Solar Electromagnetic Radiation Study for Solar Cycle 22

. Ed(s): Pap, Judit M.; Frohlich, Claus; Ulrich, Roger K. (Dept. of Physics and Astronomy)

ISBN 10: 0792349997 / ISBN 13: 9780792349990

Published by Kluwer Academic Publishers, 1998

About this Item

Proceedings of the SOLERS22 Workshop held at the NSO/Sac Peak, Sunspot, NM, U.S.A., June 17-21, 1996 Editor(s): Pap, Judit M.; Frohlich, Claus; Ulrich, Roger K. (Dept. of Physics and Astronomy). Num Pages: 517 pages, biography. BIC Classification: PGS; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 244 x 170 x 30. Weight in Grams: 923. . 1998. Reprinted from SOLAR PHYSICS, 177, 1998. Hardback. . . . . Books ship from the US and Ireland.

Seller Inventory # V9780792349990

Bibliographic Details

• Title: Solar Electromagnetic Radiation Study for Solar Cycle 22
• Publisher: Kluwer Academic Publishers
• Publication Date: 1998
• Language: English
• ISBN 10: 0792349997
• ISBN 13: 9780792349990
• Binding: Hardcover
• Condition: New

About this title

Synopsis

Measurements of solar irradiance, both bolometric and at various wavelengths, over the last two decades have established conclusively that the solar energy flux varies on a wide range of time scales, from minutes to the 11-year solar cycle. The major question is how the solar variability influences the terrestrial climate.
The Solar Electromagnetic Radiation Study for Solar Cycle 22 (SOLERS22) is an international research program operating under the auspices of the Solar-Terrestrial Energy Program (STEP) Working Group 1: `The Sun as a Source of Energy and Disturbances'. STEP is sponsored by the Scientific Committee of Solar-Terrestrial Physics (SCOSTEP) of the International Council of Scientific Unions (ICSU).
The main goal of the SOLERS22 1996 Workshop was to bring the international research community together to review the most recent results obtained from observations, theoretical interpretation, empirical and physical models of the variations in the solar energy flux and their possible impact on climate studies. These questions are essential for researchers and graduate students in solar-terrestrial physics.