VARIATIONS IN SOLAR MAGNETIC ACTIVITY DURING THE LAST 200 000 YEARS: IS THERE A SUN-CLIMATE CONNECTION?

dc.contributor.authorSharma M.
dc.date.accessioned2021-09-28T02:28:14Z
dc.date.available2021-09-28T02:28:14Z
dc.date.issued2002
dc.description.abstractThe production of 10Be in the Earth’s atmosphere depends on the galactic cosmic ray influx that, in turn, is affected by the solar surface magnetic activity and the geomagnetic dipole strength. Using the estimated changes in 10Be production rate and the geomagnetic field intensity, variations in solar activity are calculated for the last 200 ka. Large variations in the solar activity are evident with the Sun experiencing periods of normal, enhanced and suppressed activity. The marine δ18O record and solar modulation are strongly correlated at the 100 ka timescale. It is proposed that variations in solar activity control the 100 ka glacial–interglacial cycles. However, the 10Be production rate variations may have been under-estimated during the interval between 115 ka and 125 ka and may have biased the results. Future tests of the hypothesis are discussed.
dc.identifierhttps://elibrary.ru/item.asp?id=14051305
dc.identifier.citationEarth and Planetary Science Letters, 2002, 199, 3-4, 459-472
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/30615
dc.titleVARIATIONS IN SOLAR MAGNETIC ACTIVITY DURING THE LAST 200 000 YEARS: IS THERE A SUN-CLIMATE CONNECTION?
dc.typeСтатья

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