Dynamics of sub-relativistic electron beams in magnetic traps - A model for solar N-bursts

Details Dynamics of sub-relativistic electron beams in magnetic traps - A model for solar N-bursts Dynamics of sub-relativistic electron beams in magnetic traps - A model for solar N-bursts

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...195..301h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 195, no. 1-2, April 1988, p. 301-309. Research supported by the Greek General

Astronomy and Astrophysics

Astrophysics

13

Magnetically Trapped Particles, Plasma Interactions, Relativistic Electron Beams, Solar Radio Bursts, Type 3 Bursts, Coronal Loops, Solar Magnetic Field

Scientific paper

The dynamic evolution of mildly relativistic electrons (10 - 100 keV) injected into a model magnetic trap is studied numerically, using the drift approximation. Wave-particle interactions are neglected, since the beam plasma system is shown to be non-linearly decoupled in the range of parameters used in this study. The results from the simulation are used to interpret certain observational characteristics of the N-bursts observed by the Nançay radio spectrograph. N-bursts are believed to be the first direct radio evidence for mirror effects in solar magnetic loops.

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