CRRES PROTEL proton equatorial distributions vs.L
This data set holds half-orbit (~5 hour) resolution \nproton distributions (19 5-deg equatorial pitch angles vs. 24 energies) \nfrom the Proton Telescope (PROTEL) on the CRRES spacecraft. \nThe energy range covered is 1-100 MeV. These data are developed from \nthe 1-min insitu pitch angle distributions by assigning each 5-deg bin \nin pitch angle a corresponding McIlwain L value and then by mapping the \ninsitu pitch angle distribution to the equator, into 0.05-wide L bins, \nassuming first adiabatic invariant conservation. The mapping yields \nequivalent equatorial pitch angles. Flux data for a given half-orbit, \ngiven 0.05-wide L bin, given equatorial pitch angle and given energy bin\nare then averaged. Data records are for a given half-orbit and given\nL bin; each record contains averaged fluxes vs. equatorial pitch angle\nand energy. The data are in SGI(UNIX) binary format. Read software\nis contained within the companion documentation.
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Complete Metadata
| @type | dcat:Dataset |
|---|---|
| accessLevel | public |
| bureauCode |
[
"026:00"
]
|
| contactPoint |
{
"fn": "NASA Space Physics Data Facility",
"@type": "vcard:Contact",
"hasEmail": "mailto:NASA-SPDF-Support@nasa.onmicrosoft.com"
}
|
| description | This data set holds half-orbit (~5 hour) resolution \nproton distributions (19 5-deg equatorial pitch angles vs. 24 energies) \nfrom the Proton Telescope (PROTEL) on the CRRES spacecraft. \nThe energy range covered is 1-100 MeV. These data are developed from \nthe 1-min insitu pitch angle distributions by assigning each 5-deg bin \nin pitch angle a corresponding McIlwain L value and then by mapping the \ninsitu pitch angle distribution to the equator, into 0.05-wide L bins, \nassuming first adiabatic invariant conservation. The mapping yields \nequivalent equatorial pitch angles. Flux data for a given half-orbit, \ngiven 0.05-wide L bin, given equatorial pitch angle and given energy bin\nare then averaged. Data records are for a given half-orbit and given\nL bin; each record contains averaged fluxes vs. equatorial pitch angle\nand energy. The data are in SGI(UNIX) binary format. Read software\nis contained within the companion documentation. |
| distribution |
[
{
"@type": "dcat:Distribution",
"format": "BIN",
"mediaType": "application/octet-stream",
"downloadURL": "ftps://spdf.gsfc.nasa.gov/pub/data/crres/particle_protel/"
},
{
"@type": "dcat:Distribution",
"format": "BIN",
"mediaType": "application/octet-stream",
"downloadURL": "https://spdf.gsfc.nasa.gov/pub/data/crres/particle_protel/"
}
]
|
| identifier | /SDE/SPASE_JSON/|b02900d6ef2cf7e5b4a3885e24cae79a |
| keyword |
[
"energeticparticles"
]
|
| license | https://www.usa.gov/government-works |
| modified | 2026-03-30 |
| programCode |
[
"026:000"
]
|
| publisher |
{
"name": "NASA Space Physics Data Facility (SPDF) Data Services",
"@type": "org:Organization"
}
|
| theme |
[
"Heliophysics"
]
|
| title | CRRES PROTEL proton equatorial distributions vs.L |
