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|a 9783540463153
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|a 10.1007/978-3-540-46315-3
|2 doi
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|a (DE-He213)978-3-540-46315-3
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|a E-Book
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|a TTDS
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| 245 |
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|a Handbook of the Solar-Terrestrial Environment
|h [electronic resource] /
|c edited by Yohsuke Kamide, Abraham C.-L. Chian.
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| 250 |
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|a 1st ed. 2007.
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| 264 |
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|a Berlin, Heidelberg :
|b Springer Berlin Heidelberg :
|b Imprint: Springer,
|c 2007.
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| 300 |
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|a XIV, 539 p.
|b online resource.
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| 336 |
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|a text
|b txt
|2 rdacontent
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|a Springer eBook Collection
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|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.
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| 520 |
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|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.
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| 590 |
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|a Loaded electronically.
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|a Electronic access restricted to members of the Holy Cross Community.
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|a Space sciences.
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| 650 |
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|a Atmospheric sciences.
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| 650 |
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|a Geophysics.
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| 650 |
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|a Observations, Astronomical.
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| 650 |
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|a Astronomy—Observations.
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| 650 |
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|a Planetology.
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| 690 |
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|a Electronic resources (E-books)
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| 700 |
1 |
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|a Kamide, Yohsuke.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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| 700 |
1 |
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|a Chian, Abraham C.-L.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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| 710 |
2 |
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|a SpringerLink (Online service)
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| 773 |
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|t Springer eBooks
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| 830 |
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|a Springer eBook Collection.
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| 856 |
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|u https://holycross.idm.oclc.org/login?auth=cas&url=https://doi.org/10.1007/978-3-540-46315-3
|3 Click to view e-book
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