Results 101 to 110 of about 639 (197)
Evidence for superdiffusive shock acceleration at interplanetary shock waves
Recent analysis of time profiles of energetic particles accelerated at interplanetary shocks has shown evidence for superdiffusive transport upstream of the shock fronts, namely for a transport characterized by a particle mean square displacement that grows faster than linearly in time.
Perri S, ZIMBARDO, Gaetano
openaire +1 more source
Abstract We present conjugate observations of ionospheric small‐scale magnetic perturbations (dB) $(dB)$ and GPS scintillations from the Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) and the Canadian High Arctic Ionospheric Network (CHAIN) during a storm‐time substorm on 9 August 2025 in the nightside auroral region ...
Yangyang Shen +12 more
wiley +1 more source
Pre‐Existing Plasmaspheric Density Structure
Abstract We perform a basic model experiment: we run two nearly identical plasmapause simulations, differing only by their initial conditions. The first run contains initial fine‐scale and mesoscale structure, and the second run is initialized with a featureless, circular plasmapause.
J. Goldstein, M. F. Thomsen
wiley +1 more source
Automatic Identification of Interplanetary Shocks Based on Machine Learning
Fast forward interplanetary shocks (FFs) are one of the primary drivers of space weather events. This study presents an automated detection algorithm for FFs based on a multilayer perceptron model, utilizing in situ measurements of interplanetary ...
Yi Tan +4 more
doaj +1 more source
Electron Energy Partition across Interplanetary Shocks. I. Methodology and Data Product. [PDF]
Wilson LB +12 more
europepmc +1 more source
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
Evolution of Electron Acceleration by Corotating Interaction Region Shocks at 1 au
We present the first observations of in situ electron acceleration at corotating interaction region (CIR) shocks near 1 au, utilizing measurements from Wind and Magnetospheric Multiscale (MMS) mission in the interplanetary medium. As the forward (reverse)
Xinnian Guo +6 more
doaj +1 more source
Interplanetary (IP) shocks efficiently modify the proton temperature anisotropy of the solar wind. Analyzing ∼800 IP shocks observed by the Wind spacecraft from 1997 to 2024, we present a statistical study of upstream and downstream proton temperature ...
Zeping Jin +8 more
doaj +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
POLYTROPIC INDICES IN INTERPLANETARY SHOCK
Shao-liang Liu +2 more
openaire +1 more source

