Results 1 to 10 of about 69,396 (273)
Dissipative Pulsar Magnetosphere [PDF]
Dissipative axisymmetric pulsar magnetosphere is calculated by a direct numerical simulation of the Strong-Field Electrodynamics equations. The magnetic separatrix disappears, it is replaced by a region of enhanced dissipation.
Andrei Gruzinov +2 more
core +2 more sources
Global-scale magnetosphere convection driven by dayside magnetic reconnection [PDF]
Plasma convection on a global scale is a fundamental feature of planetary magnetosphere. The Dungey cycle explains that steady-state convection within the closed part of the magnetosphere relies on magnetic reconnection in the nightside magnetospheric ...
Lei Dai +10 more
doaj +2 more sources
Controlling of merging electric field and IMF magnitude on storm-time changes in thermospheric mass density [PDF]
The controls of merging electrical field, Em, and IMF (interplanetary magnetic field) magnitude, B, on the storm-time changes in upper thermospheric mass density are statistically investigated using GRACE accelerometer observations and the OMNI data ...
Y. L. Zhou +4 more
doaj +1 more source
Observations of a Mini‐Magnetosphere Above the Martian Crustal Magnetic Fields
Mars is typically regarded as a non‐magnetic planet. Currents in the Martian ionosphere generate a Venus‐like induced magnetosphere which deflects the solar wind flows and piles up the interplanetary magnetic fields.
Kai Fan +9 more
doaj +1 more source
Large-scale current systems in the ionosphere and the magnetosphere are intimately controlled by the solar wind-magnetosphere interaction and the magnetosphere-ionosphere coupling.
Guan Le +14 more
doaj +1 more source
Is Our Understanding of Solar-Wind/Magnetosphere Coupling Satisfactory?
An assessment of our physics-based understanding of solar-wind/magnetosphere coupling finds that the understanding is not complete. Solar-wind/magnetosphere coupling is foundational to magnetospheric physics and it is a key to comprehending and ...
Joseph E. Borovsky
doaj +1 more source
Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission
Mercury’s southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury flyby.
S. Orsini +91 more
doaj +1 more source
Reconsideration on the concept model of throat aurora
The solar wind-magnetosphere-ionosphere coupling driven by the solar wind is a systematic process that involves the buffering of magnetosheath and the response and feedback of magnetosphere and ionosphere.
Desheng Han, Huixuan Qiu, Run Shi
doaj +1 more source
BLACK HOLE MAGNETOSPHERES [PDF]
10 pages, 4 figures, recommended for publication in the Astrophysical ...
Antonios Nathanail, Ioannis Contopoulos
openaire +3 more sources
Kp index correlates with the many magnetosphere properties, which are used to measure the level of magnetic activity. In the solar system, the two different planets, Mercury with weak magnetic field and Jupiter with strong magnetic field, are selected ...
Mays M. Al-Gbory, Najat Mohamed Ameen
doaj +1 more source

