Non-linear plasma wave decay to longer wavelength

Author(s):  
F. Anderegg ◽  
M. Affolter ◽  
A. Ashourvan ◽  
D. H. E. Dubin ◽  
F. Valentini ◽  
...  
2010 ◽  
Vol 53 (1) ◽  
pp. 014008 ◽  
Author(s):  
S Kneip ◽  
S R Nagel ◽  
C Bellei ◽  
O Cheklov ◽  
R J Clarke ◽  
...  

1993 ◽  
Vol 10 (4) ◽  
pp. 283-286 ◽  
Author(s):  
Andrew Melatos ◽  
Peter Robinson

AbstractClumpy, intense wave packets observed in situ in the Jovian and terrestrial electron foreshocks, and in the Earth’s auroral acceleration zone, point to the existence of non-linear plasma turbulence in these regions. In non-linear turbulence, wave packets collapse to short scales and high fields, stopping only when coherent wave-particle interactions efficiently dissipate the energy in the waves. The purpose of this paper is to examine the shortest scales and highest fields achieved during collapse in a strongly magnetised plasma, and identify parts of the solar system where the magnetised aspects of wave collapse are important.


2020 ◽  
Vol 1531 ◽  
pp. 012021
Author(s):  
Kanwal Gurbakhsish Kaur ◽  
Pawan Kumar ◽  
Niti Kant ◽  
Jyoti Rajput

2001 ◽  
Vol 56-57 ◽  
pp. 755-759 ◽  
Author(s):  
J.B Lister ◽  
R Khayrutdinov ◽  
D.J.N Limebeer ◽  
V Lukash ◽  
Y Nakamura ◽  
...  

1973 ◽  
Vol 13 (6) ◽  
pp. 807-816 ◽  
Author(s):  
J. Jancarik ◽  
V.N. Tsytovich

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