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OverviewThe global structure of the heliosphere changes dramatically with the solar circle. Our knowledge of the heliosphere in three dimensions under solar-minimum conditions has advanced significantly in the last 10 years, largely as a result of the on-going ESA/NASA Ulysses mission. Similar advances in our understanding of the heliosphere at solar maximum are to be expected with the return of Ulysses to the Sun's polar regions in 2000/2001. The papers in this volume address a wide range of topics related to the solar-maximum heliosphere, and include many of the latest findings from Ulysses and other space-based missions. Ground-based studies and theoretical modeling are also well represented. Specific questions include: what are the dominant processes that determine the global structure of the inner heliosphere under conditions of high solar activity, and what are the key differences between the high-latitude heliosphere at solar maximum and solar minimum? The book is intended for those carrying out active research in the fields of solar and heliospheric physics. Full Product DetailsAuthor: R.G. MarsdenPublisher: Springer Imprint: Springer Edition: Softcover reprint of the original 1st ed. 2001 Weight: 0.748kg ISBN: 9789048157235ISBN 10: 9048157234 Pages: 431 Publication Date: 15 December 2010 Audience: Professional and scholarly , Professional & Vocational Format: Paperback Publisher's Status: Active Availability: Out of stock  The supplier is temporarily out of stock of this item. It will be ordered for you on backorder and shipped when it becomes available. Table of ContentsSection 1: The Sun and Corona Near Solar Maximum.- Section 2: The Large-Scale Structure of the Heliophere Near Solar Maximum.- Section 3: Energetic Particles in the Heliosphere.- Section 4: Cosmic Rays in the Heliosphere.- Section 5: The Heliosphere in the Local Interstellar Medium.- Author Index.- List of Participants.ReviewsAuthor InformationTab Content 6Author Website:Countries AvailableAll regions |
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