Electrostatic Waves with Rapid Frequency Shifts in the Solar Wind from PSP observations

Author(s):  
Lily Kromyda ◽  
David M. Malaspina ◽  
Robert E. Ergun ◽  
Jasper Halekas ◽  
Michael L. Stevens ◽  
...  
2008 ◽  
Author(s):  
D. A. Gurnett ◽  
W. S. Kurth ◽  
L. F. Burlaga ◽  
M. H. Acuna ◽  
N. F. Ness ◽  
...  

2021 ◽  
Author(s):  
Ahmad Lalti ◽  
Yuri Khotyaintsev ◽  
Daniel Graham ◽  
Andris Vaivad ◽  
Andreas Johlander

<p>Energy dissipation at collisionless shocks is still an open question. Wave particle interactions are believed to be at the heart of it, but the exact details are still to be figured out. One type of waves that is known to be an efficient dissipator of solar wind kinetic energy are electrostatic waves in the shock ramp, such as ion acoustic waves with frequency around the ion plasma frequency or Bernstein waves with frequency around the electron cyclotron frequency and its harmonics. The electric field of such waves is typically larger than 100 mV/m, large enough to disturb particle dynamics. In this study we use the magnetospheric multiscale (MMS) spacecraft, to investigate the source and evolution of electrostatic waves in the shock ramp of quasi-perpendicular super-critical shocks, and study their effect on solar wind thermalization.</p>


1988 ◽  
Vol 8 (1) ◽  
pp. 35-38 ◽  
Author(s):  
N. Omidi ◽  
T.Z. Ma ◽  
K. Quest ◽  
M. Ashour-Abdalia ◽  
D. Gurnett ◽  
...  

2021 ◽  
Vol 48 (17) ◽  
Author(s):  
Yuki Harada ◽  
Yoshiya Kasahara ◽  
Masaki N. Nishino ◽  
Satoshi Kurita ◽  
Yoshifumi Saito ◽  
...  

Author(s):  
D. B. Graham ◽  
Yu. V. Khotyaintsev ◽  
A. Vaivads ◽  
N. J. T. Edberg ◽  
A. I. Eriksson ◽  
...  

1984 ◽  
Vol 75 ◽  
pp. 597
Author(s):  
E. Grün ◽  
G.E. Morfill ◽  
T.V. Johnson ◽  
G.H. Schwehm

ABSTRACTSaturn's broad E ring, the narrow G ring and the structured and apparently time variable F ring(s), contain many micron and sub-micron sized particles, which make up the “visible” component. These rings (or ring systems) are in direct contact with magnetospheric plasma. Fluctuations in the plasma density and/or mean energy, due to magnetospheric and solar wind processes, may induce stochastic charge variations on the dust particles, which in turn lead to an orbit perturbation and spatial diffusion. It is suggested that the extent of the E ring and the braided, kinky structure of certain portions of the F rings as well as possible time variations are a result of plasma induced electromagnetic perturbations and drag forces. The G ring, in this scenario, requires some form of shepherding and should be akin to the F ring in structure. Sputtering of micron-sized dust particles in the E ring by magnetospheric ions yields lifetimes of 102to 104years. This effect as well as the plasma induced transport processes require an active source for the E ring, probably Enceladus.


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