scholarly journals High‐Frequency Plasma Waves and Pitch Angle Scattering Induced by Pulsed Electron Beams

2019 ◽  
Vol 124 (9) ◽  
pp. 7543-7552
Author(s):  
G. L. Delzanno ◽  
V. Roytershteyn
Keyword(s):  
High Frequency ◽  
Pitch Angle ◽  
Electron Beams ◽  
Plasma Waves ◽  
Angle Scattering ◽  
High Frequency Plasma ◽  
Frequency Plasma

Coupling between High-Frequency Plasma Waves in Laser-Plasma Interactions

1995 ◽  
Vol 74 (12) ◽  
pp. 2236-2239 ◽  
Author(s):  
M. J. Everett ◽  
A. Lal ◽  
C. E. Clayton ◽  
W. B. Mori ◽  
T. W. Johnston ◽  
...  
Keyword(s):  
Laser Plasma ◽  
High Frequency ◽  
Plasma Waves ◽  
Plasma Interactions ◽  
Laser Plasma Interactions ◽  
High Frequency Plasma ◽  
Frequency Plasma

Nonlinear propagation of high-frequency plasma waves in a magnetized plasma

1977 ◽  
Vol 18 (2) ◽  
pp. 249-256 ◽  
Author(s):  
P. K. Shukla
Keyword(s):  
High Frequency ◽  
Nonlinear Effects ◽  
Plasma Waves ◽  
Electron Plasma ◽  
Magnetized Plasma ◽  
Nonlinear Propagation ◽  
Arbitrary Angle ◽  
High Frequency Plasma ◽  
Frequency Plasma ◽  
Density Perturbations

We study nonlinear effects associated with large amplitude electron plasma waves propagating at an arbitrary angle to the external magnetic field. It is shown that the nonlinear coupling of high-frequency plasma waves with static density perturbations leads to a convective instability. The growth length of the latter is obtained. The evolution of the wave electric field is also investigated.

scholarly journals Solar Orbiter’s first Venus Flyby: MAG observations of structures and waves associated with the induced Venusian magnetosphere

2021 ◽  
Author(s):  
Martin Volwerk ◽  
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
High Frequency ◽  
Cyclotron Frequency ◽  
Plasma Waves ◽  
Bow Shock ◽  
High Frequency Plasma ◽  
Frequency Plasma ◽  
Mirror Mode ◽  
Proton Cyclotron

<p>The induced magnetosphere of Venus is created by the interaction of the solar wind and embedded interplanetary magnetic field with the exosphere and ionosphere of Venus. Solar Orbiter entered Venus’s magnetotail far downstream, > 70 Venus radii, of the planet and exited the magnetosphere over the north pole. This offered a unique view of the system over distances that were only flown through once by three other missions before, Mariner 10, Galileo and Bepi-Colombo. The large-scale structure and activity of the induced magnetosphere is studied as well as the high-frequency plasma waves both in the magnetosphere and in a limited region upstream of the planet where interaction with Venus’s exosphere is expected.  It is shown that Venus’s magnetotail is very active during the Solar Orbiter flyby. Structures such as flux ropes, and reconnection sites are encountered as well as a strongly overdraping of the magnetic field downstream of the bow shock and planet. High-frequency plasma waves (up to 6 times the local proton cyclotron frequency) are observed in the magnetotail, which are identified as Doppler-shifted proton cyclotron waves, whereas in the upstream solar wind these waves appear just below the proton cyclotron frequency (as expected) but are very patchy. The bow shock is quasi perpendicular, however, expected mirror mode activity is not found directly behind it; instead there is strong cyclotron wave power. This is most-likely caused by the relatively low plasma-beta  behind the bow shock. Much further downstream in the magnetosheath mirror mode of magnetic hole structures are identified. This presentation will take place after the second Venus flyby by Solar Orbiter and BepiColombo and Solar Orbiter on 9 and 10 August, respectively.</p>

scholarly journals Wind/WAVES observations of high-frequency plasma waves in solar wind reconnection exhausts

2007 ◽  
Vol 112 (A1) ◽  
pp. n/a-n/a ◽  
Author(s):  
K. E. J. Huttunen ◽  
S. D. Bale ◽  
T. D. Phan ◽  
M. Davis ◽  
J. T. Gosling
Keyword(s):  
Solar Wind ◽  
High Frequency ◽  
Wind Waves ◽  
Plasma Waves ◽  
High Frequency Plasma ◽  
Frequency Plasma

The Development of Polyethylene Naphthalate Films by Low-pressure High-frequency Plasma Chemical Vapor Deposition System with Advance Oxidations Process

2015 ◽  
Vol 18 (1) ◽  
Author(s):  
Nuttee Thungsuk ◽  
Toshifumi Yuji ◽  
Narong Mungkung ◽  
Yoshimi Okamura ◽  
Atsushi Fujimaru ◽  
...  
Keyword(s):  
Chemical Vapor Deposition ◽  
Vapor Deposition ◽  
High Frequency ◽  
Chemical Vapor ◽  
Low Pressure ◽  
Polyethylene Naphthalate ◽  
Plasma Chemical ◽  
Plasma Chemical Vapor Deposition ◽  
High Frequency Plasma ◽  
Frequency Plasma

AbstractThe low-pressure high-frequency plasma chemical vapor deposition (CVD) system was developed with non-thermal plasma process to study the Polyethylene naphthalate (PEN) surface characteristics. Plasma surface treatment by oxygen can improve the adhesive properties. A mixture of Ar and O

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