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MAVEN Solar Energetic Particle (SEP) Experiment: Ion and Electron hourly fluxes in Rare look direction from s1 sensor

Time span: 2014-09-22 - 2024-05-14

Original ~8-seconds data source at:PDS Data System
Only arithmetic hourly averaging 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 Mars

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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-KeV/n )
Fluxes   (Numbers below are min/max energies in KeV/n)
Ions
19.7-21.1
21.1-22.5
22.4-23.8
23.8-26.6
26.5-29.3
29.3-33.3
33.3-38.7
38.7-45.5
45.5-55.1
55.1-67.3
67.3-83.7
83.6-105.4
105.8-134.2
133.7-170.3
170.6-219.4
219.1-282.9
283.2-368.8
369.5-480.5
480.5-627.5
628.0-822.0
822.0-1078.0
1081.5-1418.5
1417.5-1862.5
1857.5-2442.5
2445.5-3214.5
3215.0-4225.0
4225.0-5575.0
5575.0-7245.0
Electrons(e)
20.1-21.5
21.5-22.9
22.9-24.3
24.3-27.1
27.1-29.9
29.9-34.1
34.1-39.7
39.8-46.8
46.8-56.6
56.6-69.3
69.2-86.2
86.2-108.8
108.2-137.8
138.0-176.0
176.7-227.3
 

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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: Robert Candey (Robert.M.Candey@nasa.gov), Head of the Space Physics Data Facility