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Corotating Interaction Regions (SPACE SCIENCES SERIES OF ISSI Volume 7)
H. Kunrow
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Description for Corotating Interaction Regions (SPACE SCIENCES SERIES OF ISSI Volume 7)
Hardcover. Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland Editor(s): Balogh, A.G.; Gosling, J.T.; Jokipii, J. R; Kallenbach, Reinald (International Space Science Institute, Bern, Switzerland); Kunow, H. Series: Space Sciences Series of ISSI. Num Pages: 411 pages, 47 black & white illustrations, 13 colour illustrations, biography. BIC Classification: PGS; PHFP. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. Dimension: 246 x 168 x 22. Weight in Grams: 912. Proceedings of an ISSI Workshop, 6-13 June, 1998, Bern, Switzerland. Series: Space Sciences Series of ISSI. 426 pages, Illustrations (some col.). Editor(s): Balogh, A.G.; Gosling, J.T.; Jokipii, J. R; Kallenbach, Reinald (International Space Science Institute, Bern, Switzerland); Kunow, H. Offers an integrated overview of the knowledge and understanding of corotating interaction regions (CIRs) in the solar wind. Papers included in this book cover the subject of CIRs from their dissipation in the outer hemisphere, and include discussions of complexities associated with their evolution with distance from the Sun. Cateogry: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly. BIC Classification: PGS; PHFP. Dimension: 246 x 168 x 22. Weight: 912.
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that ... Read more
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that ... Read more
Product Details
Format
Hardback
Publication date
2000
Publisher
Springer
Number of pages
425
Condition
New
Series
Space Sciences Series of ISSI
Number of Pages
411
Place of Publication
Dordrecht, Netherlands
ISBN
9780792360803
SKU
V9780792360803
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15
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