Possibilities and problems of the interpretation of solar magnetograph measurements and applications to flare-active regions

Details Possibilities and problems of the interpretation of solar magnetograph measurements and applications to flare-active regions Possibilities and problems of the interpretation of solar magnetograph measurements and applications to flare-active regions

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285..123s&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Reconnection in Space Plasma, Volume 2 p 123-128 (SEE N89-24974 1

Physics

2

Magnetic Measurement, Magnetic Signatures, Solar Flares, Solar Magnetic Field, Data Sampling, Solar Activity

Scientific paper

The basic uncertainties encountered in the interpretation of magnetograph data, and possibilities for deriving more reliable information are reviewed. The problems are illustrated by describing the data handling of a vector magnetograph. Examples of observed flare-active regions demonstrate the state of information which can be obtained.

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