Handbook of the solar-terrestrial environment
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 understan...
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| Autres auteurs: | , |
|---|---|
| Format: | Livre numérique |
| Langue: | Anglais |
| Publié: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Springer e-books
[20..].
Cham : Springer Nature |
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Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Handbook of the solar-terrestrial environment, Yohsuke Kamide, Abrahm C.-L. Chian (Eds.), Berlin, Springer, 2007, 1 vol. (XIV-539 p.), 978-3-540-46314-6 |
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| 245 | 0 | 0 | |a Handbook of the solar-terrestrial environment |c edited by Y. Kamide, A. Chian. |
| 260 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg : |b Springer e-books. | ||
| 260 | |a Cham : |b Springer Nature, |c [20..]. | ||
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 505 | 1 | |a An Overview of the Solar Terrestrial Environment An Overview of the Solar Terrestrial Environment The Sun The Solar Interior Radial Structure, Rotation, Solar Activity Cycle Solar Atmosphere Solar Wind Coronal Mass Ejection Solar Radio Emissions The Earth Magnetosphere Ionosphere Thermosphere Space Plasmas Space Plasmas Magnetic Reconnection Nonlinear Processes in Space Plasmas Processes in the Solar-Terrestrial Environment The Aurora Geomagnetic Storms Substorms Ultra Low Frequency Waves in the Magnetosphere Space Weather Effects of the Solar Cycle on the Earth s Atmosphere Planets and Comets in the Solar System Planetary Magnetospheres The Solar-Comet Interactions | |
| 506 | |a Accès en ligne pour les établissements français bénéficiaires des licences nationales | ||
| 506 | |a Accès soumis à abonnement pour tout autre établissement | ||
| 506 | |a Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 | ||
| 520 | |a 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 | ||
| 700 | 1 | |a Kamide, Yohsuke. |4 pbd | |
| 700 | 1 | |a Chian, Abraham C.-L. |4 pbd | |
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