Mathematics – Logic
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..221g&link_type=abstract
In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:
Mathematics
Logic
Neutrino Flux, Solar Magnetic Field, Diameter
Scientific paper
The study of the Sun as a variable star on a short time scale has been performed using the results of different experiments provided the measurements of global solar neutrino characteristics. The phenomenological model of temporal behavior was suggested based on 20-year long solar neutrino counting rate in Homestake detector. This model is used to describe and to predict the measurements of neutrino counting rate, solar diameter and magnetic field. From the comparison of this model with observations follows clearly that the model is valid for description of neutrino flux measurements by Cl-Ar and Ga-Ge detectors and radius of the Sun and it works perfectly for the prediction of the global magnetic field. Temporal behavior of solar global magnetic field during last 7 years since 1994 up to now is in a good agreement with the prediction of the phenomenological model based on the neutrino registration in Homestake taken from 1971 to 1991. The correlation between neutrino flux counting rate and diameter and their anti-correlation with magnetic field are demonstrated. Comparison with the perturbations of the geomagnetic field has been performed.
Gavryusev Vladimir
Gavryuseva Elena
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