[PDF] Top 20 Coupling of the solar wind, magnetosphere and ionosphere by MHD waves
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Coupling of the solar wind, magnetosphere and ionosphere by MHD waves
... Alfv´en waves back towards the ...the waves originate from coupling between the ionosphere and magnetosphere, I have (for now) sim- ply dubbed them ... See full document
188
On the plasma sheet dependence on solar wind and substorms and its role in magnetosphere ionosphere coupling
... The problem of preferential electron acceleration in the flow bursts is a rather new puzzle. There are differ- ent reasons providing asymmetry between two species. One of them is, certainly, the difference in mass and ... See full document
8
Space and ground based investigations of solar wind magnetosphere ionosphere coupling
... the magnetosphere at any one ...the ionosphere suggest that dayside reconnection occurs in quasi-episodic bursts which may last for 2 min, with a canonical repetition rate of 8 min ...the ionosphere ... See full document
15
GUMICS 4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds
... fluctuating solar wind conditions during interplane- tary coronal mass ejections (ICMEs) using the Grand Unified Magnetosphere-Ionosphere Coupling Simulation (GUMICS- ...lar wind ... See full document
19
Temporal and spatial variability of auroral forms in the 10–14 MLT sector: Relationship to plasma convection and solar wind magnetosphere coupling
... events are observed to be associated with shortlived bursts of enhanced convection (e.g. Lockwood et al., 1990a, b). So far it has not been demonstrated that the ion drift crosses the magnetic separatrix in such cases. ... See full document
20
Review of ionospheric effects of solar wind magnetosphere coupling in the context of the expanding contracting polar cap boundary model
... both hemispheres simultaneously (e.g. Imber et al., 2006), and the consequences for the ionosphere. There also remain a number of questions about the flow generated during substorms. For example, what are the ... See full document
23
The importance of ground magnetic data in specifying the state of magnetosphere–ionosphere coupling: a personal view
... Using the KRM method, it has been demonstrated that the auroral electrojet consists of two major components, i.e., the electric field-dominant and the conductivity- dominant currents, and that their relative importance ... See full document
8
Transmission of the electric fields to the low latitude ionosphere in the magnetosphere-ionosphere current circuit
... The solar wind energy is transmitted to low latitude ionosphere in a current circuit from a dynamo in the magneto- sphere to the equatorial ionosphere via the polar ...inner ... See full document
11
ULF waves in the outer magnetosphere: Geotail observation 1 transverse waves
... with solar wind ...the solar wind provides broadband energy that couples to the eigen modes of the magnetospheric ...by MHD waveguide/cavity modes, have been observed to occur often at ... See full document
23
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling
... upstream solar wind input conditions in relation to geomagnetic response is physically ...the solar wind, the gross features of solar wind – magne- tosphere interactions and ... See full document
7
Multisatellite observations of the magnetosphere response to changes in the solar wind and interplanetary magnetic field
... the solar wind dynamic pressure ac- companying interplanetary (IP) shocks cause earthward mo- tion of the bow shock and the magnetopause and launch fast and intermediate mode waves into the ... See full document
15
Solar wind magnetosphere ionosphere interactions in the earth's plasma environment
... the magnetosphere via open field lines, producing boundary layers inside the magnetopause which extend down to the dayside ionosphere forming the cool (few hundred eV) ‘dayside cusp’ ...polar ... See full document
21
Five plus four equals nine: Combining the THEMIS and Cluster missions
... also presents a unique opportunity to investigate dayside coup- ling processes and the dynamics of the flank magnetopause (not shown). When combined with the multi-spacecraft Cluster mission and ground-based experiments ... See full document
6
The Generation and Damping of Propagating MHD Kink Waves in the Solar Atmosphere
... detect waves with certain periods and displacement amplitudes is also subject to observational constraints based on the resolution of the DST and analysis ... See full document
11
Extreme events and long-range correlations in space weather
... coupled solar wind – magnetosphere system, are far from equilibrium and the commonly used techniques of statistical analysis can not be applied readily, and the nonlinear dynamics and complex- ity ... See full document
7
Simulation of the ionospheric effect of intense geomagnetic storms of july and november 2004 using a low latitude 3d theoretical model
... Basu et al. (2001) analyzed the effects of the great magnetic storm of July 15, 2000 on the equatorial ionosphere by ground based and satellite in situ measurements. They observed a large westward plasma drift in ... See full document
7
Time scale of the largest imaginable magnetic storm
... the magnetosphere (plasma plus magnetic field perturbation) is limited, in or- der of magnitude, by the minimum pressure of Earth’s dipole field at the location of each flux ...the solar wind to ... See full document
5
Effects of Stratification and Flows on P-1/P-2 Ratios and Anti-node Shifts Within Closed Loop Structures
... Recent high-cadence, high-resolution observations have led to discussions re- lating to the idea of flows within coronal loops (see, Kopp et al., 1985; Ofman and Wang, 2008). Often, localised brightenings can be observed ... See full document
19
Type III solar radio bursts and Langmuir waves in the solar wind
... The growth rate formulae for Langmuir waves generated by non-relativistic, anisotropic electrons for the cases of a continuous and discontinuous electron pitch angle distribution are giv[r] ... See full document
94
PC index as a proxy of the solar wind energy that entered into the magnetosphere: 2 Relation to the interplanetary electric field E KL before substorm onset
... One can suggest that the shortest and longest values ΔT observed at the wings of the frequency curve with minimal incidence of events may be due to the random dispersion related, among other things, to the incorrect ... See full document
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