03502nam 2200685Ia 450 991077706120332120230421044732.00-19-756048-21-280-54001-X97866105400130-19-535907-01-4294-1539-8(CKB)1000000000414136(EBL)271249(OCoLC)251536586(SSID)ssj0000130225(PQKBManifestationID)11148391(PQKBTitleCode)TC0000130225(PQKBWorkID)10082369(PQKB)10549229(MiAaPQ)EBC271249(StDuBDS)EDZ0002351196(Au-PeEL)EBL271249(CaPaEBR)ebr10142187(CaONFJC)MIL54001(OCoLC)466424529(EXLCZ)99100000000041413619931115d1995 uy 0engur|n|---|||||txtccrConvection and substorms[electronic resource] paradigms of magnetospheric phenomenology /Charles F. KennelNew York Oxford University Press19951 online resource (429 p.)International series on astronomy and astrophysics ;2Previously issued in print: 1995.0-19-508529-9 Includes bibliographical references (p. [311]-401) and index.Contents; 1. Introduction; 2. The Teardrop Magnetosphere; 3. The Bell-Like Magnetosphere; 4. The Viscous Magnetosphere; 5. The Reconnecting Magnetosphere; 6. Correlation of Geomagnetic Activity with the Solar Wind; 7. The Reconnection Substorm; 8. Bursty Magnetopause Reconnection; 9. Bimodal Plasma Sheet Flow; 10. Convection for Northward Interplanetary Field; 11. The Nightside Auroral Oval; 12. The Auroral Substorm; 13. The Geosynchronous Substorm; 14. Coordination of the Geosynchronous and Auroral Substorms; 15. Triggered Substorms; 16. On the Relation between Convection and Substorms17. EpilogueReferences; IndexThe magnetosphere is the region where cosmic rays & the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights & other aurorae. The configuration & dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, & to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere & substorms have long been used as the principle paradigms for studying this vital region. The author here presents a synthesis of the convection & substorm literatures, & an analysis of convection & substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.International series on astronomy and astrophysics ;2.MagnetosphereMagnetospheric substormsConvection (Meteorology)Magnetosphere.Magnetospheric substorms.Convection (Meteorology)538.766538/.766Kennel Charles F.1939-1526738MiAaPQMiAaPQMiAaPQBOOK9910777061203321Convection and substorms3769030UNINA