Results 31 to 40 of about 2,952 (203)
Introduction: During recent years magnetosheath plasma structures called “jets” are identified in spacecraft data as localized regions in the magnetosheath where the dynamic pressure is enhanced compared to the background.
Marius Echim +9 more
doaj +1 more source
Solar wind reconstruction from magnetosheath data using an adjoint approach [PDF]
We present a new method to reconstruct solar wind conditions from spacecraft data taken during magnetosheath passages, which can be used to support, e.g., magnetospheric models.
C. Nabert +4 more
doaj +1 more source
On the Magnetic Field Configuration of the Magnetosheath
The magnetosheath is the region where the shocked solar wind interacts directly with the magnetosphere. Here we examine the magnetic field throughout the equatorial magnetosheath as a function of the solar wind IMF direction using observational data sets
Steven Michael Petrinec
doaj +1 more source
Jets in Planetary Magnetosheath
Abstract The study of jets in the Earth's magnetosheath has been a subject of extensive investigation for over a decade due to their profound impact on the geomagnetic environment and their close connection with shock dynamics. While the variability of the solar wind and its interaction with Earth's magnetosphere provide valuable insights into ...
Yufei Zhou +5 more
openaire +1 more source
First identification of mirror mode waves in Venus' magnetosheath?
In this paper first time observations of mirror mode like structures in Venus' magnetosheath are presented. Using magnetometer data from the Venus Express spacecraft it is shown that in two regions in the Venusian magnetosheath strong compressional waves
M. Volwerk +5 more
doaj +1 more source
Turbulence in the near-Venusian space: Venus Express observations
With Venus Express magnetic field measurements at 32 Hz from 2006 to 2012, we investigate statistically the magnetic fluctuations in the near-Venusian space.
SuDong Xiao +5 more
doaj +1 more source
A model of the magnetosheath magnetic field during magnetic clouds [PDF]
Magnetic clouds (MCs) are huge interplanetary structures which originate from the Sun and have a paramount importance in driving magnetospheric storms. Before reaching the magnetosphere, MCs interact with the Earth's bow shock.
L. Turc +3 more
doaj +1 more source
Energetic Electron Pitch-angle Distributions in the Martian Space Environment: Pancake
We perform a statistical investigation of the occurrence rates of energetic electron (100–500 eV) pancake pitch-angle distributions (PADs) in the Martian space environment by utilizing 6 yr of MAVEN data. In the Martian ionosphere, we find the following:
Z. Z. Guo, Y. Y. Liu, Z. Wang, Y. Xu
doaj +1 more source
Geoeffectiveness of Magnetosheath Jets
<p>The study on high speed plasma flows in the Earth&#8217;s magnetosheath, or commonly known as jets, has been a popular topic for discussion in recent decades. These jets can often be characterised by increases in the dynamic pressure compared to the background plasma.
Linus Norenius +6 more
openaire +2 more sources
The penetration of ions into the magnetosphere through the magnetopause turbulent current sheet [PDF]
This paper reports the results of numerical modeling of magnetosheath ion motion in the magnetopause current sheet (MCS) in the presence of magnetic fluctuations.
A. Taktakishvili +6 more
doaj +1 more source

