Flux, Evolution and Velocity Pattern of Solar Intranetwork Magnetic Fields

Details Flux, Evolution and Velocity Pattern of Solar Intranetwork Magnetic Fields Flux, Evolution and Velocity Pattern of Solar Intranetwork Magnetic Fields

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aspc..184..222w&link_type=abstract

Third Advances in Solar Physics Euroconference: Magnetic Fields and Oscillations, ASP Conference Series vol.184, p. 222-226. Eds

Physics

Sun: Magnetic Field, Sun: Intranetwork

Scientific paper

In this paper we summarized the primary results in the studies of solar intranetwork (IN) magnetic fields, based mainly on a set of the best time sequence of Big Bear magnetograms ever obtained. More than 2,500 individual intranetwork elements were identified and their flux measured; more than 500 elements were followed from birth to death, which allowed accurate estimation of flux evolution and velocity pattern.

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