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- Q4551085 subject Q7060964.
- Q4551085 abstract "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 main-stream scientists to occur as the redistribution of power from the diurnal cycle as a result of the observation window and atmospheric extinction.".
- Q4551085 wikiPageWikiLink Q1068381.
- Q4551085 wikiPageWikiLink Q320638.
- Q4551085 wikiPageWikiLink Q4916811.
- Q4551085 wikiPageWikiLink Q525.
- Q4551085 wikiPageWikiLink Q5570538.
- Q4551085 wikiPageWikiLink Q6555326.
- Q4551085 wikiPageWikiLink Q7060964.
- Q4551085 comment "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 main-stream scientists to occur as the redistribution of power from the diurnal cycle as a result of the observation window and atmospheric extinction.".
- Q4551085 label "160-minute solar cycle".