by V. Antonelli, L. Miramonti, C. Pena-Garay, A. Serenelli
Publisher: arXiv 2012
Number of pages: 51
After reviewing the striking results of the last two decades, which were determinant to solve the long standing solar neutrino puzzle and refine the Standard Solar Model, we focus our attention on the more recent results in this field and on the experiments presently running or planned for the near future.
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by James Schombert - University of Oregon
The purpose of this course is to educate you on the basic science behind our exploration of the Solar System so you may make informed choices as future/current voters on issues of our environment and the future of science in this country.
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Here we describe the magnetic field from the convection zone, where it is built up by the solar dynamo, to the solar surface, where it manifests itself in the form of sunspots and faculae, and beyond into the solar atmosphere and heliosphere.
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Helioseismology studies the structure and dynamics of the Sun's interior by observing oscillations on the surface. The basic principles, recent advances and perspectives of global and local helioseismology are reviewed in this text.
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