The Magnetodiscs and Aurorae of Giant Planets

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...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Άλλοι συγγραφείς: Szego, Karoly (Επιμελητής έκδοσης), Achilleos, Nicholas (Επιμελητής έκδοσης), Arridge, Chris (Επιμελητής έκδοσης), Badman, Sarah (Επιμελητής έκδοσης), Delamere, Peter (Επιμελητής έκδοσης), Grodent, Denis (Επιμελητής έκδοσης), Galland Kivelson, Margaret (Επιμελητής έκδοσης), Louarn, Philippe (Επιμελητής έκδοσης)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: New York, NY : Springer New York : Imprint: Springer, 2016.
Σειρά:Space Sciences Series of ISSI, 50
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
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245 1 4 |a The Magnetodiscs and Aurorae of Giant Planets  |h [electronic resource] /  |c edited by Karoly Szego, Nicholas Achilleos, Chris Arridge, Sarah Badman, Peter Delamere, Denis Grodent, Margaret Galland Kivelson, Philippe Louarn. 
264 1 |a New York, NY :  |b Springer New York :  |b Imprint: Springer,  |c 2016. 
300 |a V, 333 p.  |b online resource. 
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490 1 |a Space Sciences Series of ISSI,  |x 1385-7525 ;  |v 50 
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. 
650 0 |a Physics. 
650 0 |a Planetology. 
650 1 4 |a Physics. 
650 2 4 |a Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 
650 2 4 |a Planetology. 
700 1 |a Szego, Karoly.  |e editor. 
700 1 |a Achilleos, Nicholas.  |e editor. 
700 1 |a Arridge, Chris.  |e editor. 
700 1 |a Badman, Sarah.  |e editor. 
700 1 |a Delamere, Peter.  |e editor. 
700 1 |a Grodent, Denis.  |e editor. 
700 1 |a Galland Kivelson, Margaret.  |e editor. 
700 1 |a Louarn, Philippe.  |e editor. 
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830 0 |a Space Sciences Series of ISSI,  |x 1385-7525 ;  |v 50 
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