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Magnetospheric substorms: An inner-magnetospheric modeling perspective
2002Abstract Kilovolt electrons cause satellite anomalies through surface charging and frequently interfere with the operation of geosynchronous spacecraft. The Magnetospheric Specification Model was designed to specify kilovolt electron fluxes at and near synchronous orbit, and while it has seen limited operational use, its accuracy is not high.
R. W. Spiro +4 more
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The global current systems of the Martian induced magnetosphere
Nature Astronomy, 2019R. Ramstad +5 more
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2018
This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary Science. Please check back later for the full article. Saturn’s magnetosphere is the region of space surrounding Saturn that is controlled by the planetary magnetic field.
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This is an advance summary of a forthcoming article in the Oxford Research Encyclopedia of Planetary Science. Please check back later for the full article. Saturn’s magnetosphere is the region of space surrounding Saturn that is controlled by the planetary magnetic field.
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2011
Part I Solar Wind-Magnetosphere Interaction 1. The Magnetopause, its Boundary Layers and Pathways to the Magnetotail 2. Quantifying Energy Transfer at the Magnetopause 3. Long-period ULF Waves Driven by Periodic Solar Wind Disturbances Part II Magnetotail Dynamics 4. Magnetotail Dynamics: Survey of Recent Progress 5.
William Liu, Masaki Fujimoto
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Part I Solar Wind-Magnetosphere Interaction 1. The Magnetopause, its Boundary Layers and Pathways to the Magnetotail 2. Quantifying Energy Transfer at the Magnetopause 3. Long-period ULF Waves Driven by Periodic Solar Wind Disturbances Part II Magnetotail Dynamics 4. Magnetotail Dynamics: Survey of Recent Progress 5.
William Liu, Masaki Fujimoto
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Science, 1979 The interaction of ultra-low-frequency pc3-5 waves with charged particles in Earth’s magnetosphere
, 2017Q. Zong, R. Rankin, Xuzhi Zhou
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Antiprotons in the magnetosphere
10th International Congress of the Brazilian Geophysical Society & EXPOGEF 2007, Rio de Janeiro, Brazil, 19-23 November 2007, 2007U. B. Jayanthi +2 more
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Hydromagnetics of the magnetosphere
Space Science Reviews, 1963Different models of the magnetosphere are discussed critically. It is pointed out that there is a principal difference between the case when the impinging interplanetary plasma has no initial magnetization, B 0 = 0, (as in the Chapman-Ferraro theory), and the case when the plasma is initially magnetized, B 0 ≠ 0, even if B 0 is very small.
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