Flare-driven habitability: Expanding life's potential around low-mass stars. [PDF]
Gao DY, Liu HG, Yang M, Zhou JL.
europepmc +1 more source
Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]
Kubyshkina D +9 more
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A Survey of Current Operations-Ready Thermospheric Density Models for Drag Modeling in LEO Operations. [PDF]
Mutschler S +10 more
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Polarity-resolved far-side magnetograms based on helioseismic measurements. [PDF]
Hamada A +4 more
europepmc +1 more source
Reduction of the space dimension of parameters characterizing geomagnetic storms during the Solar Cycle 24. [PDF]
Siluszyk A +5 more
europepmc +1 more source
Starspots as the origin of ultrafast drifting radio bursts from an active M dwarf. [PDF]
Zhang J +18 more
europepmc +1 more source
Electrodynamic forcing of the Duskside ionosphere and the super fountain effect during the superstorm of May 10 to 11 2024. [PDF]
Venugopal I, Thampi SV, Bhaskar A.
europepmc +1 more source
Observation-based modelling of magnetised coronal mass ejections with EUHFORIA [PDF]
Context. Coronal mass ejections (CMEs) are the primary source of strong space weather disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic pressure and internal magnetic fields, for which reliable predictions at Earth are
Camilla Scolini +2 more
exaly +2 more sources
In times of growing technological sophistication and of our dependence on electronic technology, we are all affected by space weather. In its most extreme form, space weather can disrupt communications, damage and destroy spacecraft and power stations ...
Howard, Timothy, Timothy Howard
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