Verlag: Berlin, Springer, 2007
Sprache: Englisch
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In den WarenkorbHardcover. Zustand: Sehr gut. 1st ed. XIV, 533 S. : Ill.; 25 Very good condition. Cover shows wear, otherwise very good condition. Sprache: Englisch Gewicht in Gramm: 1675.
Verlag: Springer Berlin Heidelberg, 2010
ISBN 10: 3642079687 ISBN 13: 9783642079689
Sprache: Englisch
Anbieter: Buchpark, Trebbin, Deutschland
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Verlag: Springer Berlin Heidelberg, Springer Berlin Heidelberg Aug 2007, 2007
ISBN 10: 3540463143 ISBN 13: 9783540463146
Sprache: Englisch
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In den WarenkorbBuch. Zustand: Neu. 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.
Verlag: Springer Berlin Heidelberg, Springer Berlin Heidelberg Nov 2010, 2010
ISBN 10: 3642079687 ISBN 13: 9783642079689
Sprache: Englisch
Anbieter: buchversandmimpf2000, Emtmannsberg, BAYE, Deutschland
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In den WarenkorbTaschenbuch. Zustand: Neu. 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.
Verlag: Springer Berlin Heidelberg, 2010
ISBN 10: 3642079687 ISBN 13: 9783642079689
Sprache: Englisch
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
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In den WarenkorbTaschenbuch. Zustand: 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.
Verlag: Springer Berlin Heidelberg, 2007
ISBN 10: 3540463143 ISBN 13: 9783540463146
Sprache: Englisch
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
EUR 213,99
Währung umrechnenAnzahl: 1 verfügbar
In den WarenkorbBuch. Zustand: 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.
Anbieter: Ria Christie Collections, Uxbridge, Vereinigtes Königreich
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In den WarenkorbZustand: New. In.
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In den WarenkorbPaperback. Zustand: Brand New. 539 pages. 9.70x7.50x1.20 inches. In Stock.