Solar activity during Skylab: Its distribution and relation to coronal holes

Details Solar activity during Skylab: Its distribution and relation to coronal holes Solar activity during Skylab: Its distribution and relation to coronal holes

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7822994s&link_type=abstract

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Computer Science

Satellite Observation, Skylab Program, Solar Activity, Solar Corona, Histograms, Life (Durability), Magnetic Properties, Solar Cycles

Scientific paper

Solar active regions observed during the period of Skylab observations (May 1973-February 1974) were examined for properties that varied systematically with location on the sun, particularly with respect to the location of coronal holes. Approximately 90 percent of the optical and X-ray flare activity occurred in one solar hemisphere (136-315 heliographic degrees longitude). Active regions within 20 heliographic degrees of coronal holes were below average in lifetimes, flare production, and magnetic complexity. Histograms of solar flares as a function of solar longitude were aligned with H alpha synoptic charts on which active region serial numbers and coronal hole boundaries were added.

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