Results 171 to 180 of about 1,276 (215)

Detection of visible-wavelength aurora on Mars. [PDF]

open access: yesSci Adv
Knutsen EW   +27 more
europepmc   +1 more source

From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves. [PDF]

open access: yesSpace Sci Rev
Turc L   +9 more
europepmc   +1 more source

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

open access: yesLiving Rev Sol Phys
Veronig AM   +12 more
europepmc   +1 more source

SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]

open access: yesSci Data
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]

open access: yesSci Rep
Orsini S   +12 more
europepmc   +1 more source

Simulation Models for Exploring Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Shay M   +24 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

Solar and interplanetary particle acceleration

open access: yesAdvances in Space Research, 2003
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

Particle acceleration by propagating interplanetary shocks

AIP Conference Proceedings, 1979
The 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

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