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About: 160-minute solar cycle     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Process100029677, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: yago:WikicatSolarPhenomenayago:Phenomenon100034213yago:PhysicalEntity100001930yago:Process100029677 New Facet based on Instances of this Class

The 160-minute solar cycle was an apparent periodic oscillation in the solar surface which was observed in a number of early sets of data collected for helioseismology. The presence of a 160 minute cycle in the Sun is not substantiated by contemporary solar observations, and the historical signal is considered by mainstream scientists to occur as the redistribution of power from the diurnal cycle as a result of the observation window and atmospheric extinction.