An analysis of apparent r-mode oscillations in solar activity, the solar diameter, the solar neutrino flux, and nuclear decay rates, with implications concerning the Sun’s internal structure and rotation, and neutrino processes-Reference-Cited by-同舟云学术

An analysis of apparent r-mode oscillations in solar activity, the solar diameter, the solar neutrino flux, and nuclear decay rates, with implications concerning the Sun’s internal structure and rotation, and neutrino processes

Published:2013-02 Issue: Volume:42 Page:62-69
ISSN:0927-6505
Container-title:Astroparticle Physics
language:en
Short-container-title:Astroparticle Physics

Author:

Sturrock P.A.,Bertello L.,Fischbach E.,Javorsek D.,Jenkins J.H.,Kosovichev A.,Parkhomov A.G.

Publisher

Elsevier BV

Subject

Astronomy and Astrophysics

Reference48 articles.

1. A 154-day periodicity in the occurrence of hard solar flares?

2. Periodicities in Solar Flare Occurrence: Analysis of Cycles 19–23

3. Rossby‐Type Wave–Induced Periodicities in Flare Activities and Sunspot Areas or Groups during Solar Maxima

4. MAGNETIC ROSSBY WAVES IN THE SOLAR TACHOCLINE AND RIEGER-TYPE PERIODICITIES

5. R-mode oscillations in uniformly rotating stars

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