Initial pitch-angle of narrowly beamed electrons injected into a magnetic mirror, formation of trapped and precipitating electron distribution, and asymmetry of hard X-ray and microwave footpoint emissions

Details Initial pitch-angle of narrowly beamed electrons injected into a magnetic mirror, formation of trapped and precipitating electron distribution, and asymmetry of hard X-ray and microwave footpoint emissions Initial pitch-angle of narrowly beamed electrons injected into a magnetic mirror, formation of trapped and precipitating electron distribution, and asymmetry of hard X-ray and microwave footpoint emissions

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007newa...12..483h&link_type=abstract

New Astronomy, Volume 12, Issue 6, p. 483-489.

Astronomy and Astrophysics

Astronomy

3

Magnetic Mirrors, Gas Dynamic Traps

Scientific paper

A new kind of static distribution function for trapped and precipitating electrons is derived by solving a time-independent Fokker Planck equation in a magnetic mirror, with injection of initially narrow-beamed electrons at an arbitrary initial pitch-angle. There are two independent parameters to determine the ratio of trapped and precipitating electrons, as well as their emissions, i.e., the mirror ratio and the initial pitch-angle, which is helpful for understanding some new features of asymmetrical hard X-ray and microwave footpoint emissions in solar observations.

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