Convection and Substorms
Paradigms of Magnetospheric Phenomenology
Format:Hardback
Publisher:Oxford University Press Inc
Published:25th Apr '96
Currently unavailable, and unfortunately no date known when it will be back
The magnetosphere is the region in which the solar wind interacts with the Earth's magnetic field, the zone which screens the Earth from most of the harmful cosmic rays which daily bombard it. The Aurora Borealis, or Norhun lights, other such phenourena result from the interaction of particles in the solar wind and the magnetosphere. Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the Planetary physicists, geophysicists, plasma astrophysicists, and scientists involved with astronautics all have a primary interest in the configuration and dynamics of the magnetosphere, and much research is devoted to convection (the circulation of solarwind plastma in the magnetiosphere) and substorms, which are linked to the aurorae and thought to stimulate convection. In this book, one of the leading scientists in the field presents a synthesis of current knowledge on convection and substorms and proposes that the steady reconnection model be replaced by a model of multiple tail reconnection events, in which many mutually interdependent reconnections occur.
"... a well-supported claim of a shift in paradigm from the old quasi-steady picture of convection to a new, much more dynamic one .... Primarily, however, it provides enjoyment and stimulation for the educated reader, and I highly recommend it to all colleagues interested in the topic." --Eos "... a well-supported claim of a shift in paradigm from the old quasi-steady picture of convection to a new, much more dynamic one .... Primarily, however, it provides enjoyment and stimulation for the educated reader, and I highly recommend it to all colleagues interested in the topic." --Eos
ISBN: 9780195085297
Dimensions: 241mm x 163mm x 34mm
Weight: 759g
432 pages