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.
"Sinopsis" puede pertenecer a otra edición de este libro.
From the reviews:
"The book is a solid, comprehensive ... text providing a full overview of solar-terrestrial science, pitched at the graduate student level. The book provides an excellent summary of the underlying physics controlling Sun-Earth connections, and it certainly merits a place on the bookshelf of an academic working in the field. ... is worthwhile for working solar-terrestrial physicists ... . If you are an ambitious graduate student and have decided you want to make a career in solar-terrestrial physics, then you might consider it ... ." (Andy Breen, EOS, Vol. 90 (11), March, 2009)
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.
"Sobre este título" puede pertenecer a otra edición de este libro.
Librería: Antiquariat Thomas Haker GmbH & Co. KG, Berlin, Alemania
Hardcover. Condición: 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. Nº de ref. del artículo: 813992
Cantidad disponible: 1 disponibles
Librería: moluna, Greven, Alemania
Gebunden. Condición: 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. Nº de ref. del artículo: 4891150
Cantidad disponible: Más de 20 disponibles
Librería: BuchWeltWeit Ludwig Meier e.K., Bergisch Gladbach, Alemania
Buch. Condición: 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. Nº de ref. del artículo: 9783540463146
Cantidad disponible: 2 disponibles
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
Buch. Condición: 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. Nº de ref. del artículo: 9783540463146
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Librería: AHA-BUCH GmbH, Einbeck, Alemania
Buch. Condición: 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. Nº de ref. del artículo: 9783540463146
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Librería: Books Puddle, Woodside, NY, Estados Unidos de America
Condición: New. pp. xiv + 539 1st Edition. Nº de ref. del artículo: 26302308
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Librería: Majestic Books, Hounslow, Reino Unido
Condición: New. Print on Demand pp. xiv + 539 255 Illus. (63 Col.). Nº de ref. del artículo: 7545659
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Librería: Biblios, Frankfurt am main, HESSE, Alemania
Condición: New. PRINT ON DEMAND pp. xiv + 539. Nº de ref. del artículo: 18302318
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