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000753532 020__ $$a9781493935444$$q(electronic book)
000753532 020__ $$a1493935445$$q(electronic book)
000753532 020__ $$z9781493935437
000753532 0247_ $$a10.1007/978-1-4939-3544-4$$2doi
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000753532 24500 $$aPlasma sources of solar system magnetospheres$$h[electronic resource] /$$cAndrew F. Nagy, Michael Blanc, Charles R. Chappell, Norbert Krupp, editors.
000753532 264_1 $$aNew York :$$bSpringer,$$c2016.
000753532 300__ $$a1 online resource.
000753532 336__ $$atext$$btxt$$2rdacontent
000753532 337__ $$acomputer$$bc$$2rdamedia
000753532 338__ $$aonline resource$$bcr$$2rdacarrier
000753532 4901_ $$aSpace sciences series of ISSI ;$$vvolume 52
000753532 500__ $$a"Previously published in Space Science Reviews Volume 192, Issues 1-4, 2015."
000753532 504__ $$aIncludes bibliographical references.
000753532 5050_ $$aForeword -- The role of the ionosphere in providing plasma to the terrestrial magnetosphere: a historical perspective -- A review of general processes related to plasma sources and losses for solar system magnetospheres -- Plasma sources in planetary magnetospheres -- The Earth: plasma sources, losses and transport processes -- Jupiter's magnetosphere: plasma sources and transport -- Saturn plasma sources and associated transport processes -- Comparison of plasma sources in solar system magnetospheres.
000753532 506__ $$aAccess limited to authorized users.
000753532 520__ $$aThis volume reviews what we know of the corresponding plasma source for each intrinsically magnetized planet. Plasma sources fall essentially in three categories: the solar wind, the ionosphere (both prevalent on Earth), and the satellite-related sources. Throughout the text, the case of each planet is described, including the characteristics, chemical composition and intensity of each source. The authors also describe how the plasma generated at the source regions is transported to populate the magnetosphere, and how it is later lost. To summarize, the dominant sources are found to be the solar wind and sputtered surface ions at Mercury, the solar wind and ionosphere at Earth (the relative importance of the two being discussed in a specific introductory chapter), Io at Jupiter and - a big surprise of the Cassini findings - Enceladus at Saturn. The situation for Uranus and Neptune, which were investigated by only one fly-by each, is still open and requires further studies and exploration. In the final chapter, the book offers a summary of the little we know of Uranus and Neptune, then summarizes in a comparative way what we know of plasma sources throughout the solar system, and proposes directions for future research. Originally published in Space Science Reviews, Vol. 192, Issues 1-4, 2015.
000753532 588__ $$aOnline resource; title from PDF title page (viewed February 1, 2016).
000753532 650_0 $$aMagnetosphere.
000753532 650_0 $$aSolar atmosphere$$xMagnetic properties.
000753532 650_0 $$aSpace plasmas.
000753532 7001_ $$aNagy, Andrew$$q(Andrew F.),$$eeditor.
000753532 7001_ $$aBlanc, Michel,$$d1949-$$eeditor.
000753532 7001_ $$aChappell, Rick,$$d1943-$$eeditor.
000753532 7001_ $$aKrupp, Norbert,$$eeditor.
000753532 77608 $$iPrint version:$$z9781493935437
000753532 830_0 $$aSpace sciences series of ISSI ;$$vvolume 52.
000753532 852__ $$bebk
000753532 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-1-4939-3544-4$$zOnline Access$$91397441.1
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000753532 980__ $$aBIB
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