Results 71 to 80 of about 7,959 (209)

Mshpy23: a user-friendly, parameterized model of magnetosheath conditions

open access: yesEarth and Planetary Physics
Lunar Environment heliospheric X-ray Imager (LEXI) and Solar wind−Magnetosphere−Ionosphere Link Explorer (SMILE) will observe magnetosheath and its boundary motion in soft X-rays for understanding magnetopause reconnection modes under various solar wind ...
Jaewoong Jung   +5 more
doaj   +1 more source

Statistical Study of Short Large‐Amplitude Magnetic Structures at Mars Observed by MAVEN

open access: yesJournal of Geophysical Research: Space Physics, Volume 131, Issue 4, April 2026.
Abstract We present a statistical study of Short Large‐Amplitude Magnetic Structures (SLAMS) in the Martian foreshock using data from the Mars Atmosphere and Volatile Evolution (MAVEN) mission between 01 January 2015 and 31 December 2019. We have identified 21,008 SLAMS during this time interval and statistical results are presented on the SLAMS ...
Tsz Kiu Wong Chan   +2 more
wiley   +1 more source

Atmospheric Effects of Magnetosheath Jets

open access: yesAtmosphere, 2022
We report effects in the upper high-latitude atmosphere related to the interaction of fast magnetosheath plasma streams, so-called jets, with the dayside magnetopause. The jets were observed by THEMIS mission in the dayside magnetosphere during a quiet day on 12 July 2009.
Alexei V. Dmitriev, Alla V. Suvorova
openaire   +2 more sources

The Pointing Error Due To Laser Propagation in Space Plasma for TianQin Gravitational Wave Detection

open access: yesSpace Weather, Volume 24, Issue 4, April 2026.
Abstract TianQin, a space‐borne gravitational wave observatory, is designed to detect gravitational‐wave signals via laser interferometry. As the inhomogeneous space plasma surrounds the inter‐satellite laser links, the propagation of the laser in space plasma can introduce pointing error noise.
Shenwei Zhou   +4 more
wiley   +1 more source

On the formation of a plasma pressure anisotropy in the dayside magnetosheath [PDF]

open access: yesAnnales Geophysicae, 1995
We present a numerical solution for the momentum equation of the magnetosheath particles that describes the distribution of the pressure anisotropy of the magnetosheath plasma in the midday meridian plane. The pressure anisotropy is a maximum near the
B. V. Rezhenov   +2 more
doaj   +1 more source

Turbulence-generated proton-scale structures in the terrestrial magnetosheath [PDF]

open access: yes, 2016
Recent results of numerical magnetohydrodynamic simulations suggest that in collisionless space plasmas turbulence can spontaneously generate thin current sheets.
Consolini, Giuseppe   +4 more
core   +3 more sources

Global Energy Circulation During a Solar Wind Density Pulse

open access: yesSpace Weather, Volume 24, Issue 4, April 2026.
Abstract We study the propagation and impacts of a strong density pulse through the magnetosphere during 11:40–12:00 UT near the peak of a geomagnetic storm on 3 February 2022. Using the Space Weather Modeling Framework Geospace global simulation, we show how the energy transport in the magnetosphere is enhanced promptly after the pulse arrival at the ...
Tuija Pulkkinen   +5 more
wiley   +1 more source

Sunward flow in Jupiter's magnetosheath

open access: yesGeophysical Research Letters, 1980
The position of Voyager crossings of Jupiter's bow shock show a dependence on solar wind pressure to the −1/3 power. This dependence is used to calculate typical bow shock speeds of 50 km/s from Voyager solar wind plasma data. Since the bow shock and magnetopause move approximately in unison in response to solar wind pressure changes, the resulting ...
G. L. Siscoe   +2 more
openaire   +1 more source

Classifying Magnetosheath Jets using MMS - Statistical Properties [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2019
Abstract Using Magnetospheric Multiscale (MMS) data, we find, classify, and analyze transient dynamic pressure enhancements in the magnetosheath (jets) from May 2015 to May 2019. A classification algorithm is presented, using in situ MMS data to classify jets ( ) into ...
Savvas Raptis   +4 more
openaire   +1 more source

Unveiling the 3D Structure of Magnetosheath Jets

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
Magnetosheath jets represent localized enhancements in dynamic pressure observed within the magnetosheath. These energetic entities, carrying excess energy and momentum, can impact the magnetopause and disrupt the magnetosphere. Therefore, they play a vital role in coupling the solar wind and terrestrial magnetosphere. However, our understanding of the
Shahab Fatemi   +6 more
openaire   +2 more sources

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