[PDF] Top 20 Ion multi-nose structures observed by Cluster in the inner Magnetosphere
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Ion multi-nose structures observed by Cluster in the inner Magnetosphere
... that nose structure can be formed under a global large scale electric ...simulated nose energy range is slightly above the observed one and its energy width is much ...features observed at the ... See full document
20
Observations of lower hybrid cavities in the inner magnetosphere by the Cluster and Viking satellites
... at Cluster al- titudes compared with the ...and Cluster altitudes than expected from simple field line scaling from Freja height, one may at least infer that individual LHCs do not extend all along a ... See full document
12
Revision of empirical electric field modeling in the inner magnetosphere using Cluster data
... index, which is the same as in the Volland-Stern model. Maynard and Chen [1975] tried to match K p -dependent loca- tions of LCE in the Volland-Stern model with measured plasmapause locations. Korth et al. [1999] ... See full document
17
Cluster observation of few-hour-scale evolution of structured plasma in the inner magnetosphere
... the ion population as temporal changes by, for example, ion energization, transport, or loss, with a timescale on the order of 1 ...an ion signature is energy–latitude dispersed, this difference ... See full document
10
Conjugate observation of sharp dynamical boundary in the inner magnetosphere by Cluster and DMSP spacecraft and ground network
... We believe such sharp transition between two different pop- ulations can only be formed dynamically, as a result of col- lision of two different plasmas. The inferred earthward- eastward propagation supports this ... See full document
10
Comparison of eight years magnetic field data from Cluster with Tsyganenko models in the inner magnetosphere
... 4 Cluster spacecraft with Tsyganenko 1989 (T89), 1996 (T96), and 2001 (T01) field models, while Clus- ter passes through, or adjacent to, the equatorial ring cur- rent, has been carried out which significantly ... See full document
18
Multi-spacecraft observation of plasma dipolarization/injection in the inner magnetosphere
... the inner magnetosphere, we investi- gate the 23 February 2004 substorm using a favorable con- stellation of four Cluster (near perigee), LANL and Geo- tail ...were observed by Cluster ... See full document
14
Ion drift simulation of sudden appearance of sub-keV structured ions in the inner magnetosphere
... the Cluster SC-4 ...of observed protons from the start location that is located at 8 R E on the ...the observed space–time, and, therefore, the figure contains even high-energy ions that are not ... See full document
8
IMF and the seasonal dependences of the electric field in the inner magnetosphere
... from Cluster EDI, which is based on a newly devel- oped technique well suited for measurements of the electric fields in the inner ...the inner magnetosphere are indeed dependent on the po- ... See full document
8
Spatial spreading of magnetospherically reflected chorus elements in the inner magnetosphere
... Abstract. Chorus-type whistler waves are known to be gen- erated in the vicinity of the magnetic equator, in the low- density plasma trough region. These wave packets propa- gate towards the magnetic poles, deviating ... See full document
7
Field line resonance structures in Mercury’s multi ion magnetosphere
... The observed magnetic component of transverse waves tends to be strongly linearly polarized and oriented ap- proximately perpendicular to the estimated field gradient (which is plasma ...two- ion simulations ... See full document
5
Shell-like configuration in O ion velocity distribution at high altitudes in the dayside magnetosphere observed by Cluster/CIS
... + ion veloc- ity distributions both observed in the Southern Hemisphere on 13 February 2001 and 14 April 2001, and the observa- tion conditions were as mentioned in the previous ...+ ion velocity ... See full document
11
Multiple discrete-energy ion features in the inner magnetosphere: 9 February 1998, event
... “nose” structure increases with L, but the high energy edge of the band 5 decreases with L. 4.2 W2K convection model Calculated spectra under the W2K model are shown in panels 5 and 6 of Fig. 1. In comparison with ... See full document
8
Solitary potential structures observed in the magnetosheath by the Cluster spacecraft
... potential structures in the magnetosheath, as well as in all other regions of its orbit, during the time period of 1 February through 30 May ...tical structures on more than one spacecraft, so that we can ... See full document
9
Characteristics of high altitude oxygen ion energization and outflow as observed by Cluster: a statistical study
... for multi space- craft measurements, Kluwer Academic Publishers, ...multispacecraft ion measurements in and near the Earth’s magnetosphere with the identical Cluster ... See full document
14
Analysis of plasma waves observed in the inner Saturn magnetosphere
... the electrons. In Fig. 14a we plot the electron phase space density measured by ELS for electrons near 1 keV versus pitch angle for the time interval 03:15:20–03:15:30 (inter- val 1), while in Fig. 14b we plot the same ... See full document
14
Simulation of electromagnetic ion cyclotron triggered emissions in the Earth's inner magnetosphere
... background magnetic field. We assume a parabolic magnetic field to model the dipole magnetic field in the equatorial region of the inner magnetosphere. Triggering EMIC waves are driven by a left‐handed ... See full document
9
Inner magnetosphere heavy ion composition during high-speed stream-driven storms
... is observed prior to ...all ion species is observed to increase. The recovery of ion flux commences at low energies initially and then extends to higher energies during the extended period of ... See full document
14
A comparison between ion characteristics observed by the POLAR and DMSP spacecraft in the high-latitude magnetosphere
... total ion counts from the CAMMICE MICS in- strument aboard the POLAR spacecraft are used to generate occurrence probability distributions of magnetospheric ion ...MICS ion spectra are characterised ... See full document
14
First multispacecraft ion measurements in and near the Earth’s magnetosphere with the identical Cluster ion spectrometry (CIS) experiment
... that there is a significant difference between the locations of the peaks for different positions. Since the peaks move closer together with energy, but the width of the low mass ions does not significantly improve, ... See full document
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