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Global magnetic reconnection during sustained sub‐Alfvénic Solar wind driving
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 …
into an Alfvén wing configuration. A Grid Agnostic Magnetohydrodynamics for Extended …
Precise and efficient orbit prediction in LEO with machine learning using exogenous variables
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 …
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
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 …
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 …
ortho‐Parker) configuration of the interplanetary magnetic field (IMF) is investigated. An …
Two-dimensional MHD simulation of the Earth's magnetosphere
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 …
Earth's dipole magnetic field and the solar wind. Solar wind conditions depend on solar …