Intra-network flux concentrations

Details Intra-network flux concentrations Intra-network flux concentrations

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acasn..29...48w&link_type=abstract

(Acta Astronomica Sinica, vol. 29, 1988, p. 48-57) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, Sept. 1988, p.

Astronomy and Astrophysics

Astrophysics

5

Magnetic Flux, Magnetic Signatures, Solar Magnetic Field, Polarity, Spatial Resolution

Scientific paper

On July 9, 1984, continuous magnetograms with 1-2 arcsec spatial resolution, 2.5 min time resolution, and noise level below 5 Gauss were obtained. Analysis of these magnetograms after calibration and empirical corrections shows that, in addition to the transient, mixed polarity field described by Livingston and Harvey (1975), there is a stable type of unipolar flux form. These features have a typical size of 2-5 arcsecs in one dimension, a total flux of (+18) Mx, a field strength of approximately 40 G and a lifetime of several hours. The features are called intranetwork flux concentrations (INFC).

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