Discussion on the Weak Component of Solar Magnetism

Details Discussion on the Weak Component of Solar Magnetism Discussion on the Weak Component of Solar Magnetism

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..125w&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

Scientific paper

More pieces of evidence are found that the intranetwork fields are intrinsically weak. They contribute the most of solar magnetic flux. Further weak field components, currently below the detection capability, are implied by the small-scale activity on the quiet Sun. To detect the weak field elements, in addition to having very high angular resolution, the sensitivity of the magnetograph is a decisive factor.

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