Convection and Substorms: Paradigms of Magnetospheric Phenomenology
Convection and Substorms: Paradigms of Magnetospheric Phenomenology
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Abstract
The magnetosphere is the region where cosmic rays and the solar wind interact with the Earth's magnetic field, creating such phenomena as the northern lights and other aurorae. The configuration and dynamics of the magnetosphere are of interest to planetary physicists, geophysicists, plasma astrophysicists, and to scientists planning space missions. The circulation of solar wind plasma in the magnetosphere and substorms have long been used as the principle paradigms for studying this vital region. Charles F. Kennel, a leading scientist in the field, here presents a synthesis of the convection and substorm literatures, and an analysis of convection and 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. Written in an accessible, non-mathematical style, this book introduces the reader to the exciting discoveries in this fast-growing field.
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Front Matter
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11
Introduction
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282
The Teardrop Magnetosphere
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403
The Bell-Like Magnetosphere
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574
The Viscous Magnetosphere
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735
The Reconnecting Magnetosphere
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966
Correlation of Geomagnetic Activity With the Solar Wind
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1077
The Reconnection Substorm
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1278
Bursty Magnetopause Reconnection and its Consequences
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1509
Bimodal Plasma Sheet Flow
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17710
Convection for Northward Interplanetary Field
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19611
The Nightside Auroral Oval
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22112
The Auroral Substorm
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24813
The Geosynchronous Substorm
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27214
Coordination of the Geosynchronous and Auroral Substorms
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28415
Triggered Substorms
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29416
On the Relation Between Convection and Substorms
- 30917 Epilogue
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End Matter
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