Parallel proton fire hose instability in the expanding solar wind: Hybrid simulations

2006 ◽  
Vol 111 (A10) ◽  
Author(s):  
Lorenzo Matteini ◽  
Simone Landi ◽  
Petr Hellinger ◽  
Marco Velli
Keyword(s):  
Solar Wind ◽  
Fire Hose ◽  
Hybrid Simulations

scholarly journals Influence of He ++ and Shock Geometry on Interplanetary Shocks in the Solar Wind: 2D Hybrid Simulations

2020 ◽  
Vol 125 (4) ◽  
Author(s):  
L. Preisser ◽  
X. Blanco‐Cano ◽  
D. Trotta ◽  
D. Burgess ◽  
P. Kajdič
Keyword(s):  
Solar Wind ◽  
Interplanetary Shocks ◽  
Hybrid Simulations

First lunar wake passage of ARTEMIS: Discrimination of wake effects and solar wind fluctuations by 3D hybrid simulations

2011 ◽  
Vol 59 (8) ◽  
pp. 661-671 ◽  
Author(s):  
S. Wiehle ◽  
F. Plaschke ◽  
U. Motschmann ◽  
K.-H. Glassmeier ◽  
H.U. Auster ◽  
...  
Keyword(s):  
Solar Wind ◽  
Lunar Wake ◽  
Wake Effects ◽  
Hybrid Simulations

scholarly journals Hybrid Simulations of Interstellar Pickup Protons Accelerated at the Solar-wind Termination Shock at Multiple Locations

2021 ◽  
Vol 911 (1) ◽  
pp. 27
Author(s):  
J. Giacalone ◽  
M. Nakanotani ◽  
G. P. Zank ◽  
J. Kòta ◽  
M. Opher ◽  
...  
Keyword(s):  
Solar Wind ◽  
Termination Shock ◽  
Solar Wind Termination Shock ◽  
Hybrid Simulations

scholarly journals The Kelvin-Helmholtz Instability From the Perspective of Hybrid Simulations

2021 ◽  
Vol 8 ◽  
Author(s):  
P. A. Delamere ◽  
N. P. Barnes ◽  
X. Ma ◽  
J. R. Johnson
Keyword(s):  
Solar Wind ◽  
Surface Waves ◽  
Energy Transport ◽  
Helmholtz Instability ◽  
Flow Shear ◽  
Planetary Magnetospheres ◽  
Dayside Magnetopause ◽  
Hybrid Simulations

The flow shear-driven Kelvin-Helmholtz (KH) instability is ubiquitous in planetary magnetospheres. At Earth these surface waves are important along the dawn and dusk flanks of the magnetopause boundary while at Jupiter and Saturn the entire dayside magnetopause boundary can exhibit KH activity due to corotational flows in the magnetosphere. Kelvin-Helmholtz waves can be a major ingredient in the so-called viscous-like interaction with the solar wind. In this paper, we review the KH instability from the perspective of hybrid (kinetic ions, fluid electrons) simulations. Many of the simulations are based on parameters typically found at Saturn’s magnetopause boundary, but the results can be generally applied to any KH-unstable situation. The focus of the discussion is on the ion kinetic scale and implications for mass, momentum, and energy transport at the magnetopause boundary.

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