Results 101 to 110 of about 252,334 (205)
Energetic positrons have been observed in the interstellar medium, and high-energy positrons with relativistic energies up to approximately 1 TeV have been detected in Galactic cosmic rays.
Huan Yu, Qi Xia, Jun Fang
doaj +1 more source
INTERPLANETARY SHOCKS LACKING TYPE II RADIO BURSTS
International audienceWe report on the radio-emission characteristics of 222 interplanetary (IP) shocks detected by spacecraft at Sun-Earth L1 during solar cycle 23 (1996 to 2006, inclusive).
Akiyama, S. +15 more
core +1 more source
Interplanetary Shocks and "Suprathermal" Flare Particles
We use ion-composition data from ACE/ULEIS, low energy electrons from ACE/EPAM, high energy protons from SoHO/ERNE, radio data from Wind/WAVES, and solar wind data from ACE/SWEPAM and ACE/MAG to investigate the solar and interplanetary circumstances near
vonRosenvinge, T. T. +2 more
core
MeV Ion Anisotropies in the Vicinity of Interplanetary Shocks
The anticipated signatures of interplanetary shock acceleration to be found in energetic ion anisotropies in the vicinity of interplanetary shocks include near-isotropic particle distributions consistent with of diffusive shock acceleration, "pancake ...
von Rosenvinge, T. T. +2 more
core
POLYTROPIC INDICES IN INTERPLANETARY SHOCK
Shao-liang Liu +2 more
openaire +1 more source
Shock-induced magnetic reconnection in the Venusian magnetotail. [PDF]
Zhang M +8 more
europepmc +1 more source
Energetic particle-mediated interplanetary shocks observed by Solar Orbiter
In collisionless shocks, energetic particles can carry enough pressure to modify the upstream plasma and the shock structure itself. This represents a regime that is often invoked in theories of cosmic-ray acceleration, but rarely observed in the ...
H. Hietala +12 more
core +1 more source
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
europepmc +1 more source
Interplanetary Coronal Mass Ejections During 1996 - 2007
Interplanetary coronal mass ejections, the interplanetary counterparts of coronal mass ejections at the Sun, are the major drivers of interplanetary shocks in the heliosphere, and are associated with modulations of the galactic cosmic ray intensity, both
Richardson, I. G., Cane, H. V.
core
Theory and observations of the interaction between magnetohydrodynamic waves and shocks. [PDF]
Zhao L +4 more
europepmc +1 more source

