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.

Bestandsnummer des Verk�ufers 9783642079689

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Bibliografische Details

Titel: Handbook of the Solar-Terrestrial Environment
Verlag: Springer Berlin Heidelberg, Springer Berlin Heidelberg Nov 2010
Ver�ffentlichungsdatum: 2010
Sprache: Englisch
ISBN-10: 3642079687
ISBN-13: 9783642079689
Bindung: Taschenbuch
Zustand: Neu

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Inhaltsangabe

Part 1: 1. Solar-Terrestrial Environment (A. C.-L. Chian and Y. Kamide). 2. The Solar Interior - Radial Structure, Rotation, Solar Activity Cycle ( A. Brandenburg). 3. Solar Atmosphere (E. R. Priest). 4. How the Corona of the Sun Becomes the Solar Wind (E. N. Parker). 5. Magnetosphere (M. Schulz). 6. Ionosphere (P.-L. Blelly and D. Alcayd�). 7. Thermosphere (S. Kato). Part 2: 8. Space Plasmas (C. Uberoi). 9. Reconnection in the Earth's Magnetosphere (A. Nishida). 10. Nonlinear Processes in Space Plasmas (L. Stenflo and P. K. Shukla). Part 3: 11. Coronal Mass Ejections (P. J. Cargill and L. K. Harra). 12. Solar Radio Emissions(J. L. Bougeret and M. Pick). 13. The Aurora (B. Hultqvist). 14. Substorms (G. Rostoker). 15. Geomagnetic Storms (Y. Kamide and Y. P. Maltsev). 16. Ultra Low Frequency Waves in the Magnetosphere (U. Villante). 17. Space Weather (L. Lanzerotti). 18. Space Climatology (K. Labitzke). 19. Planetary Magnetospheres (M. G. Kivelson). 20. The Solar-Comet Interaction (D. A. Mendis)

Cr�ticas

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)

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