Intra-network flux concentrations

Details Intra-network flux concentrations Intra-network flux concentrations

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cha%26a..12..241w&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 12, Issue 3, p. 241-248.

Astronomy and Astrophysics

Astrophysics

Scientific paper

On 1984 July 9, we obtained continuous magnetograms with 1``-2'' spatial resolution, 2.5min time resolution and noise level below 5 Gauss at Big Bear Solar Observatory. 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 uni-polar flux forms. These features have a typical size of 2``-5'' in one dimension, a total flux of (+18) Mx, a field strength of approximately 40G and a lifetime of several hours. We call these Intra-Network Flux Concentrations (INFC).

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