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The magnetodiscs and aurorae of gian...

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The magnetodiscs and aurorae of giant planets[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	538.7660992
書名/作者:	The magnetodiscs and aurorae of giant planets/ edited by Karoly Szego ... [et al.].
其他作者:	Szego, Karoly.
出版者:	New York, NY : : Springer New York :, 2016.
面頁冊數:	v, 333 p. : : ill. (some col.), digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Planets - Magnetospheres.
標題:	Auroras.
標題:	Physics.
標題:	Extraterrestrial Physics, Space Sciences.
標題:	Planetology.
ISBN:	9781493933952
ISBN:	9781493933945
摘要、提要註:	Readers will find grouped together here the most recent observations, current theoretical models and present understanding of the coupled atmosphere, magnetosphere and solar wind system. The book begins with a general discussion of mass, energy and momentum transport in magnetodiscs. The physics of partially ionized plasmas of the giant planet magnetodiscs is of general interest throughout the field of space physics, heliophysics and astrophysical plasmas; therefore, understanding the basic physical processes associated with magnetodiscs has universal applications. The second chapter characterizes the solar wind interaction and auroral responses to solar wind driven dynamics. The third chapter describes the role of magnetic reconnection and the effects on plasma transport. Finally, the last chapter characterizes the spectral and spatial properties of auroral emissions, distinguishing between solar wind drivers and internal driving mechanisms. The in-depth reviews provide an excellent reference for future research in this discipline.
電子資源:	http://dx.doi.org/10.1007/978-1-4939-3395-2

The magnetodiscs and aurorae of giant planets[electronic resource] /
The magnetodiscs and aurorae of giant planets[electronic resource] /edited by Karoly Szego ... [et al.]. - New York, NY :Springer New York :2016. - v, 333 p. :ill. (some col.), digital ;24 cm. - Space sciences series of ISSI,v.501385-7525 ;. - Space sciences series of ISSI ;v.37..

Readers will find grouped together here the most recent observations, current theoretical models and present understanding of the coupled atmosphere, magnetosphere and solar wind system. The book begins with a general discussion of mass, energy and momentum transport in magnetodiscs. The physics of partially ionized plasmas of the giant planet magnetodiscs is of general interest throughout the field of space physics, heliophysics and astrophysical plasmas; therefore, understanding the basic physical processes associated with magnetodiscs has universal applications. The second chapter characterizes the solar wind interaction and auroral responses to solar wind driven dynamics. The third chapter describes the role of magnetic reconnection and the effects on plasma transport. Finally, the last chapter characterizes the spectral and spatial properties of auroral emissions, distinguishing between solar wind drivers and internal driving mechanisms. The in-depth reviews provide an excellent reference for future research in this discipline.

ISBN: 9781493933952

Standard No.: 10.1007/978-1-4939-3395-2doiSubjects--Topical Terms:

653482
Planets
--Magnetospheres.

LC Class. No.: QB603.M26

Dewey Class. No.: 538.7660992

The magnetodiscs and aurorae of giant planets[electronic resource] /
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520 $a Readers will find grouped together here the most recent observations, current theoretical models and present understanding of the coupled atmosphere, magnetosphere and solar wind system. The book begins with a general discussion of mass, energy and momentum transport in magnetodiscs. The physics of partially ionized plasmas of the giant planet magnetodiscs is of general interest throughout the field of space physics, heliophysics and astrophysical plasmas; therefore, understanding the basic physical processes associated with magnetodiscs has universal applications. The second chapter characterizes the solar wind interaction and auroral responses to solar wind driven dynamics. The third chapter describes the role of magnetic reconnection and the effects on plasma transport. Finally, the last chapter characterizes the spectral and spatial properties of auroral emissions, distinguishing between solar wind drivers and internal driving mechanisms. The in-depth reviews provide an excellent reference for future research in this discipline.
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