[PDF] Top 20 Decoding solar wind–magnetosphere coupling
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Decoding solar wind–magnetosphere coupling
... enhanced solar wind dynamic ...the solar wind parameters, some of these are listed in section ...the coupling functions, which describe the enhancement of -Dst over the course of a ... See full document
14
Decoding solar wind–magnetosphere coupling
... using solar wind parameters alone, and it is not clear how much the model repre- sents a smoothed time average over the bursty events or how much it represents steady tail reconnection occurring between the ... See full document
18
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
On the plasma sheet dependence on solar wind and substorms and its role in magnetosphere ionosphere coupling
... the solar wind ...of solar wind state and substorms, which have different dynamics and provide comparable partial contributions to these ... See full document
8
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
Correlation of solar wind velocity with different parameters during geomagnetic disturbances
... the solar wind energy during HILDCAA in his PhD thesis to described the electrodynamical process caused by the solar wind magnetosphere coupling for HILDCAA events (high ... See full document
12
Statistical study of chorus wave distributions in the inner magnetosphere using Ae and solar wind parameters
... the solar wind velocity and density but also on the ver- tical interplanetary magnetic field component ...strong coupling with the Earth’s geomagnetic ...to solar wind velocity (Figure ... See full document
14
Jovian electron modulations by the solar wind interaction with the magnetosphere
... Jovian magnetosphere are investigated in detail by using data from three spacecraft, Pioneer 10, 11, and ...the solar wind at the position of ...the coupling of both the source modulation at ... See full document
10
The coupling between the solar wind and proton fluxes at GEO
... a solar wind magnetosphere coupling function for the Dst ...this coupling function analytically, using the geom- etry of dayside reconnection between the solar wind and ... See full document
7
On the validity of Akasofu’s ε parameter and of the Vasyliunas et al general formula for the rate of solar wind magnetosphere energy input
... the solar wind and the Earth’s magne- ...the solar wind energy input into the magnetosphere is called the en- ergy coupling function between the solar wind and the ... See full document
7
Temporal and spatial variability of auroral forms in the 10–14 MLT sector: Relationship to plasma convection and solar wind magnetosphere coupling
... The present study adds new information on the temporal/ spatial evolution of the auroral precipitation and its detailed relationships with ionospheric convection in the dayside polar ionosphere (cf. Figs. 6, 8 and 10), ... See full document
20
The influence of solar wind and geomagnetic indices on lower band chorus emissions in the inner magnetosphere
... which solar wind-magnetosphere coupling function controls the Dst index, Boynton, Balikhin, Billings, Wei, et ...a solar wind-magnetosphere coupling ...cross ... See full document
14
Space and ground based investigations of solar wind magnetosphere ionosphere coupling
... The deduced dayside reconnection rates imply that reconnection is occurring across 20% of the width of the magnetosphere at any one time. On the other hand, observations of flux transfer events at the dayside ... See full document
15
Coupling of the solar wind, magnetosphere and ionosphere by MHD waves
... This chapter sets out the methods – the model, governing equations and computer codes – used to investigate self-consistent magnetosphere-ionosphere (MI) coupling in later chapters. We have in fact ... See full document
188
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind – magnetosphere coupling
... The solar wind is a supersonic plasma flow, originating from the Sun, in which coherent structures, waves and turbu- lence coexist and interact over various spatial and temporal ... See full document
7
Dependence of Geomagnetic Storms on Diverse Solar Wind Parameters, Interplanetary Magnetic Field, Interplanetary Conditions for Solar Cycle 23
... diverse solar wind parameters, interplanetary conditions and interplanetary magnetic field, it is clear that solar wind parameter such as solar wind speed V and plasma proton ... See full document
8
Effect of Solar Influences on Earths Magnetosphere and Upper Atmosphere
... how solar plasma does inters in geomagnetosphere and affect the upper ...cover solar cycles 23 and maxima of solar cycle 24. The study of solar cycle 23 has unique important because occurrence ... See full document
9
Alfvén wave boundary condition for responsive magnetosphere ionosphere coupling
... indicating that the ionosphere can act as a highly conducting reflecting boundary on the dayside, but more like an insulating boundary on the nightside. Of course, there are more sophisticated routes to estimating the ... See full document
14
A global view of storms and substorms
... the magnetosphere is effectively coupled with the IMF, substorms are highly variable and unpredictable in ...inner magnetosphere, it has been proposed that substorms are important in generating geomagnetic ... See full document
17
Cassini observations of ionospheric plasma in Saturn's magnetotail lobes
... Figure 1. Cassini’s trajectory in Kronocentric Solar Magnetospheric Coordinates (KSM) for Cassini’s rev. 27 of Saturn from 04 August to 28 August 2006 projected in the X-Y plane (top) and noon-midnight meridional ... See full document
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