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Diagnosis of coronal magnetic field with data of Nobeyama Radio Heliograph
DOI: 10.1016/S1384-1076(02)00088-X
Bibcode: 2002NewA....7..135H
Nakajima, Hiroshi; Huang, Guang-Li
The expression is derived for the coronal magnetic field strength from the observations of brightness, temperature, peak frequency, spectral index, and polarization degree of solar microwave bursts. One example of solar burst on November 28, 1998 is given for the calculation of coronal magnetic field from the data of Nobeyama Radio Heliograph (NoR…
2002
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New Astronomy
SOHO
16