Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts

Details Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008adspr..42.1523g&link_type=abstract

Advances in Space Research, Volume 42, Issue 9, p. 1523-1526.

Other

2

Scientific paper

The paper presents the analysis of experimental data on electron fluxes with energies 10 keV 10 MeV. Data were obtained during 1978 2005 years in different space experiments (COSMOS-900, MIR Space Station, ACTIVE, SAMPEX, CORONAS-I, CORONAS-F, NOAA POES-17, TATYANA and others). Two areas of electron flux enhancements are studied in the paper: the near-equatorial (L < 1.2) zone and the middle-latitude (1.2 < L < 1.9) zone. It is shown that electron flux enhancements are regularly registered at L < 2 and the observed formations have some typical features. Electron peaks at L < 1.2 appear sporadically while peaks at 1.2 < L < 1.9 are observed regularly. The approximations of spectra by several functions including kappa-function are presented.

Affiliated with

Also associated with

No associations

Rating

Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral characteristics of electron fluxes at L < 2 under the Radiation Belts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1841007