POSSIBILITY OF ^DETERMINING EHE ■ MAGNETIC FTSID JNTEl^ITY IN THE ; QUEER SOLAS CORONA BY EXAMIWIKG .THE PROPAGATION OF IHE.jPQLAREED RADIATION OF DISCRETE SOURCES
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جذب تشدیدی و اتلاف امواج هیدرومغناطیسی در تاج خورشید
Although, the hot solar corona was discovered more than sixty years ago, however, the exact dissipation mechanism that heats the corona is still unknown. Resonant absorption and damping of Alfven waves appear to be one of the major candidates in this respect. The corona is highly structured and inhomogeneous medium, containing a large number of discrete magnetic loops. In this paper a cylindr...
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