The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
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The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
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No. 9780195359077. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten. Details...
(*) Derzeit vergriffen bedeutet, dass dieser Titel momentan auf keiner der angeschlossenen Plattform verfügbar ist.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
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No. 9780195359077. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten. Details...
(*) Derzeit vergriffen bedeutet, dass dieser Titel momentan auf keiner der angeschlossenen Plattform verfügbar ist.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The config… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur. Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field. Digital Content>E-books>Science>Space>Space, Oxford University Press Digital >16<
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(*) Derzeit vergriffen bedeutet, dass dieser Titel momentan auf keiner der angeschlossenen Plattform verfügbar ist.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
- No. 9780195359077. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
No. 9780195359077. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configu… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae.The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions.The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region.Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.; PDF; Scientific, Technical and Medical > Astronomy, space & time > Solar system: the Sun & planets, Oxford University Press<
No. 9780195359077. Versandkosten:Instock, Despatched same working day before 3pm, zzgl. Versandkosten.
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The config… Mehr…
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur. Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field. Digital Content>E-books>Science>Space>Space, Oxford University Press Digital >16<
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Detailangaben zum Buch - Convection and Substorms: Paradigms of Magnetospheric Phenomenology Charles F. Kennel Author
EAN (ISBN-13): 9780195359077 Erscheinungsjahr: 1996 Herausgeber: Oxford University Press Digital >16
Buch in der Datenbank seit 2007-02-26T04:35:01+01:00 (Berlin) Detailseite zuletzt geändert am 2023-12-01T01:25:00+01:00 (Berlin) ISBN/EAN: 9780195359077
ISBN - alternative Schreibweisen: 978-0-19-535907-7 Alternative Schreibweisen und verwandte Suchbegriffe: Autor des Buches: kennel, longenbach james Titel des Buches: phenomenology
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