Results 31 to 40 of about 103,965 (278)
External solar wind variability causes motion of the magnetopause and changes of this boundary's current structure, and the resulting inductive processes, may be exploited to determine the interior structure of magnetized planets.
S. Zomerdijk‐Russell +3 more
doaj +1 more source
The Triple Dusk-Dawn Aberration of the Solar Wind at Earth
In this Brief Report it is pointed out that there are three dusk-dawn aberrations of the solar-wind plasma and magnetic structure approaching Earth and the magnitudes of these aberrations are estimated for various solar-wind types monitored from L1 ...
Joseph E. Borovsky
doaj +1 more source
MESSENGER Observations and Global Simulations of Highly Compressed Magnetosphere Events at Mercury
We identify and examine all MErcury Surface Space ENvironment, GEochemistry, and Ranging (MESSENGER) crossings of Mercury's dayside magnetopause with magnetospheric field intensities ≥300 nT.
X. Jia +7 more
semanticscholar +1 more source
Juno's highly inclined orbits provide opportunities to sample high‐latitude magnetic field lines connected to the orbit of Io, among the other Galilean satellites.
A. H. Sulaiman +12 more
doaj +1 more source
Stormtime Energetics: Energy Transport Across the Magnetopause in a Global MHD Simulation
Coupling between the solar wind and magnetosphere can be expressed in terms of energy transfer through the separating boundary known as the magnetopause.
Austin Brenner +5 more
doaj +1 more source
Magnetosphere-Ionosphere Coupling: Implications of Non-Equilibrium Conditions
The response times of the coupled magnetosphere-ionosphere-thermosphere system are, on average, greater than the autocorrelation timescales of solar wind forcing. This means that the system is rarely, if ever, in equilibrium.
Mike Lockwood, Stan W. H. Cowley
doaj +1 more source
Response of convection electric fields in the magnetosphere to IMF orientation change [PDF]
[1] The transient response of convection electric fields in the inner magnetosphere to southward turning of the interplanetary magnetic field (IMF) is investigated using in‐situ electric field observations by the CRRES and Akebono spacecraft.
Brautigam, D. +7 more
core +1 more source
The plasmas (electrons and ions) in the inner magnetosphere have wide energy ranges from electron volts to mega-electron volts (MeV). These plasmas rotate around the Earth longitudinally due to the gradient and curvature of the geomagnetic field and by ...
K. Shiokawa +47 more
semanticscholar +1 more source
In the frame of complex systems research, methods used to quantitatively analyze specific dynamic phenomena are often used to analyze phenomena from other disciplines on the grounds that are governed by similar dynamics.
Pavlos I. Zitis +3 more
doaj +1 more source
How the IMF By induces a By component in the closed magnetosphere and how it leads to asymmetric currents and convection patterns in the two hemispheres [PDF]
We used the Lyon‐Fedder‐Mobarry global magnetohydrodynamics model to study the effects of the interplanetary magnetic field (IMF) By component on the coupling between the solar wind and magnetosphere‐ionosphere system.
P. Tenfjord +7 more
semanticscholar +1 more source

