Temporal dispersion structures of proton and electron bursts in the Earth's magnetotail

Details Temporal dispersion structures of proton and electron bursts in the Earth's magnetotail Temporal dispersion structures of proton and electron bursts in the Earth's magnetotail

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993p%26ss...41..461t&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 41, no. 6, p. 461-467

Mathematics

6

Analysis (Mathematics), Electrons, Geomagnetic Tail, Protons, Temporal Distribution, Velocity Distribution, Ampte (Satellites), Explorer 50 Satellite, Geomagnetism, Lorentz Force, Particle Motion

Scientific paper

We present an analytical approximation of the behavior of the velocity dispersion structure of the energetic particle bursts generated during magnetic field topology reconstruction within the Earth's magnetotail. We show that some critical distance S exists, such that if the distance S between the source and the spacecraft S greater than S(sub c), the burst exhibits only normal velocity dispersion (more energetic particles appear before low energy particles). For S less than S(sub c), both inverse (for higher energies) and normal (for lower energies) parts coexist in the structure. These calculations are compared with the observational data.

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