[PDF] Top 20 Geotail observations of two-component protons in the midnight plasma sheet
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Geotail observations of two-component protons in the midnight plasma sheet
... cold plasma in the near- Earth magnetotail under northward IMF, we find that two- component protons are observed in the midnight plasma sheet (−10>X GSM >−30 R E , |Y GSM ... See full document
17
Temperature anisotropies of electrons and two-component protons in the dusk plasma sheet
... and protons have temper- ature anisotropy in the cold plasma ...the plasma sheet, some other mechanism that selectively heats electrons in the parallel direction may ...for plasma ... See full document
16
Origin of temperature anisotropies in the cold plasma sheet: Geotail observations around the Kelvin-Helmholtz vortices
... of two separate (cold and hot) components in the magnetosphere-like region inside the KH vortical struc- ...proton component occasionally consisted of counter-streaming beams near the current layer in the ... See full document
18
Cluster observations of a magnetic field cavity in the plasma sheet
... (top two panels of Figure 2) indicate that at ~1900 UT the magnetosphere was in the recovery phase following a substorm that occurred at 1823 UT, detected as a decrease in the X component and evidence for ... See full document
7
Characteristics of storm time ion composition in the near Earth plasma sheet using Geotail and RBSP measurements
... near-Earth plasma sheet and inner magnetosphere during the main phase of the geomagnetic storms is investigated in this work by using two satellite-based ...(1) Geotail and RBSP ... See full document
16
Substorm observations in the early morning sector with Equator-S and Geotail
... side plasma sheet as well as near the boundary of the plasma sheet in association with a local dipolarization following an onset of the global poleward expansion of the ...the plasma ... See full document
10
ANGEO - Substorm observations in the early morning sector with Equator-S and Geotail
... side plasma sheet as well as near the boundary of the plasma sheet in association with a local dipolarization following an onset of the global poleward expansion of the ...the plasma ... See full document
9
ANGEO - Observations of flux rope − associated particle bursts with GEOTAIL in the distant tail
... In a more careful examination of the angular distributions of energetic electron with E > 38 keV, presented in Figs. 4a and 11a, observed for some minutes after the onset of the burst, we can note that although the ... See full document
17
Statistical study of transient plasma structures in magnetotail lobes and plasma sheet boundary layer: Interball-1 observations
... beamlet observations In this section we perform the statistical analysis of beamlet observations for different magnetospheric and interplanetary ...the two horizontal field components at a given ... See full document
12
ANGEO - Spatial structure of the plasma sheet boundary layer at distances greater than 180 RE as derived from energetic particle measurements on GEOTAIL
... the two results then the assumption of constant speed of plasmoid propagation may be incor- ...z component of the magnetic ®eld because the spacecraft crosses the neutral ... See full document
11
Multi-instrument observations of the ionospheric counterpart of a bursty bulk flow in the near-Earth plasma sheet
... the observations of Yeoman and L¨uhr (1997) and Wild and Yeoman (2000) were inter- preted as the signatures of ionospheric Hall current vortices associated with field-aligned currents ...These two regions ... See full document
15
Geotail observations of FTE velocities
... the component of the mag- netic field perpendicular to the event axis is large, den- sities decrease for subsonic flows and increase for super- sonic ...the component of the magnetic field perpendicular to ... See full document
10
Observations of electron vorticity in the inner plasma sheet
... The initial onset is not seen by C3, which is the southern- most spacecraft in the constellation. However, it does see a similar increase in the velocity at about the time that the spacecraft exits the ion diffusion ... See full document
11
Contrasting dynamics of electrons and protons in the near Earth plasma sheet during dipolarization
... The exact moments of the first DF observation by differ- ent spacecraft (we will call this front the onset-related DF) are presented in Table 2, where this DF is marked as “DF0”. Assuming 1-D magnetic structure of DF we ... See full document
20
Observations of convection in the dayside magnetosphere by the beam instrument on Geotail
... reported observations of convection in the dayside magnetosphere by the beam instrument on ...the plasma at the Geotail locations is convected toward the ... See full document
8
Double frequency oscillations of low energy plasma associated with transverse Pc 5 pulsations: GEOTAIL satellite observations
... 1. Introduction A couple of decades ago, Kokubun et al. (1977) investi- gated particle flux variations associated with low-frequency hydromagnetic waves by using Ogo 5 satellite observations from which several ... See full document
11
Solar Wind Control of Density and Temperature in the Near-Earth Plasma Sheet: WIND-GEOTAIL Collaboration. Abstract
... magnetotail plasma sheet parameters on the solar wind is cen- tral to magnetospheric ...the plasma sheet population ...the plasma sheet protons, while the earth’s ... See full document
5
Cluster EDI convection measurements across the high-latitude plasma sheet boundary at midnight
... in two different ways in order to determine the magnitude and direction of the electron drift ...The two tech- niques are complementary in that triangulation is most ac- curate for small-to-moderate drifts, ... See full document
13
The magnetopause shape and location: a comparison of the Interball and Geotail observations with models
... the plasma rest frame, we cannot predict the actual value of perpendicular velocity components simply by the time shift of data without an analysis of the propaga- tion of the ... See full document
9
Occurrence rate of dipolarization fronts in the plasma sheet: Cluster observations
... any two DF events observed by different satellites as the same joint-observation DF event if their time difference is less than 30 s before ...any two adjacent DFs observed by different satellites with a ... See full document
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