The Contribution of Magnetic Flux Tubes to Brightness Fluctuations on the Extreme Limb of the Sun

Details The Contribution of Magnetic Flux Tubes to Brightness Fluctuations on the Extreme Limb of the Sun The Contribution of Magnetic Flux Tubes to Brightness Fluctuations on the Extreme Limb of the Sun

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998soph..183..277k&link_type=abstract

Solar Physics, v. 183, Issue 2, p. 277-282 (1998).

Physics

2

Scientific paper

Magnetic flux tubes are considered to be a possible source of observed brightness variations on the extreme limb of the Sun. A computer code to simulate the brightness fluctuations is developed. It follows from numerical modeling that a filling factor of f=4% is required to explain the observed fine structure. Such a value is typical for the boundaries of supergranules. Tubes produce a local maximum of intensity just inside the limb.

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