Differences between transmitter precipitation peaks and storm injection peaks in low-altitude energetic electron spectra

Details Differences between transmitter precipitation peaks and storm injection peaks in low-altitude energetic electron spectra Differences between transmitter precipitation peaks and storm injection peaks in low-altitude energetic electron spectra

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jgra..11112202d&link_type=abstract

Journal of Geophysical Research, Volume 111, Issue A12, CiteID A12202

Physics

Plasma Physics

3

Space Plasma Physics: Wave/Particle Interactions (2483, 6984), Space Plasma Physics: Active Perturbation Experiments, Space Plasma Physics: Charged Particle Motion And Acceleration, Space Plasma Physics: Particle Acceleration

Scientific paper

Peaks in the energy spectrum of energetic radiation belt electrons (100 keV to 1 MeV) are evidence of pitch angle scattering by wave-particle interactions. Low-altitude satellites in the inner magnetosphere have reported two types of spectral peaks, corresponding to two different scattering mechanisms. However, previously published reports have focused on either on one type or on the other type of peak. We present here a side-by-side comparison of the two kinds of spectral phenomena in order to make clear the differences between them.

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