaging Software Version: INSERTVERSIONHERE
Level 1 software version: 11
Time Resolution: 1 hour
Note: Timestamps mark Beginning of averaging interval.
These data are binned into wider energy ranges than the raw data.
They should be useful for plotting trends or computing ratios.
Column 1: Year
Column 2: Day of year (fractional)
Column 3: Hour of day
Column 4: Minute of hour
Column 5: Second of minute
Column 6: LET Livetime (seconds)
Column 7:  10.0 - 15.0 MeV/nuc nickel intensity (1/(cm^2 s sr MeV/nuc))"
Column 8:  15.0 - 27.0 MeV/nuc nickel intensity (1/(cm^2 s sr MeV/nuc))"
Column 9:  27.0 - 40.0 MeV/nuc nickel intensity (1/(cm^2 s sr MeV/nuc))"
Column 10 - 12: 3 nickel counts, same energy ranges as above (counts/minute)"
Column 13 - 15: 3 nickel statistical uncertainties  (1/(cm^2 s sr MeV/nuc))
Bad/missing data are filled as follows:
     -9999.9 for floating-point data
     -9999 for integer data
1-hour Averages and Uncertainties are calculated as follows:
     I = Sum(Ii)/M
     U(I) = sqrt ( Sum( Ii^2/Ni ) ) / M
     I is the hourly average intensity
     U(I) is the uncertainty in the calculated average intensity
     Ii is the intensity for minute i in one of the energy bins
     Ii^2 = Ii * Ii  (in case the notation is confusing...)
     Ni is the counts for minute i in one of the energy bins
     M is the number of good 1-minute records in the averaging interval.
BEGIN DATA
END HEADER

