Electron heating and acceleration at collisionless shocks in the solar wind

2000 ◽  
Author(s):  
J. T. Gosling
Keyword(s):  
Solar Wind ◽  
Collisionless Shocks ◽  
Electron Heating

Modeling proton and electron heating in the fast solar wind

2020 ◽  
Author(s):  
L. Adhikari ◽  
G.P. Zank ◽  
L.-L. Zhao ◽  
M. Nakanotani ◽  
S. Tasnim
Keyword(s):  
Solar Wind ◽  
Fast Solar Wind ◽  
Electron Heating

On Solar-Wind Electron Heating at Large Solar Distances

Solar Physics ◽  
2013 ◽  
Vol 289 (4) ◽  
pp. 1359-1370 ◽  
Author(s):  
Igor V. Chashei ◽  
Hans J. Fahr
Keyword(s):  
Solar Wind ◽  
Electron Heating ◽  
Solar Wind Electron

scholarly journals Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection

2013 ◽  
pp. 557-587
Author(s):  
Parviz Ghavamian ◽  
Steven J. Schwartz ◽  
Jeremy Mitchell ◽  
Adam Masters ◽  
J. Martin Laming
Keyword(s):  
Solar Wind ◽  
Supernova Remnant ◽  
Ion Temperature ◽  
Collisionless Shocks

Particle energisation and transport at collisionless shocks propagating through turbulent media.

2021 ◽  
Author(s):  
Domenico Trotta ◽  
Francesco Valentini ◽  
David Burgess ◽  
Sergio Servidio
Keyword(s):  
Solar Wind ◽  
Vlasov Equation ◽  
Coarse Graining ◽  
Bow Shock ◽  
Plasma Transport ◽  
Collisionless Shocks ◽  
Turbulent Structures ◽  
Novel Technique ◽  
Earth’S Bow Shock

<p>Shocks and turbulence are spectacular, ubiquitous phenomena and are crucial ingredients to understand the production and transport of energetic particles in several astrophysical systems. The interaction between an oblique, supercritical shock and fully developed plasma turbulence is here investigated by means of kinetic simulations, for different turbulence amplitudes. The role of pre-existing, upstream turbulence on plasma transport is addressed using a novel technique, relying on the coarse-graining of the Vlasov equation. We find that the upstream transport properties strongly depend on upstream turbulence strength, with patterns modulated by the presence of turbulent structures. These results are relevant for a variety of systems, ranging from the Earth's bow shock interacting with solar wind turbulence, to the largest scales of radio relics in galaxy clusters.</p>

scholarly journals Electron-Ion Temperature Equilibration in Collisionless Shocks: The Supernova Remnant-Solar Wind Connection

2013 ◽  
Vol 178 (2-4) ◽  
pp. 633-663 ◽  
Author(s):  
Parviz Ghavamian ◽  
Steven J. Schwartz ◽  
Jeremy Mitchell ◽  
Adam Masters ◽  
J. Martin Laming
Keyword(s):  
Solar Wind ◽  
Supernova Remnant ◽  
Ion Temperature ◽  
Collisionless Shocks
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