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[PDF] Top 20 The magnetosphere under weak solar wind forcing

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The magnetosphere under weak solar wind forcing

The magnetosphere under weak solar wind forcing

... The steady nature of the polar cap showing no clear and systematic tendency to shrink or expand over such a long pe- riod also relates to a lack of solar wind driving. On the one hand, there is no ... See full document

15

Parametric study of the solar wind interaction with the Hermean magnetosphere for a weak interplanetary magnetic field

Parametric study of the solar wind interaction with the Hermean magnetosphere for a weak interplanetary magnetic field

... the solar wind with the Hermean magnetosphere when the interplanetary magnetic field is weak, performing a parametric study for all the range of hydrodynamic values of the solar ... See full document

29

Impact of solar wind depression on the dayside magnetosphere under northward interplanetary magnetic field

Impact of solar wind depression on the dayside magnetosphere under northward interplanetary magnetic field

... a magnetosphere with parallel ...the solar wind to simulate a decrease in the solar wind dynamic pressure followed by its ...the solar wind velocity, a gap (abrupt ... See full document

16

Weak and strong comets in the solar wind

Weak and strong comets in the solar wind

... To test these ideas experimentally, artificial comets were created in and near the E a rth ’s magnetosphere in 1984 and 1985 as part of the AM PTE (Ac­ tive Magnetospheric Paticles Tracer Explorers) mission. ... See full document

272

The role of the bow shock in solar wind-magnetosphere coupling

The role of the bow shock in solar wind-magnetosphere coupling

... unappreciated. Under nominal solar wind conditions there is little variation in the shock strength with solar wind variations, the dominant conversion of energy is from plasma flow to ... See full document

7

Coupling of the solar wind, magnetosphere and ionosphere by MHD waves

Coupling of the solar wind, magnetosphere and ionosphere by MHD waves

... Connecting Magnetosphere and Ionosphere A sizeable portion of ionospheric and magnetospheric research, both past and ongoing, treats one part of the system passively, ...the magnetosphere under the ... See full document

188

Nonlinear evolution of the modulational instability under weak forcing and damping

Nonlinear evolution of the modulational instability under weak forcing and damping

... The nonlinear interaction between the fundamental mode and the sidebands is not the dominant mechanism. The magenta curve exhibits oscillations around an averaged value growing exponentially, whereas the yellow curve ... See full document

9

Space  and ground based investigations of solar wind magnetosphere ionosphere coupling

Space and ground based investigations of solar wind magnetosphere ionosphere coupling

... consequence, 14 events are shown in panels a and c; only 13 events are seen in panels b, d, and e. In all cases the polar cap contained at least 0.5 GWb of open flux prior to onset, the average flux being nearly 0.8 GWb ... See full document

15

Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

Dawn-dusk asymmetry in particles of solar wind origin within the magnetosphere

... inner magnetosphere is a su- perposition of the electric field due to the co-rotation of the ionosphere with the Earth and the convection electric field associated with the earthward convection from the X-line in ... See full document

9

Solar wind forcing at Mercury: WSA-ENLIL model results

Solar wind forcing at Mercury: WSA-ENLIL model results

... as solar wind dynamic pressure are key for determining the Mercury magnetopause standoff distance, for ...the solar wind speed and southward IMF strength (B s ) at ...kinetic ... See full document

13

The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling

The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling

... – solar windmagnetosphere – iono- sphere coupled system is ...for solar wind magnetic turbu- lence events during duskward electric field and southward B z driven geomagnetic ...of ... See full document

7

Dawn–dusk asymmetries in the coupled solar wind–magnetosphere–ionosphere system: a review

Dawn–dusk asymmetries in the coupled solar wind–magnetosphere–ionosphere system: a review

... a weak partial ring current, they found a day–night asymmetry with negative H perturbation around noon and positive H perturbation around midnight, primar- ily caused by region 1 field-aligned ...asymmetry. ... See full document

33

Ensemble downscaling in coupled solar wind-magnetosphere modeling for space weather forecasting

Ensemble downscaling in coupled solar wind-magnetosphere modeling for space weather forecasting

... upstream solar wind conditions (though there remain many technical and scientific ...situ solar wind observations from spacecraft at the first Lagrange point ...the solar wind ... See full document

13

Ensemble downscaling in coupled solar wind-magnetosphere modeling for space weather forecasting

Ensemble downscaling in coupled solar wind-magnetosphere modeling for space weather forecasting

... upstream solar wind conditions (though there remain many technical and scientific ...situ solar wind observations from spacecraft at the first Lagrange point ...the solar wind ... See full document

11

Deep Solar Activity Minimum 2007-2009: Solar Wind Properties and Major Effects on the Terrestrial Magnetosphere

Deep Solar Activity Minimum 2007-2009: Solar Wind Properties and Major Effects on the Terrestrial Magnetosphere

... of solar wind and interplanetary magnetic field parameters during the solar minimum of 2007 – 2009 from measurements returned by the IMPACT and PLASTIC instruments on ...the solar ... See full document

29

Adjustment of a Coastal Buoyant Outflow Under Tidal and Wind Forcing

Adjustment of a Coastal Buoyant Outflow Under Tidal and Wind Forcing

... alongshore wind stress was ...a weak buoyant inflow or larger density difference yields the spreading of a surface- advected a minimum of more than four inflow Rossby radius ... See full document

63

First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground

First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground

... team; T. Nagai at the Tokyo Institute of Technology and the Geo- tail/MGF team, Geotail/MGF data was provided through DARTS at the Institute of Space and Astronautical Science (ISAS) in Japan; P. D´ecr´eau at CNRS/LPCE ... See full document

15

On the plasma sheet dependence on solar wind and substorms and its role in magnetosphere ionosphere coupling

On the plasma sheet dependence on solar wind and substorms and its role in magnetosphere ionosphere coupling

... the solar wind driver, we address the hierarchy of controlling SW parameters and their cross-correlation time delays with plasma sheet pa- rameters, emphasizing the difference in response be- tween plasma ... See full document

8

Solar wind interaction with the Earth’s magnetosphere: the role of reconnection in the presence of a large scale sheared flow

Solar wind interaction with the Earth’s magnetosphere: the role of reconnection in the presence of a large scale sheared flow

... must under- line that the role of the reconnection microphysics capable of changing, or not, the large scale evolution has been proved in our study in a limited, but significant range of parameters, namely 25 ≤ m ... See full document

10

Decoding solar wind–magnetosphere coupling

Decoding solar wind–magnetosphere coupling

... Decoding Solar WindMagnetosphere Coupling ...the solar wind and ...preselected solar wind coupling ...ferent solar wind-magnetosphere interaction ... See full document

14

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