Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...163..239m&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 163, no. 1-2, July 1986, p. 239-245.
Astronomy and Astrophysics
Astrophysics
12
Bursts, Electron Capture, Solar Electrons, Solar Flares, Solar X-Rays, Time Dependence, Electron Distribution, Particle Acceleration, Radiant Flux Density, Time Lag
Scientific paper
The behavior of the spatially homogeneous electron trap model of solar hard X-ray bursts is analyzed, allowing for possible temporal variation of ambient density. Significant departures from the constant density case are found. Delays in excess of those possible in the static trap model may occur, without appeal to additional acceleration. Also the time profile of the X-ray flux may reflect the fast electron source function, rather than the actual instantaneous electron population. Large delays between hard X-rays and microwaves are a likely consequence of this. The implications of the present results for inference of gradual phase acceleration processes are discussed as well as those of the site of the hard X-ray emission. It is emphasized that consideration of the possible effects of time-dependent density is necessary for reliable inference of the importance of any acceleration processes.
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