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100   $a19931115d1995      uy             0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aConvection and substorms$b[electronic resource] $eparadigms of magnetospheric phenomenology /$fCharles F. Kennel
210   $aNew York $cOxford University Press$d1995
215   $a1 online resource (429 p.)
225 1 $aInternational series on astronomy and astrophysics ;$v2
300   $aPreviously issued in print: 1995.
311   $a0-19-508529-9 
320   $aIncludes bibliographical references (p. [311]-401) and index.
327   $aContents; 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 Substorms
327   $a17. EpilogueReferences; Index
330 8 $aThe magnetosphere is the region where cosmic rays & the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights & other aurorae. The configuration & dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, & to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere & substorms have long been used as the principle paradigms for studying this vital region. The author here presents a synthesis of the convection & substorm literatures, & an analysis of convection & substorm interactions; he also suggests that the currently accepted steady reconnection model may be advantageously replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.
410  0$aInternational series on astronomy and astrophysics ;$v2.
606   $aMagnetosphere
606   $aMagnetospheric substorms
606   $aConvection (Meteorology)
615  0$aMagnetosphere.
615  0$aMagnetospheric substorms.
615  0$aConvection (Meteorology)
676   $a538.766
676   $a538/.766
700   $aKennel$b Charles F.$f1939-$01526738
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910777061203321
996   $aConvection and substorms$93769030
997   $aUNINA