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The representation of magnetic field lines from magnetograph data

โœ Scribed by Randolph H. Levine

Publisher
Springer
Year
1975
Tongue
English
Weight
310 KB
Volume
44
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

Several methods currently used to extrapolate the structure of the solar magnetic field from surface measurements are examined and compared. In particular, the differences between the methods of Schmidt for potential fields and of Nakagawa and Raadu for force-free fields are explained. Suggestions are made regarding the use of these theoretical procedures in making physical conclusions. * These four planes are defined by the relations xo<x<xl, O<z< 0% y~yo; xo<x<xl, O<z< 0% y=yl; yo<y<yl, O<z< ~, x=xo; yo<y<yl, O<z< ~, x=xl.

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