Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux

Details Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..292..195k&link_type=abstract

Physics Letters B, Volume 292, Issue 1-2, p. 195-200.

Physics

14

Scientific paper

We show that if the twist of toroidal magnetic fields in the sun is sizeable, a seasonal oscillation of the solar neutrino flux occurs. Although the size of the twist is not known, the development of the twist is believed to be the origin of the cylic oscillations with polarity reversals of solar magnetic fields in every 11 years. We found that with some sizes of twists, both Cl and Kamiokande II data can be reproduced reasonably well. Especially, the fine up-down structure of the Cl data is interpreted as an effect of the twist.

Affiliated with

Also associated with

No associations

Rating

Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux 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 Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Twisting toroidal magnetic fields and the seasonal oscillation of the solar neutrino flux will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1871213