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The spectrum of gyrosynchrotron emission from solar flares generally peaks in the microwave range. Its optically-thin, high-frequency component, above the spectral peak, is often used for diagnostics of the nonthermal electrons and the magnetic field
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::999de2aaefd0b4f339507d6d9ead55fe
Publikováno v:
Astrophysical Journal; 11/1/2018, Vol. 867 Issue 1, p1-1, 1p
