Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]
Kubyshkina D +9 more
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Wavelet Coherence Analysis of Plasma Beta, Alfven Mach Number, and Magnetosonic Mach Number during Different Geomagnetic Storms. [PDF]
Giri A +4 more
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SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]
Roy S +24 more
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Unexpected major geomagnetic storm caused by faint eruption of a solar trans-equatorial flux rope. [PDF]
Teng W, Su Y, Ji H, Zhang Q.
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Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
europepmc +1 more source
Relation between magnetopause position and reconnection rate under quasi-steady solar wind dynamic pressure. [PDF]
Kim H +5 more
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Solar Wind Magnetosphere Ionosphere Link Explorer (SMILE): Science and Mission Overview. [PDF]
Wang C +3 more
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Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun. [PDF]
Gopalswamy N +5 more
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Evaluation of the <i>Salmonella</i> type 3 secretion system (T3SS) as part of a protein production platform for space biology applications. [PDF]
Kang MK, Bevington J, Tullman-Ercek D.
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STEREO interplanetary shocks and foreshocks
AIP Conference Proceedings, 2013We use STEREO data to study shocks driven by stream interactions and the waves associated with them. During the years of the extended solar minimum 2007-2010, stream interaction shocks have Mach numbers between 1.1-3.8 and θBn ∼20-86°. We find a variety of waves, including whistlers and low frequency fluctuations.
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