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 Jay M. Pasachoff - Alpha
Everything revolves around it...and now you can learn all about the origin and history of the sun. With information on the sun's physical properties; how solar flares, sunspots, and winds on its surface affect Earth's atmosphere and environment.
by Sami Solanki, Bernd Inhester, Manfred Schussler - arXiv
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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This textbook studies the solar wind and other plasma environments. It is aimed for students of space physics. The text covers plasma physics, heliosphere, solar wind, magnetosphere, ionosphere, auroras, cosmic rays, space weather, etc.
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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.