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[null,"1.","Record Nr.",null,"UNINA9910450955803321"]
[null,null,"Autore",null,"Kennel Charles F. <1939->"]
[null,null,"Titolo",null,"Convection and substorms [[electronic resource] ] : paradigms of magnetospheric phenomenology / / Charles F. Kennel"]
[null,null,"Pubbl/distr/stampa",null,"New York, : Oxford University Press, 1995"]
[null,null,"ISBN",null,"0-19-756048-2"]
[{"$nulls":4},"1-280-54001-X"]
[{"$nulls":4},"9786610540013"]
[{"$nulls":4},"0-19-535907-0"]
[{"$nulls":4},"1-4294-1539-8"]
[null,null,"Descrizione fisica",null,"1 online resource (429 p.)"]
[null,null,"Collana",null,"International series on astronomy and astrophysics ; ; 2"]
[null,null,"Disciplina",null,"538.766"]
[{"$nulls":4},"538/.766"]
[null,null,"Soggetti",null,"Magnetosphere"]
[{"$nulls":4},"Magnetospheric substorms"]
[{"$nulls":4},"Convection (Meteorology)"]
[{"$nulls":4},"Electronic books."]
[null,null,"Lingua di pubblicazione",null,"Inglese"]
[null,null,"Formato",null,"Materiale a stampa"]
[null,null,null,"Livello bibliografico","Monografia"]
[null,null,null,"Note generali","Previously issued in print: 1995."]
[null,null,null,"Nota di bibliografia","Includes bibliographical references (p. [311]-401) and index."]
[null,null,"Nota di contenuto",null,"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 Substorms"]
[{"$nulls":4},"17. EpilogueReferences; Index"]
[null,null,null,"Sommario/riassunto","The magnetosphere is the region where cosmic rays & the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights & other aurorae. The configuration & dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, & to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere & "]
[{"$nulls":4},"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."]