[PDF] Top 20 The role of the bow shock in solar wind-magnetosphere coupling
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The role of the bow shock in solar wind-magnetosphere coupling
... the role of the bow shock in coupling solar wind energy to the magnetosphere using global magnetohydrodynamic simulations of the solar wind- ... See full document
7
Decoding solar wind–magnetosphere coupling
... Decoding Solar Wind–Magnetosphere Coupling ...the solar wind and ...preselected solar wind coupling ...ferent solar wind-magnetosphere ... See full document
14
Decoding solar wind–magnetosphere coupling
... Decoding solar wind-magnetosphere coupling ...the solar wind and ...preselected solar wind coupling ...different solar wind-magnetosphere ... See full document
18
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling
... the bow shock and in the ...upstream solar wind input conditions in relation to geomagnetic response is physically ...the solar wind, the gross features of solar ... See full document
7
Review of ionospheric effects of solar wind magnetosphere coupling in the context of the expanding contracting polar cap boundary model
... of solar wind magnetosphere coupling on the ionosphere during so called normal solar wind ...the magnetosphere, but perhaps more importantly it represents one of the main ... See full document
23
Review of ionospheric effects of solar wind magnetosphere coupling in the context of the expanding contracting polar cap boundary model
... of solar wind magnetosphere coupling on the ionosphere during so called normal solar wind ...the magnetosphere, but perhaps more importantly it represents one of the main ... See full document
23
Simulated solar wind plasma interaction with the Martian exosphere: influence of the solar EUV flux on the bow shock and the magnetic pile-up boundary
... the shock overshoot is about few ion inertial length (T´atrallyay et ...major role in the Martian aurorae recently observed with the Mars- Express spacecraft (Bertaux et ... See full document
8
First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground
... the bow shock, 13 R E downstream of the position of ...the bow shock and the propagation of the gener- ated waves through the bow shock, magnetosheath and mag- netosphere towards ... See full document
15
On the plasma sheet dependence on solar wind and substorms and its role in magnetosphere ionosphere coupling
... the magnetosphere, which control the efficiency of field-aligned acceleration (T e and eTN), vary in a wide range due to the combined action of two dif- ferent factors, solar wind state and ...the ... See full document
8
ANGEO - Observations of polar patches generated by solar wind Alfvén wave coupling to the dayside magnetosphere
... and solar wind speed of 770 km/s, negative propagation delays of about ...the bow shock subsolar point are ...decelerated solar wind from the bow shock to the ... See full document
27
Acceleration of solar wind ions to 1 MeV by electromagnetic structures upstream of the Earth's bow shock
... It results in rapid, stochastic acceleration of ions in the direction perpendicular to the ambient magnetic field. The electric potential of the structures can be compared to a field of moguls on a ski slope, capable of ... See full document
6
Acceleration of solar wind ions to 1 MeV by electromagnetic structures upstream of the Earth's bow shock
... to shock drift acceleration [6] of solar ions or to leakage from the magnetosphere ...the bow shock, incompatible with both the concepts of leakage and shock drift ... See full document
7
Access of solar wind electrons into the Martian magnetosphere
... the bow shock where solar wind electrons stream to mirror-like field with a positive potential and explains the appearance of top-flat electron ... See full document
14
On a magnetosphere disturbed by solar wind; observations of macroelectrons
... investigated magnetosphere is not ...the bow shock and the magnetopause, and entered the region where the x-component of magnetic induction dropped far below the dipole level, B x <−80 nT (see for ... See full document
9
The state of the solar wind and magnetosphere during the maunder minimum
... the bow-shock sits ahead of the magnetosphere by the same fraction as today’s ...r shock ∼ 14.5R E today, the MM shock stand-off distance would be ∼ 29R E ... See full document
6
Wind observations of the terrestrial bow shock: 3 D shape and motion
... the Wind orbiter, generally targeted to stay in the solar wind, passed through the Earth’s magnetosphere ∼ 50 ...distinct bow shock crossings were collected during the inbound ... See full document
9
Solar wind magnetosphere ionosphere interactions in the earth's plasma environment
... the solar wind plasma, which blows continuously outward from the Sun at speeds ~400 km s –1 ...the solar wind blows from left to ...the bow shock, formed because the solar ... See full document
21
Large-scale solar wind flow around Saturn's non-axisymmetric magnetosphere
... The solar wind is highly supersonic, thus forming a detached bow shock upstream of the magnetosphere that decelerates, heats, and de flects the ...and solar ... See full document
9
Coupling of the solar wind, magnetosphere and ionosphere by MHD waves
... Thus, the flow vortices are also magnetic vortices, giving rise to field-aligned currents (shown here by the black circles). Magnetospheric convection arises from the fact that magnetic field-lines over Earth’s magnetic ... See full document
188
Space and ground based investigations of solar wind magnetosphere ionosphere coupling
... The discussion so far has concentrated on sub-solar and magnetotail reconnection, which cause the overall quantity of open flux in the magnetosphere to change. When IMF B z > 0 nT, reconnection is expected ... See full document
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