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STEREO-B Solar Electron Proton Telescope (SEPT) Experiment: Ion and Electron hourly omnidirectional fluxes

Data source at: CDAWeb
Only arithmetic hourly averaging ( between north field of view, south field of view, sunward direction, and anti-sunward direction ) was done. (No averaging of logarithms and No threshold numbers of finer scale points.)
We believe, these data will be useful for looking at large solar disturbances near STEREO-B

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Time span: 2006-11-14 - 2014-09-26

Enter start and stop dates: year,month,day(YYYYMMDD) or year,day_of_year(YYYYDOY)
   Start time    Stop time

Units: 1/(sec-cm**2-ster-MeV/n )
Fluxes   (Numbers below are min/max energies in MeV/n)
Electrons(e)
0.000-0.035
0.035-0.045
0.045-0.055
0.055-0.065
0.065-0.075
0.075-0.085
0.085-0.105
0.105-0.125
0.125-0.145
0.145-0.165
0.165-0.195
0.195-0.225
0.225-0.255
0.255-0.295
0.295-0.335
0.335-0.375
0.375-0.425
0.425-0.485
0.485-0.545
0.545-0.615
0.615-0.695
0.695-0.785
0.785-0.875
0.875-0.985
0.985-1.115
1.115-1.255
1.255-1.405
1.405-1.585
1.585-1.775
1.775-1.995
1.995-2.235
2.235-6.500
Ions
0.000-0.075
0.075-0.084
0.084-0.093
0.093-0.101
0.101-0.110
0.110-0.119
0.119-0.137
0.137-0.156
0.156-0.175
0.175-0.193
0.193-0.220
0.220-0.246
0.246-0.273
0.273-0.312
0.312-0.351
0.351-0.390
0.390-0.438
0.438-0.496
0.496-0.555
0.555-0.623
0.623-0.701
0.701-0.788
0.788-0.876
0.876-0.983
0.983-1.112
1.112-1.251
1.251-1.400
1.400-1.578
1.578-1.767
1.767-1.985
1.985-2.224
2.224-6.500


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If you have any questions/comments about the OMNWeb Plus, contact Dr. Natalia Papitashvili,Mail Code 672, NASA/Goddard Space Flight Center, Greenbelt, MD 20771

NASA Official: Dr. Robert McGuire, Head of the Space Physics Data Facility