Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...56..125b&link_type=abstract
Solar Physics, vol. 56, Jan. 1978, p. 125-151.
Astronomy and Astrophysics
Astronomy
52
Far Ultraviolet Radiation, Solar Corona, Solar Cycles, Solar Magnetic Field, Ultraviolet Astronomy, Lines Of Force, Magnetic Dipoles, Magnetic Flux, Magnetic Poles, Magnetic Signatures, Skylab Program
Scientific paper
Skylab and ground-based observations in the extreme UV range of the spectrum are used to analyze characteristics of coronal holes, and to correlate their development with variations in the solar cycle. The mergence of bipolar magnetic regions (BMR) during the declining phase of the cycle is held reponsible for the formation of large equatorial holes (M-regions, which cause recurring geomagnetic storms). The BMR mergence model can also be applied to polar cap holes.
Bohlin David J.
Sheeley Neil R. Jr.
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