Results 231 to 240 of about 54,745 (274)

Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]

open access: yesSpace Sci Rev
Kubyshkina D   +9 more
europepmc   +1 more source

A Survey of Current Operations-Ready Thermospheric Density Models for Drag Modeling in LEO Operations. [PDF]

open access: yesJ Astronaut Sci
Mutschler S   +10 more
europepmc   +1 more source

Polarity-resolved far-side magnetograms based on helioseismic measurements. [PDF]

open access: yesSci Rep
Hamada A   +4 more
europepmc   +1 more source

Reduction of the space dimension of parameters characterizing geomagnetic storms during the Solar Cycle 24. [PDF]

open access: yesSci Rep
Siluszyk A   +5 more
europepmc   +1 more source

Starspots as the origin of ultrafast drifting radio bursts from an active M dwarf. [PDF]

open access: yesSci Adv
Zhang J   +18 more
europepmc   +1 more source

Observation-based modelling of magnetised coronal mass ejections with EUHFORIA [PDF]

open access: yesAstronomy and Astrophysics, 2019
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

Coronal Mass Ejections

open access: yes, 2011
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
core   +3 more sources

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