Results 21 to 30 of about 16,773 (267)

In Situ Observation of a Magnetopause Indentation that Is Correspondent to Throat Aurora and Is Caused by Magnetopause Reconnection

open access: yesGeophysical Research Letters, 2022
Throat auroras have been suggested to correspond to magnetopause indentations, but how such indentations can be generated is an open question. Using coordinated magnetopause in situ and two‐dimensional auroral imaging observations, we showed that a ...
HuiXuan Qiu   +8 more
doaj   +1 more source

Electron Bulk Heating at Saturn's Magnetopause [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2020
Abstract Magnetic reconnection at the magnetopause (MP) energizes ambient plasma via the release of magnetic energy and produces an “open” magnetosphere allowing solar wind particles to directly enter the system. At Saturn, the nature of MP reconnection remains unclear.
I. Cheng   +5 more
openaire   +5 more sources

Global MHD Simulations of Neptune's Magnetosphere [PDF]

open access: yes, 2016
A global magnetohydrodynamic (MHD) simulation has been performed in order to investigate the outer boundaries of Neptune's magnetosphere at the time of Voyager 2's flyby in 1989 and to better understand the dynamics of magnetospheres formed by highly ...
Chittenden, J   +3 more
core   +1 more source

The magnetopause shape and location: a comparison of the Interball and Geotail observations with models [PDF]

open access: yesAnnales Geophysicae, 2002
A number of magnetopause models have been developed in the course of last three decades. We have chosen seven of them and tested them using a fresh set of magnetopause crossings observed by Interball-1, Magion-4, and Geotail satellites.
J. Šafránková   +5 more
doaj   +1 more source

IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites—a mission concept proposed for the ESA M3 2020/2022 launch [PDF]

open access: yes, 2012
The dayside magnetopause is the primary site of energy transfer from the solar wind into the magnetosphere, and modulates the activity observed within the magnetosphere itself.
Amm, O.   +19 more
core   +3 more sources

Extreme geomagnetic disturbances due to shocks within CMEs [PDF]

open access: yes, 2015
We report on features of solar wind-magnetosphere coupling elicited by shocks propagating through coronal mass ejections (CMEs) by analyzing the intense geomagnetic storm of 6 August 1998.
Baker   +28 more
core   +2 more sources

Statistical survey of day-side magnetospheric current flow using Cluster observations: magnetopause [PDF]

open access: yesAnnales Geophysicae, 2017
We present a statistical survey of current structures observed by the Cluster spacecraft at high-latitude day-side magnetopause encounters in the close vicinity of the polar cusps.
E. Liebert   +4 more
doaj   +1 more source

Ion Larmor radius effects near a reconnection X line at the magnetopause: THEMIS observations and simulation comparison [PDF]

open access: yes, 2016
We report a Time History of Events and Macroscale Interactions during Substorms (THEMIS-D) spacecraft crossing of a magnetopause reconnection exhaust ~9 ion skin depths (di) downstream of an X line. The crossing was characterized by ion jetting at speeds
Angelopoulos, V   +10 more
core   +1 more source

Magnetopause transects

open access: yesGeophysical Research Letters, 1996
A novel method is described for reconstruction of two‐dimensional current‐layer structures from measurements taken by a single spacecraft traversing the layer. In its present form, the method is applicable only to 2D magneto‐hydrostatic structures that are passively convected past the observing spacecraft. It is tested on a magnetopause crossing of the
B. U. Ö. Sonnerup, M. Guo
openaire   +1 more source

Juno Magnetometer Observations at Ganymede: Comparisons With a Global Hybrid Simulation and Indications of Magnetopause Reconnection

open access: yesGeophysical Research Letters, 2022
Juno's flyby of Ganymede on 7 June 2021, provides a unique opportunity to explore the moon's magnetosphere. By means of Magnetometer (MAG) observations and a hybrid numerical simulation, we provide a global description of this environment and analyze the
N. Romanelli   +11 more
doaj   +1 more source

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