Solar Wind Magnetosphere Coupling (18 results)

Hardcover. Condition: Very Good. 807 pages, 8vo. No DJ. Shelfwear: scuffing along edges and covers, tanned page edges. Tight binding, no marks. Volume is in Very Good condition.

Condition: Fine. 1986th Edition. Used book that is in almost brand-new condition. May contain a remainder mark. Better World Books: Buy Books. Do Good.

Gr.-8°, original hardcover. 1. ed. XVI, 807 p. Stamp on preliminary page and title, otherwise fine copy. Sprache: Englisch Gewicht in Gramm: 0.

808 S. mit zahlreichen Abbildungen, (808 pp. with a lot of figures), 9027723036 Sprache: Englisch Gewicht in Gramm: 1550 Groß 8°, Original-Pappband (Hardcover), sauberes Exemplar, (fine copy),

Paperback. Condition: Brand New. 164 pages. 8.66x5.91x0.37 inches. In Stock.

Condition: New. In.

Condition: New. pp. 828.

Paperback. Condition: Brand New. 828 pages. 9.30x6.10x1.90 inches. In Stock.

Taschenbuch. Condition: Neu. Druck auf Anfrage Neuware - Printed after ordering - This monograph is the outgrowth of an AGU (American Geophysical Union) Chapman Conference on Solar Wind-Magnetosphere Coupling, and it contains most of the formal papers presented at the conference including the summary panel. The conference was held on February 12-15,1985 at the Jet Propulsion Laboratory of the California Institute of Technology in Pasadena, California, U.S.A. It was attended by over 150 scientists from most of the nations active in space research. The purpose of the conference was to bring together scientists from all areas of solar-terrestrial physics, both theoretical and experimental, in order to focus attention on the solar wind-magnetosphere coupling problem, to provide a timely forum for the exchange of ideas, and to promote interdisciplinary collaboration. The conference agenda consisted of eight sessions: six topical, one poster, and one summary. The topical sessions were 'Solar Wind and Geomagnetic Activity,' 'AM PTE Mission,' 'Solar Wind and Polar Cusp,' 'Auroral Zone and Polar Cap,' 'Solar Wind and Magnetotail,' and 'Theoretical Modeling and Simulations.' The conference concluded with a two-hour summary panel discussion which attempted to provide an assessment of the progress that has been made as well as underscore the problems, old and new, which remain unanswered. Sydney Chapman (1889-1970) was one of the early pioneers in the study of the influence of the sun and magnetosphere on the earth's upper atmosphere, and it was most appropriate that this conference be one in the AGU series named in his honor.

Paperback. Condition: Like New. Like New. book.

paperback. Condition: New. NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Condition: new. Questo è un articolo print on demand.

Taschenbuch. Condition: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This monograph is the outgrowth of an AGU (American Geophysical Union) Chapman Conference on Solar Wind-Magnetosphere Coupling, and it contains most of the formal papers presented at the conference including the summary panel. The conference was held on February 12-15,1985 at the Jet Propulsion Laboratory of the California Institute of Technology in Pasadena, California, U.S.A. It was attended by over 150 scientists from most of the nations active in space research. The purpose of the conference was to bring together scientists from all areas of solar-terrestrial physics, both theoretical and experimental, in order to focus attention on the solar wind-magnetosphere coupling problem, to provide a timely forum for the exchange of ideas, and to promote interdisciplinary collaboration. The conference agenda consisted of eight sessions: six topical, one poster, and one summary. The topical sessions were 'Solar Wind and Geomagnetic Activity,' 'AM PTE Mission,' 'Solar Wind and Polar Cusp,' 'Auroral Zone and Polar Cap,' 'Solar Wind and Magnetotail,' and 'Theoretical Modeling and Simulations.' The conference concluded with a two-hour summary panel discussion which attempted to provide an assessment of the progress that has been made as well as underscore the problems, old and new, which remain unanswered. Sydney Chapman (1889-1970) was one of the early pioneers in the study of the influence of the sun and magnetosphere on the earth's upper atmosphere, and it was most appropriate that this conference be one in the AGU series named in his honor. 828 pp. Englisch.

Taschenbuch. Condition: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Magnetic reconnection at the dayside magnetopause is one of the most important mechanisms that efficiently transfers solar wind particles, momentum, and energy into the Earth's magnetosphere. Cold dense plasma, originating either directly from the ionosphere or from the plasmasphere, has often been observed at the adjacent magnetopause. These cold plasmas may affect reconnection since they modify the plasma properties on the magnetospheric side significantly. Case and statistical studies of the characteristics of the cold ions observed at the dayside magnetopause are presented by using Cluster spacecraft datasets. The behavior of the cold dense plasma of ionospheric origin during magnetic reconnection at the dayside magnetopause, occurrence rates of plasmaspheric plumes and ionospheric outflows, and their dependence on the solar wind/Interplanetary Magnetic Field (IMF) conditions have been investigated. Finally, a controlling factor that leads to the asymmetric reconnection geometry at the magnetopause has been examined.

Condition: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This monograph is the outgrowth of an AGU (American Geophysical Union) Chapman Conference on Solar Wind-Magnetosphere Coupling, and it contains most of the formal papers presented at the conference including the summary panel. The conference was held on Feb.

Condition: New. Print on Demand pp. 828.

Condition: New. PRINT ON DEMAND pp. 828.

Taschenbuch. Condition: Neu. This item is printed on demand - Print on Demand Titel. Neuware -This monograph is the outgrowth of an AGU (American Geophysical Union) Chapman Conference on Solar Wind-Magnetosphere Coupling, and it contains most of the formal papers presented at the conference including the summary panel. The conference was held on February 12-15,1985 at the Jet Propulsion Laboratory of the California Institute of Technology in Pasadena, California, U.S.A. It was attended by over 150 scientists from most of the nations active in space research. The purpose of the conference was to bring together scientists from all areas of solar-terrestrial physics, both theoretical and experimental, in order to focus attention on the solar wind-magnetosphere coupling problem, to provide a timely forum for the exchange of ideas, and to promote interdisciplinary collaboration. The conference agenda consisted of eight sessions: six topical, one poster, and one summary. The topical sessions were 'Solar Wind and Geomagnetic Activity,' 'AM PTE Mission,' 'Solar Wind and Polar Cusp,' 'Auroral Zone and Polar Cap,' 'Solar Wind and Magnetotail,' and 'Theoretical Modeling and Simulations.' The conference concluded with a two-hour summary panel discussion which attempted to provide an assessment of the progress that has been made as well as underscore the problems, old and new, which remain unanswered. Sydney Chapman (1889-1970) was one of the early pioneers in the study of the influence of the sun and magnetosphere on the earth's upper atmosphere, and it was most appropriate that this conference be one in the AGU series named in his honor.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 828 pp. Englisch.