Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical …
M Ruszkowski, C Pfrommer - The Astronomy and Astrophysics Review, 2023 - Springer
Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …
Closing in on the origin of Galactic cosmic rays using multimessenger information
JB Tjus, L Merten - Physics Reports, 2020 - Elsevier
In cosmic ray physics extensive progress has been made in recent years, both concerning
theory and observation. The vast details in direct, indirect and secondary detections on the …
theory and observation. The vast details in direct, indirect and secondary detections on the …
Pre-flight calibration and near-earth commissioning results of the mercury plasma particle experiment (MPPE) onboard MMO (Mio)
Y Saito, D Delcourt, M Hirahara, S Barabash… - Space Science …, 2021 - Springer
BepiColombo Mio (previously called MMO: Mercury Magnetospheric Orbiter) was
successfully launched by Ariane 5 from Kourou, French Guiana on October 20, 2018. The …
successfully launched by Ariane 5 from Kourou, French Guiana on October 20, 2018. The …
A database of MMS bow shock crossings compiled using machine learning
Identifying collisionless shock crossings in data sent from spacecraft has so far been done
manually or using basic algorithms. It is a tedious job that shock physicists have to go …
manually or using basic algorithms. It is a tedious job that shock physicists have to go …
Nonthermal electron acceleration at collisionless quasi-perpendicular shocks
Shock waves propagating in collisionless heliospheric and astrophysical plasmas have
been studied extensively over the decades. One prime motivation is to understand the …
been studied extensively over the decades. One prime motivation is to understand the …
[HTML][HTML] Shock propagation and associated particle acceleration in the presence of ambient solar-wind turbulence
The topic of this review paper is on the influence of solar wind turbulence on shock
propagation and its consequence on the acceleration and transport of energetic particles at …
propagation and its consequence on the acceleration and transport of energetic particles at …
Evidence of electron acceleration via nonlinear resonant interactions with whistler-mode waves at foreshock transients
Shock waves are sites of intense plasma heating and charged particle acceleration. In
collisionless solar wind plasmas, such acceleration is attributed to shock drift or Fermi …
collisionless solar wind plasmas, such acceleration is attributed to shock drift or Fermi …
Direct observations of energy transfer from resonant electrons to whistler-mode waves in magnetosheath of Earth
Electromagnetic whistler-mode waves in space plasmas play critical roles in collisionless
energy transfer between the electrons and the electromagnetic field. Although resonant …
energy transfer between the electrons and the electromagnetic field. Although resonant …
Theory of electron injection at oblique shock of finite thickness
A theory of electron injection into diffusive shock acceleration (DSA) for the generation of
cosmic-ray electrons at collisionless shocks is presented. We consider a recently proposed …
cosmic-ray electrons at collisionless shocks is presented. We consider a recently proposed …
Intense Whistler-mode Waves at Foreshock Transients: Characteristics and Regimes of Wave− Particle Resonant Interaction
Thermalization and heating of plasma flows at shocks result in unstable charged-particle
distributions that generate a wide range of electromagnetic waves. These waves, in turn, can …
distributions that generate a wide range of electromagnetic waves. These waves, in turn, can …