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100%: Charles F. Kennel: Convection and Substorms: Paradigms of Magnetospheric Phenomenology (ISBN: 9780195359077) in Englisch, auch als eBook.Nur diese Ausgabe anzeigen…
100%: KENNEL, CHARLES F.: CONVECTION AND SUBSTORMS: PARADIGMS OF MAGNETOSPHERIC PHENOMENOLOGY (INTERNATIONAL SERIES ON ASTRONOMY AND ASTROPHYSICS, 2) (ISBN: 9780195085297) Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, in Englisch, Broschiert.Nur diese Ausgabe anzeigen…
Convection and Substorms: Paradigms of Magnetospheric Phenomenology
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Convection and Substorms - Paradigms of Magnetospheric Phenomenology
~EN NW EB DLISBN: 9780195359077 bzw. 0195359070, vermutlich in Englisch, Oxford University Press, neu, E-Book, elektronischer Download.
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Convection and Substorms: 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. Englisch, Ebook.
Convection and Substorms: 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. Englisch, Ebook.
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Convection and Substorms: Paradigms of Magnetospheric Phenomenology : Paradigms of Magnetospheric Phenomenology
EN NW EB DLISBN: 9780195359077 bzw. 0195359070, in Englisch, Oxford University Press, neu, E-Book, elektronischer Download.
Lieferung aus: Vereinigtes Königreich Großbritannien und Nordirland, Despatched same working day before 3pm.
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.
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.
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Convection and Substorms: Paradigms of Magnetospheric Phenomenology (International Series on Astronomy and Astrophysics)
EN HC USISBN: 9780195085297 bzw. 0195085299, in Englisch, Oxford University Press, gebundenes Buch, gebraucht.
Lieferung aus: Vereinigte Staaten von Amerika, Versandkosten nach: USA.
Von Händler/Antiquariat, Books Express.
Oxford University Press. Hardcover. Good. Ships with Tracking Number! International Shipping available. Ships with Tracking Number! May not contain Access Codes or Supplements. Buy with confidence, excellent customer service! d.
Von Händler/Antiquariat, Books Express.
Oxford University Press. Hardcover. Good. Ships with Tracking Number! International Shipping available. Ships with Tracking Number! May not contain Access Codes or Supplements. Buy with confidence, excellent customer service! d.
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Convection and Substorms, Paradigms of Magnetospheric Phenomenology (1996)
EN HC NWISBN: 9780195085297 bzw. 0195085299, in Englisch, Oxford University Press Inc, gebundenes Buch, neu.
Lieferung aus: Niederlande, Vermoedelijk 2-3 weken.
bol.com.
The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics... The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the steady reconnection model be replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Taal: Engels;Afmetingen: 34x243x163 mm;Gewicht: 781,00 gram;Verschijningsdatum: april 1996;ISBN10: 0195085299;ISBN13: 9780195085297; Engelstalig | Hardcover | 1996.
bol.com.
The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics... The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the steady reconnection model be replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.Taal: Engels;Afmetingen: 34x243x163 mm;Gewicht: 781,00 gram;Verschijningsdatum: april 1996;ISBN10: 0195085299;ISBN13: 9780195085297; Engelstalig | Hardcover | 1996.
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Convection and Substorms: Paradigms of Magnetospheric Phenomenology (International Series on Astronomy and Astrophysics) (1996)
EN HC USISBN: 9780195085297 bzw. 0195085299, in Englisch, Oxford University Press, USA, gebundenes Buch, gebraucht.
Lieferung aus: Vereinigte Staaten von Amerika, Versandkosten nach: USA.
Von Händler/Antiquariat, Ergodebooks.
Oxford University Press, USA, 1996-02-08. Hardcover. Good. Buy with confidence. Excellent Customer Service & Return policy. Ships Fast. Expedite Shipping Available.
Von Händler/Antiquariat, Ergodebooks.
Oxford University Press, USA, 1996-02-08. Hardcover. Good. Buy with confidence. Excellent Customer Service & Return policy. Ships Fast. Expedite Shipping Available.
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CONVECTION AND SUBSTORMS: PARADIGMS OF MAGNETOSPHERIC PHENOMENOLOGY (INTERNATIONAL SERIES ON ASTRONOMY AND ASTROPHYSICS, 2)
EN USISBN: 9780195085297 bzw. 0195085299, in Englisch, Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, gebraucht.
Lieferung aus: Indien, Versandkosten nach: USA.
Von Händler/Antiquariat, BOOKS INTERNATIONAL.
Used - Very Good. Very good condition.
Von Händler/Antiquariat, BOOKS INTERNATIONAL.
Used - Very Good. Very good condition.
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Convection and Substorms: Paradigms of Magnetospheric Phenomenology (1995)
EN USISBN: 9780195085297 bzw. 0195085299, in Englisch, Oxford University Press, gebraucht.
Lieferung aus: Vereinigte Staaten von Amerika, Versandkosten nach: USA.
Von Händler/Antiquariat, bookstore brengelman.
Oxford University Press. As New/No Jacket. 1995. 0195085299 .
Von Händler/Antiquariat, bookstore brengelman.
Oxford University Press. As New/No Jacket. 1995. 0195085299 .
8
Convection and Substorms: Paradigms of Magnetospheric Phenomenology
EN NW EB DLISBN: 9780195359077 bzw. 0195359070, in Englisch, Oxford University Press, Vereinigtes Königreich Großbritannien und Nordirland, neu, E-Book, elektronischer Download.
Lieferung aus: Deutschland, zzgl. Versandkosten.
Paradigms of Magnetospheric Phenomenology, Paradigms of Magnetospheric Phenomenology.
Paradigms of Magnetospheric Phenomenology, Paradigms of Magnetospheric Phenomenology.
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