Results 31 to 40 of about 940 (176)

Magnetosheath-cusp interface [PDF]

open access: yesAnnales Geophysicae, 2004
Abstract. We advance the achievements of Interball-1 and other contemporary missions in exploration of the magnetosheath-cusp interface. Extensive discussion of published results is accompanied by presentation of new data from a case study and a comparison of those data within the broader context of three-year magnetopause (MP) crossings by Interball-1.
S. Savin   +35 more
openaire   +5 more sources

On the Magnetic Field Configuration of the Magnetosheath

open access: yesTerrestrial, Atmospheric and Oceanic Sciences, 2013
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

Turbulence in the near-Venusian space: Venus Express observations

open access: yesEarth and Planetary Physics, 2020
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

Kinetic‐Scale Turbulence in the Venusian Magnetosheath [PDF]

open access: yesGeophysical Research Letters, 2020
Abstract While not specifically designed as a planetary mission, NASA's Parker Solar Probe (PSP) mission uses a series of Venus gravity assists (VGAs) in order to reduce its perihelion distance. These orbital maneuvers provide the opportunity for direct measurements of the Venus plasma environment at high cadence.
T. A. Bowen   +27 more
openaire   +4 more sources

Magnetosheath waves under very low solar wind dynamic pressure: Wind/Geotail observations [PDF]

open access: yesAnnales Geophysicae, 2005
The expanded bow shock on and around "the day the solar wind almost disappeared" (11 May 1999) allowed the Geotail spacecraft to make a practically uninterrupted 54-h-long magnetosheath pass near dusk (16:30-21:11 magnetic local time) at a radial ...
C. J. Farrugia   +10 more
doaj   +1 more source

Energetic Electron Pitch-angle Distributions in the Martian Space Environment: Pancake

open access: yesThe Astrophysical Journal, 2023
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

The penetration of ions into the magnetosphere through the magnetopause turbulent current sheet [PDF]

open access: yesAnnales Geophysicae, 2003
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

Geoeffectiveness of Magnetosheath Jets

open access: yes, 2020
<p>The study on high speed plasma flows in the Earth’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

Cluster observations of bounday layer structure and a flux transfer event near the cusp [PDF]

open access: yesAnnales Geophysicae, 2005
On the 25th January 2002 between 10:00 and 12:00 UT, the four Cluster spacecraft passed through the northern high-latitude cusp, the dayside magnetosphere and into the magnetosheath in a linear formation.
R. C. Fear   +8 more
doaj   +1 more source

The Evolution of Parallel Electric Field Across the Earth's Magnetosheath

open access: yesGeophysical Research Letters, Volume 53, Issue 19, 16 October 2026.
Abstract In Earth's collisionless magnetosheath, turbulence evolution and energy transformation across the system, especially at kinetic scales, remain poorly quantified without full‐coverage of high‐resolution observations. Using multi‐traversal observations from the 2023 and 2024 Magnetospheric Multiscale (MMS) Unbiased Magnetosheath Campaign, we ...
Y. Qi   +5 more
wiley   +1 more source

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