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C. P. Burgess, N. S. Dzhalilov, T. I. Rashba, V. B. Semikoz and J. W. F. Valle, “Resonant Origin for Density Fluctuations Deep within the Sun: Helioseismology and Magneto-Gravity Waves,” Monthly Notices of the Royal Astronomical Society, Vol. 348, No. 2, 2004, pp. 609-624. doi:10.1111/j.1365-2966.2004.07392.x

has been cited by the following article:

• TITLE: Quasi-Biennial Modulation of the Solar Neutrino Flux: A “Telescope” for the Solar Interior

  AUTHORS: Loris D’Alessi, Antonio Vecchio, Vincenzo Carbone, Monica Laurenza, Marisa Storini

  KEYWORDS: Solar Neutrinos; Solar Cycle; Solar Interior

  JOURNAL NAME: Journal of Modern Physics, Vol.4 No.4A, April 30, 2013

  ABSTRACT: An oscillating magnetic field deep within the solar radiative region can significantly alter the helioseismic g-modes. The presence of density gradients along g-modes, can excite Alfvén waves resonantly, the resulting waveforms show sharp spikes in the density profile at radii comparable with the neutrino’s resonant oscillation length. This process should explain the observed quasi-biennial modulation of the solar neutrino flux. If confirmed, the coupling between solar neutrino flux and g-modes should be used as a “telescope” for the solar interior.