Feasibility of detecting high-energy electrons in the solar corona from the synchrotron emission

Details Feasibility of detecting high-energy electrons in the solar corona from the synchrotron emission Feasibility of detecting high-energy electrons in the solar corona from the synchrotron emission

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974izssr..38.1842v&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Kharkov, Ukrainian SSR, Sept. 25-28, 1973.) Akademiia Nauk SSSR, Izv

Physics

Electron Counters, High Energy Electrons, Solar Corona, Solar Electrons, Synchrotron Radiation, Infrared Spectra, K Lines, Optical Emission Spectroscopy, Solar Flares, Solar Spectra

Scientific paper

It is proven analytically that electrons can be detected, and their characteristics identified, from their synchrotron emission in the optical spectral range. The feasibility of determining the principal characteristics of electrons accelerated by solar flares is based on studying the electron synchrotron emission from measurements of the spectral brightness of the active K-corona within the visible and IR regions of the spectrum.

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