Detection of visible-wavelength aurora on Mars. [PDF]
Knutsen EW +27 more
europepmc +1 more source
From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves. [PDF]
Turc L +9 more
europepmc +1 more source
Optimization of the grid-stiffened structure via PSO-LSSVR surrogate modeling and sensitivity analysis. [PDF]
Gai J +5 more
europepmc +1 more source
Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
europepmc +1 more source
SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]
Roy S +24 more
europepmc +1 more source
Remote sensing of mercury sodium exospheric patterns in relation to particle precipitation and interplanetary magnetic field. [PDF]
Orsini S +12 more
europepmc +1 more source
Simulation Models for Exploring Magnetic Reconnection. [PDF]
Shay M +24 more
europepmc +1 more source
A Survey of Current Operations-Ready Thermospheric Density Models for Drag Modeling in LEO Operations. [PDF]
Mutschler S +10 more
europepmc +1 more source
Solar and interplanetary particle acceleration
Abstract The nature and location of energetic particle acceleration (excluding planetary magnetospheres) in the inner heliosphere ( 1000 km/sec) coronal mass ejections is examined, but we find that they are not normally associated with relativistic energetic particle acceleration, although they may enhance the energy of particles already present in ...
Simnett, George
openaire +2 more sources
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Particle acceleration by propagating interplanetary shocks
AIP Conference Proceedings, 1979The process of charged particle acceleration in interplanetary shocks has been simulated for typical parameters. Since space probe observations of charged particle fluxes are the principle means of inferring the action of an acceleration mechanism, the simulation was designed to follow particles backwards in time from a given observing point, usually 1
R B Decker, Armstrong T P, Decker R B
exaly +2 more sources

