Synopsis
The Handbook of Solar-Terrestrial Environment is a unique compendium. Recognized international leaders in their field contribute chapters on basic topics of solar physics, space plasmas and the Earth's magnetosphere. The book further covers applied topics like the aurora, magnetospheric storms, space weather, space climatology and planetary science. This book will be of highest value as a reference for researchers working in the area of planetary and space science.
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Handbook of the Solar-Terrestrial Environment (eng)
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Handbook of the Solar-Terrestrial Environment
Edité par
Springer Berlin Heidelberg, 2010
ISBN 10 : 3642079687
ISBN 13 : 9783642079689
Neuf
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Vendeur : moluna, Greven, Allemagne
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Etat : New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. A unique compendium on the Solar-Terrestrial Environment by the leading experts worldwideContains parts on the Sun and the Solar Wind, the Earth, Space Plasmas, and on Processes and Phenomena in the Solar-Terrestrial EnvironmentA u. N° de réf. du vendeur 5047022
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Handbook of the Solar-Terrestrial Environment
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Handbook of the Solar-Terrestrial Environment
Edité par
Springer Berlin Heidelberg Nov 2010, 2010
ISBN 10 : 3642079687
ISBN 13 : 9783642079689
Neuf
Taschenbuch
Vendeur : BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Allemagne
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ing energy into space, as much as . erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di cult. rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth's the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than keV to more than GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci cally the close coupling of di erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment. 556 pp. Englisch. N° de réf. du vendeur 9783642079689
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Handbook of the Solar-Terrestrial Environment
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Handbook of the Solar-Terrestrial Environment
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Taschenbuch. Etat : Neu. Handbook of the Solar-Terrestrial Environment | Yohsuke Kamide (u. a.) | Taschenbuch | xiv | Englisch | 2010 | Springer | EAN 9783642079689 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. N° de réf. du vendeur 107220300
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Handbook of the Solar-Terrestrial Environment
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Handbook of the Solar-Terrestrial Environment
Edité par
Springer Berlin Heidelberg, Springer Nov 2010, 2010
ISBN 10 : 3642079687
ISBN 13 : 9783642079689
Neuf
Taschenbuch
Vendeur : buchversandmimpf2000, Emtmannsberg, BAYE, Allemagne
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ing energy into space, as much as . erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di cult. rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth¿s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than keV to more than GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci cally the close coupling of di erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment.Springer-Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 556 pp. Englisch. N° de réf. du vendeur 9783642079689
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Handbook of the Solar-Terrestrial Environment
Edité par
Springer Berlin Heidelberg, 2010
ISBN 10 : 3642079687
ISBN 13 : 9783642079689
Neuf
Taschenbuch
Vendeur : AHA-BUCH GmbH, Einbeck, Allemagne
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ing energy into space, as much as . erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di cult. rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth's the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than keV to more than GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci cally the close coupling of di erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment. N° de réf. du vendeur 9783642079689
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Handbook of the Solar-Terrestrial Environment
Edité par
J.B. Metzler, 2010
ISBN 10 : 3642079687
ISBN 13 : 9783642079689
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Etat : Hervorragend. Zustand: Hervorragend | Seiten: 556 | Sprache: Englisch | Produktart: Bücher | As a star in the universe, the Sun is constantly releas- cover a wide range of time and spatial scales, making ?? ing energy into space, as much as ? ? ?? erg/s. Tis observations in the solar-terrestrial environment c- energy emission basically consists of three modes. Te plicated and the understanding of processes di?cult. ?rst mode of solar energy is the so-called blackbody ra- In the early days, the phenomena in each plasma diation, commonly known as sunlight, and the second region were studied separately, but with the progress mode of solar electromagnetic emission, such as X rays of research, we realized the importance of treating and UV radiation, is mostly absorbed above the Earth¿s the whole chain of processes as an entity because of stratosphere. Te third mode of solar energy emission is strong interactions between various regions within in the form of particles having a wide range of energies the solar-terrestrial system. On the basis of extensive from less than ? keV to more than ? GeV. It is convenient satellite observations and computer simulations over to group these particles into lower-energy particles and thepasttwo decades, it hasbecomepossibleto analyze higher-energy particles, which are referred to as the so- speci?cally the close coupling of di?erent regions in the lar wind and solar cosmic rays, respectively. solar-terrestrial environment. N° de réf. du vendeur 9838881/1
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