Formation of Solar Magnetic Flux Tubes Observed with Hinode

Details Formation of Solar Magnetic Flux Tubes Observed with Hinode Formation of Solar Magnetic Flux Tubes Observed with Hinode

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..560n&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 10, p. 560 - 564 (2008)

Astronomy and Astrophysics

Astronomy

Scientific paper

The solar surface, photosphere, is covered with magnetic flux tubes with kilo gauss field strength and spacial scale of ~200 km. It has been believed that those flux tube areas formed through convective instability, however the hypothesis has lacked the observational support so far. The Solar Optical Telescope of Hinode revealed the formation of those flux tubes for the first time. The observation is well explained with the theoretical model predicted thirty years ago.

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