Solar Photosphere: Filigree

Details Solar Photosphere: Filigree Solar Photosphere: Filigree

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2254m&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2254. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Atmosphere

Scientific paper

The solar filigree (figure 1) is a pattern of strings of small bright points, visible in the SOLAR PHOTOSPHERE located in the dark lanes which separate granules. Its origin is magnetic, and each bright point is the site of a magnetic flux tube (see the fourth section). The solar filigree was first observed in the wings of the Hα line at 6563 Å, at the Sacramento Peak Observatory, in 1972, by Dunn...

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