Global magnetic reconnection during sustained sub‐Alfvénic Solar wind driving

BL Burkholder, LJ Chen, M Sarantos… - Geophysical …, 2024 - Wiley Online Library
When the solar wind speed falls below the local Alfvén speed, the magnetotail transforms
into an Alfvén wing configuration. A Grid Agnostic Magnetohydrodynamics for Extended …

Precise and efficient orbit prediction in LEO with machine learning using exogenous variables

F Caldas, C Soares - 2024 IEEE Congress on Evolutionary …, 2024 - ieeexplore.ieee.org
The increasing volume of space objects in Earth's orbit presents a significant challenge for
Space Situational Awareness (SSA). And in particular, accurate orbit prediction is crucial to …

Complex interaction of reconnected field lines at Earth's magnetopause under sub‐Alfvénic solar wind with northward magnetic field

H Hasegawa, RE Denton, LJ Chen… - Journal of …, 2024 - Wiley Online Library
We present observations on 24 April 2023 by the Magnetospheric Multiscale spacecraft at
the dayside, mid‐latitude magnetopause, when an interplanetary magnetic cloud (MC) with …

Dawn‐dusk asymmetry of the magnetopause distance under the parker spiral configuration of the IMF

B Janda, F Němec, Z Němeček… - Journal of Geophysical …, 2024 - Wiley Online Library
The dawn‐dusk asymmetry of the magnetopause radial distance under the Parker (and
ortho‐Parker) configuration of the interplanetary magnetic field (IMF) is investigated. An …

Two-dimensional MHD simulation of the Earth's magnetosphere

S Filawati, B Setiahadi, BA Subagyo - Astrophysics and Space Science, 2023 - Springer
The magnetosphere is the outermost part of the Earth, formed by the interaction of the
Earth's dipole magnetic field and the solar wind. Solar wind conditions depend on solar …