Online Resource
Cambridge University Press (CUP)
;
1993
In:
Symposium - International Astronomical Union Vol. 157 ( 1993), p. 59-61
In:
Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 157 ( 1993), p. 59-61
Abstract:
A short compilation of various radio methods of the determination of magnetic fields in the solar corona is given which, completed by observations in other spectral ranges (e.g. the optical and X-ray ranges), results in a complex picture of the magnetic field. Some topics of interest are the following: (1) Comparison with a standard reference magnetic field in the solar corona, (2) Possible evidence of substantial small-scale fluctuations of the magnetic field (e.g. in active regions), (3) Indication of magnetic fields substantially in excess of the standard distribution (e.g. in limb flare events).
Type of Medium:
Online Resource
ISSN:
0074-1809
DOI:
10.1017/S0074180900173875
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
1993
SSG:
16,12
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