Criteria for plasma-wave losses for electrons streaming from an acceleration region

Details Criteria for plasma-wave losses for electrons streaming from an acceleration region Criteria for plasma-wave losses for electrons streaming from an acceleration region

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...201..521s&link_type=abstract

Astrophysical Journal, vol. 201, Oct. 15, 1975, pt. 1, p. 521-525.

Astronomy and Astrophysics

Astrophysics

12

Astronomical Models, Electron Plasma, Particle Acceleration, Plasma Waves, Solar X-Rays, Bursts, Collisional Plasmas, Criteria, Energy Dissipation, Nonrelativistic Mechanics, Plasma-Particle Interactions

Scientific paper

Consistent criteria are derived for determining when losses due to collective excitation of electron plasma waves will be important for electrons streaming from an acceleration region. The analysis is nonrelativistic and one-dimensional, but includes the effect of Coulomb collisions. These criteria are applied to source models for solar hard X-ray bursts, and it is shown that these losses will almost never be important for the observations obtained thus far. The case in which the acceleration region and the X-ray source partially overlap is considered briefly.

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