Relative timing of solar prompt gamma-ray line and X-ray emission expected from a trap plus precipitation model for protons and electrons

Details Relative timing of solar prompt gamma-ray line and X-ray emission expected from a trap plus precipitation model for protons and electrons Relative timing of solar prompt gamma-ray line and X-ray emission expected from a trap plus precipitation model for protons and electrons

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213..383h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 383-396.

Astronomy and Astrophysics

Astrophysics

20

Gamma Ray Spectra, Line Spectra, Solar Electrons, Solar Protons, Solar X-Rays, Electron Precipitation, Emission Spectra, Proton Precipitation, Solar Flares, Trapped Particles

Scientific paper

Hard X-ray and prompt gamma-ray line emissions are the most direct signatures of respectively electron and ion acceleration during solar flares. A model is presented describing the time dependent transport of energetic ions from the acceleration region to the interaction volume. The temporal evolution of some of the prompt gamma-ray lines produced by the protons once they have reached deep and dense layers is predicted. The relative timing of gamma-rays and of hard X-rays produced by electrons simultaneously injected in the same coronal loop is examined and the results are discussed in the frame of existing observations.

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