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Multi-Wavelength Investigations of Solar Activity (IAU S223)

Multi-Wavelength Investigations of Solar Activity (IAU S223)

£68.00

Part of Proceedings of the International Astronomical Union Symposia and Colloquia

  • Date Published: May 2005
  • availability: In stock
  • format: Hardback
  • isbn: 9780521851954

£ 68.00
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  • These Proceedings present the most recent results from the highly successful international solar space missions (SOHO, CORONAS-F, TRACE, RHESSI, YOHKOH) and ground observatories around the Earth, reported at the IAU Symposium 223 held in St Petersburg, Russia, June 14-19, 2004. These include discussions of the current theories of solar dynamics and activity, new constraints provided by the multi-wavelength observations of the Sun from the interior to the heliosphere, as well as discussions of future coordinated plans and efforts of multi-wavelength investigations of the Sun. The Proceedings contain the material of seven plenary sessions and three round-table discussions: Relationship between solar and stellar activities, Coordination of observations and data analysis for CORONAS-F, SOHO, and related projects, and Analysis and interpretation of historical solar activity data. This volume includes 26 review papers covering all aspects of solar activity studies, and more than 200 contributed papers.

    • The most recent results from international solar space missions
    • Proceedings from conference of the International Astronomical Union
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    Product details

    • Date Published: May 2005
    • format: Hardback
    • isbn: 9780521851954
    • length: 760 pages
    • dimensions: 254 x 182 x 37 mm
    • weight: 1.56kg
    • contains: 418 b/w illus. 28 tables
    • availability: In stock
  • Table of Contents

    Section I: Solar Cycle in the Interior, Atmosphere and Heliosphere
    Section II-III: Structure and Evolution of Active Regions from the Sub-Photospheric Layers to the Corona, Filaments and Prominences
    Section IV: Multi-Scale Coronal Structures and Links to Photospheric Magnetic Field
    Section V: Energy Transport, Storage and Release in the Solar Atmosphere and Corona
    Section VI: Heliospheric Effects and Space Weather Research
    Section VII: Multi-Wavelength Observations of the Sun from Ground and Space.

  • Editors

    Alexander V. Stepanov, Pulkovo Observatory, St. Petersburg

    Elena E. Benevolenskaya, Stanford University, California

    Alexander G. Kosovichev, Stanford University, California

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