Results 81 to 90 of about 1,158 (191)
Corotating drift-bounce resonance of plasmaspheric electron with poloidal ULF waves
The purpose of this paper is to understand how low energy plasmaspheric electrons respond to ULF waves excited by interplanetary shocks impinging on magnetosphere. It is found that both energy and pitch angle dispersed plasmaspheric electrons with energy
Qiu-Gang Zong +6 more
doaj +1 more source
Variations of Heavy Ions in Different Types of Interplanetary Shocks
Heavy ions upstream and downstream of interplanetary shocks are not only subject to acceleration, heating, and spatiotemporal modulation during their propagation in interplanetary space, but they can also, in turn, influence the dynamical properties of ...
Cong Wang, Qian Ye, Xuan Cheng, Fei He
doaj +1 more source
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
Pickup ions (PUIs) often experience acceleration and heating as they traverse interplanetary shocks, leading to the formation of a distinct suprathermal tail in their energy spectra downstream of the shock.
Weining Wang +5 more
doaj +1 more source
Solar Orbiter encounters an unusually high Mach number interplanetary shock
Aims. The objective of this study is to characterise and understand the magnetic structure of an extremely high Mach number interplanetary shock. Methods.
Dimmock A. P. +7 more
doaj +1 more source
Modelling large solar proton events with the shock-and-particle model
We have developed a new version of a model that combines a two-dimensional Sun-to-Earth magnetohydrodynamic (MHD) simulation of the propagation of a CME-driven shock and a simulation of the transport of particles along the interplanetary magnetic field ...
Pomoell Jens +5 more
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
Evolution of Turbulence at an Interplanetary Shock Observed by the Solar Orbiter and Wind Spacecraft
This work presents a case study of the evolution of turbulence in the vicinity of an interplanetary shock observed by Solar Orbiter (SolO) at 0.83 au and Wind at 1 au on 2023 November 30.
Sujan Prasad Gautam +3 more
doaj +1 more source
Electron cyclotron harmonic (ECH) waves are electrostatic emissions frequently observed in the Earth’s magnetosphere. By precipitating magnetospheric hot electrons into the ionosphere, ECH waves play a critical role in the formation of diffuse aurora ...
Yi Xie +18 more
doaj +1 more source
Shock-induced magnetic reconnection in the Venusian magnetotail
Magnetic reconnection, a universal process governing energy release in astrophysical plasmas, has long been studied as a key phenomenon in magnetized planets. However, its drivers and impacts in unmagnetized bodies remain poorly understood.
Meng Zhang +8 more
doaj +1 more source

