The reconnection of magnetic field lines in the solar corona

Details The reconnection of magnetic field lines in the solar corona The reconnection of magnetic field lines in the solar corona

Publishing date

Mar 1975

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l.129s&link_type=abstract

Journals

Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 2, p. L129-L131. NASA-supported research.

Science

Astronomy and Astrophysics

Field

Astronomy

Additional info 2

27

Additional info 3

Lines Of Force, Magnetic Signatures, Solar Corona, Solar Magnetic Field, Spectroheliographs, Magnetic Dipoles, Magnetic Flux, Skylab Program, Spaceborne Astronomy

Type

Scientific paper

Abstract

Skylab XUV coronal spectroheliograms and photospheric magnetograms are
compared. This comparison shows that, as new bipolar magnetic fields
emerge through the solar surface into the corona, the new coronal fields
interact with the old ones in a manner that suggests the reconnection of
the field lines.

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