Solar neutrinos, solar activity cycle and quasibiennial variation

Details Solar neutrinos, solar activity cycle and quasibiennial variation Solar neutrinos, solar activity cycle and quasibiennial variation

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....7..108r&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 7 (A85-2

Physics

Solar Activity, Solar Cycles, Solar Neutrinos, Annual Variations, Argon Isotopes

Scientific paper

From the observed solar neutrino flux, it is shown that annual, 11-year, and quasi-biennial variation (nonstationary) of solar neutrino flux exist. It is pointed out that the appearance of quasi-biennial variation is due to the interaction of the solar core with the solar surface layers. This interaction occurs just before the sunspot maximum, and it decays before the sunspot minimum. During the interaction, a large amount of He-3 is mixed periodically in the core so that the rate of reaction He-3 + He-4 - Be-7 + gamma varies periodically; thus, quasi-biennial variation in the solar neutrino flux occurs during the solar activity cycle.

Affiliated with

Also associated with

No associations

Rating

Solar neutrinos, solar activity cycle and quasibiennial variation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Solar neutrinos, solar activity cycle and quasibiennial variation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar neutrinos, solar activity cycle and quasibiennial variation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-745856