LEADER 04527nam 22006975 450 001 9910254638403321 005 20210525081219.0 010 $a1-4939-3544-5 024 7 $a10.1007/978-1-4939-3544-4 035 $a(CKB)3710000000579430 035 $a(EBL)4384563 035 $a(SSID)ssj0001607056 035 $a(PQKBManifestationID)16317201 035 $a(PQKBTitleCode)TC0001607056 035 $a(PQKBWorkID)14895933 035 $a(PQKB)10901998 035 $a(DE-He213)978-1-4939-3544-4 035 $a(MiAaPQ)EBC4384563 035 $a(PPN)191705993 035 $a(EXLCZ)993710000000579430 100 $a20160127d2016 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aPlasma Sources of Solar System Magnetospheres /$fedited by Andrew F. Nagy, Michel Blanc, Charles Chappell, Norbert Krupp 205 $a1st ed. 2016. 210 1$aNew York, NY :$cSpringer New York :$cImprint: Springer,$d2016. 215 $a1 online resource (296 p.) 225 1 $aSpace Sciences Series of ISSI,$x1385-7525 ;$v52 300 $a"Previously published in Space Science Reviews Volume 192, Issues 1- 4, 2015." 311 $a1-4939-3543-7 320 $aIncludes bibliographical references at the end of each chapters. 327 $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. 330 $aThis volume reviews what we know of the corresponding plasma source for each intrinsically magnetized planet. Plasma sources fall essentially in three categories: the solar wind, the ionosphere (both prevalent on Earth), and the satellite-related sources. Throughout the text, the case of each planet is described, including the characteristics, chemical composition and intensity of each source. The authors also describe how the plasma generated at the source regions is transported to populate the magnetosphere, and how it is later lost. To summarize, the dominant sources are found to be the solar wind and sputtered surface ions at Mercury, the solar wind and ionosphere at Earth (the relative importance of the two being discussed in a specific introductory chapter), Io at Jupiter and ? a big surprise of the Cassini findings ? Enceladus at Saturn. The situation for Uranus and Neptune, which were investigated by only one fly-by each, is still open and requires further studies and exploration. In the final chapter, the book offers a summary of the little we know of Uranus and Neptune, then summarizes in a comparative way what we know of plasma sources throughout the solar system, and proposes directions for future research. Originally published in Space Science Reviews, Vol. 192, Issues 1-4, 2015. 410 0$aSpace Sciences Series of ISSI,$x1385-7525 ;$v52 606 $aSpace sciences 606 $aPlanetology 606 $aPlasma (Ionized gases) 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 606 $aPlanetology$3https://scigraph.springernature.com/ontologies/product-market-codes/G18010 606 $aPlasma Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P24040 615 0$aSpace sciences. 615 0$aPlanetology. 615 0$aPlasma (Ionized gases). 615 14$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 615 24$aPlanetology. 615 24$aPlasma Physics. 676 $a538.766 702 $aNagy$b Andrew F$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aBlanc$b Michel$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aChappell$b Rick,1943-$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aKrupp$b Norbert$4edt$4http://id.loc.gov/vocabulary/relators/edt 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254638403321 996 $aPlasma Sources of Solar System Magnetospheres$91820634 997 $aUNINA