Physics
Scientific paper
Jan 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008georl..3502815d&link_type=abstract
Geophysical Research Letters, Volume 35, Issue 2, CiteID L02815
Physics
28
Magnetospheric Physics: Energetic Particles: Precipitating, Atmospheric Processes: Atmospheric Electricity, Atmospheric Processes: Lightning
Scientific paper
Using CGRO/BATSE data, a possible new source of high-energy electrons and positrons in the earth's inner magnetosphere is presented. These particles are generated within the upper atmosphere by Compton scattering and pair-production of gamma-rays originating from near the tropopause as Terrestrial Gamma-ray Flashes (TGFs). Once created, these energetic electrons and positrons follow the geomagnetic field into the inner magnetosphere where they can be detected in low-earth orbit, either near the TGF magnetic foot point or at the conjugate point several thousand kilometers away. Approximately 17% of CGRO/BATSE events previously identified as terrestrial gamma-ray flashes are, in fact, such electrons and positrons. With energies extending above 30 MeV, this previously unidentified population contains some of the most energetic particles accelerated in the near-earth environment.
Dwyer Joseph R.
Grefenstette Brian W.
Smith Masson D.
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