Results 21 to 30 of about 282,550 (204)
The possible influence of MHD turbulence on the energy distributions of ions in the Earth's plasma sheet was studied using data taken by the THEMIS satellites.
A. V. Eyelade +9 more
doaj +1 more source
High-beta plasma blobs in the morningside plasma sheet [PDF]
Equator-S frequently encountered, i.e. on 30% of the orbits between 1 March and 17 April 1998, strong variations of the magnetic field strength of typically 5–15-min duration outside about 9RE during the late-night/early-morning hours.
G. Haerendel +9 more
doaj +1 more source
The Role of Mesoscale Plasma Sheet Dynamics in Ring Current Formation
During geomagnetically active periods ions are transported from the magnetotail into the inner magnetosphere and accelerated to energies of tens to hundreds of keV. These energetic ions, of mixed composition with the most important species being H+ and O+
K. A. Sorathia +8 more
doaj +1 more source
Response of convection electric fields in the magnetosphere to IMF orientation change [PDF]
[1] The transient response of convection electric fields in the inner magnetosphere to southward turning of the interplanetary magnetic field (IMF) is investigated using in‐situ electric field observations by the CRRES and Akebono spacecraft.
Brautigam, D. +7 more
core +1 more source
World-Sheet Duality, Space-Time Foam, and the Quantum Fate of a Stringy Black Hole [PDF]
We interpret Minkowski black holes as world-sheet {\it spikes } which are related by world-sheet { \it duality} to {\it vortices } that correspond to Euclidean black holes. These world-sheet defects induce defects in the gauge fields of the corresponding
Abrikosov +48 more
core +4 more sources
Plasma sheet expansion: Statistical characteristics [PDF]
The present study addresses the cause of plasma sheet expansion by statistically comparing the characteristics of lobe‐to‐plasma sheet (LB‐to‐PS) and PS‐to‐LB crossings observed by the Geotail satellite. Whereas the flapping motion of the magnetotail causes both types of crossing, the PS expansion (thinning) can be associated only with the LB‐to‐PS (PS‐
S. Ohtani, T. Mukai
openaire +1 more source
Properties of plasmas that constitute the plasma sheet in the near-Earth magnetotail vary according to the solar wind conditions and location in the tail. In this case study, we present multi-spacecraft observations by Cluster that show a transition of
Hee-Eun Kim, Ensang Lee
doaj +1 more source
Measurement of plasma impedance in sheet plasma.
For plasma heating by the ion cyclotron resonance (ICR), we have measured the plasma impedance when a RF electric field is applied to the plasma. The minimum value of R appears near f-72kHz.
Takahiko WAKATSUKI +4 more
openaire +2 more sources
Magnetization of the plasma sheet [PDF]
Long‐term‐averaged three‐dimensional data‐based models were made of the −30 < x < −10, ∣y∣ < 15, ∣z∣ < 5 RE plasma sheet region. The average magnetic moments 〈μ〉 and Chew‐Goldberger‐Low (CGL) double adiabatic parameters α⊥ and α∥ were evaluated for ions and electrons.
Richard L. Kaufmann +2 more
openaire +1 more source
Electron firehose instabilities can be excited at dipolarization fronts and in the magnetic reconnection outflow in the terrestrial magnetotail, but their occurrence rate in the plasma sheet is unclear.
Jiayun Wei +8 more
doaj +1 more source

