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Interplanetary Magnetic Field (IMF)

Effects of the interplanetary magnetic field y component on the dayside aurora

Effects of the interplanetary magnetic field y component on the dayside aurora

... associated field-aligned currents, as shown in ...the field-aligned currents can produce auro- ras, probably weak, at higher ...the field-aligned currents are ...when IMF B y > 0 and ...

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Can an interplanetary magnetic field reach the surface of Venus?

Can an interplanetary magnetic field reach the surface of Venus?

... The interplanetary magnetic field can theoret- ically reach (under the condition of stationary solar wind) Venus’ surface and justifies the nonzero field measurements by Venus ...perform ...

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Dependence of Geomagnetic Storms on Diverse Solar Wind Parameters, Interplanetary Magnetic Field, Interplanetary Conditions for Solar Cycle 23

Dependence of Geomagnetic Storms on Diverse Solar Wind Parameters, Interplanetary Magnetic Field, Interplanetary Conditions for Solar Cycle 23

... parameters, interplanetary conditions and interplanetary magnetic field, it is clear that solar wind parameter such as solar wind speed V and plasma proton temperature are effective in causing ...

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Modulation of dayside reconnection during northward interplanetary magnetic field

Modulation of dayside reconnection during northward interplanetary magnetic field

... southward IMF interval as the iono- spheric signatures of flux transfer events at the dayside ...the interplanetary magnetic field had a northward ...northward IMF, using the SuperDARN ...

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Radio Burst Related Geomagnetic Storms with CMEs, Interplanetary Magnetic Field and Solar Wind Disturbances

Radio Burst Related Geomagnetic Storms with CMEs, Interplanetary Magnetic Field and Solar Wind Disturbances

... The occurrence of a geomagnetic storm depends upon the solar conditions, particularly the southward interplanetary magnetic field (IMF) component. Some researchers have suggested a ...

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North South Asymmetry of the Interplanetary Magnetic Field Magnitude and the Geomagnetic Indices

North South Asymmetry of the Interplanetary Magnetic Field Magnitude and the Geomagnetic Indices

... daily interplanetary magnetic field (IMF), and the geomagnetic indices (aa, Ap, Kp, and DST) have been used to examine the asymmetry between the solar field north and south of the he- ...

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Hybrid Vlasov modelling of nightside auroral proton precipitation during southward interplanetary magnetic field conditions

Hybrid Vlasov modelling of nightside auroral proton precipitation during southward interplanetary magnetic field conditions

... In this paper, we present an overview of nightside proton precipitation in a global magnetospheric hybrid-Vlasov sim- ulation under southward interplanetary magnetic field (IMF) conditions, ...

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Interplanetary magnetic field control of fast azimuthal flows in the nightside high latitude ionosphere

Interplanetary magnetic field control of fast azimuthal flows in the nightside high latitude ionosphere

... upstream interplanetary magnetic field (IMF) from the MAG instrument [Smith et ...in magnetic local time (MLT) but are scaled in magnetic latitude according to the overall size ...

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Study of Response of Extreme Meso-Scale Field-Aligned Current to Interplanetary Magnetic Field Components BX, BY and BZ During Geomagnetic Storm

Study of Response of Extreme Meso-Scale Field-Aligned Current to Interplanetary Magnetic Field Components BX, BY and BZ During Geomagnetic Storm

... and interplanetary magnetic ...the field-aligned currents (FACs), commonly referred to as Birkeland currents after he first suggested their existence in the upper atmosphere in ...

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Cluster observations of the midaltitude cusp under strong northward interplanetary magnetic field

Cluster observations of the midaltitude cusp under strong northward interplanetary magnetic field

... region with reduced convection near the equatorward boundary of the cusp, which is characterized by low sunward/antisunward convection. However, duskward- dawnward convection persists as observed on SC1 and SC2. ...

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Influence of the interplanetary magnetic field on the ring current injection rate

Influence of the interplanetary magnetic field on the ring current injection rate

... 3) Concerning the combination (Bz , V, D), the expo- nents for Bz , V , and D show almost no variability for the change in the range of Bz; the exponents for Bz are about unity, those for V are about two, and those for D ...

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Ionospheric response to the interplanetary magnetic field southward turning: Fast onset and slow reconfiguration

Ionospheric response to the interplanetary magnetic field southward turning: Fast onset and slow reconfiguration

... the IMF near the magnetopause and the initial ionospheric response to be 7 ...the IMF southward ...of magnetic perturbations at different locations. The maximum magnetic perturbation tended to ...

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Kinematic models of the interplanetary magnetic field

Kinematic models of the interplanetary magnetic field

... and magnetic field in interplanetary space de- velop into ...the IMF is a power law over a wide range of frequencies (typically in the MHz regime) (Coleman ...the IMF structure is an ...

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Finite size scaling in the solar wind magnetic field energy
density as seen by WIND

Finite size scaling in the solar wind magnetic field energy density as seen by WIND

... the interplanetary magnetic field (IMF) fluctuations are a topic of considerable interest in space ...the IMF fluctuations such as intermittency [Tu and Marsch, 1995; Burlaga, ...

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Multisatellite observations of the magnetosphere response to changes in the solar wind and interplanetary magnetic field

Multisatellite observations of the magnetosphere response to changes in the solar wind and interplanetary magnetic field

... electric field perturbations are still not fully ...electric field observed by the GEOS-2 satellite showed a transient signature of about 7 mV m −1 in the dayside mag- netosphere associated with the onset ...

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Non Gaussianity and cross scale coupling in interplanetary magnetic field turbulence during a rope–rope magnetic  reconnection event

Non Gaussianity and cross scale coupling in interplanetary magnetic field turbulence during a rope–rope magnetic reconnection event

... der in each sliding window of size 5000 data points across the time series of Fig. 2, and a window shift of 400 data points. Then, we increased the size of the window by 1000 data points (keeping the same window shift), ...

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Transmission of the electric fields to the low latitude ionosphere in the magnetosphere-ionosphere current circuit

Transmission of the electric fields to the low latitude ionosphere in the magnetosphere-ionosphere current circuit

... electric field is intensified by the southward interplanetary magnetic field (IMF), driving the ionospheric DP2 currents composed of two-cell Hall current vortices in high latitudes and ...

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Advanced Panspermia of Origin of Life and Evolution

Advanced Panspermia of Origin of Life and Evolution

... across interplanetary space to strike Earth's magnetosphere ...called Interplanetary Magnetic Field (IMF), in turn affects the earth’s magnetic ...planetary magnetic ...

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Geomagnetic Parameters Influencing Geomagnetic Storms in Relation to Solar Terrestrial Relationship

Geomagnetic Parameters Influencing Geomagnetic Storms in Relation to Solar Terrestrial Relationship

... the interplanetary magnetic field turns southward, permitting interplanetary and terrestrial magnetic field lines to merge at the dayside magnetopause and energy to be ...

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April 2000 magnetic storm: Solar wind driver and magnetospheric response

April 2000 magnetic storm: Solar wind driver and magnetospheric response

... interplanetary magnetic field had an intense and long-sustained southward magnetic field orientation, and the solar wind magnetic pressure was very large, which compressed the ...

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