scholarly journals Generation of strong magnetic fields for magnetized plasma experiments at the 1-MA pulsed power machine

2021 ◽  
Vol 6 (4) ◽  
pp. 046901
Author(s):  
V. V. Ivanov ◽  
A. V. Maximov ◽  
R. Betti ◽  
L. S. Leal ◽  
J. D. Moody ◽  
...  
Keyword(s):  
Magnetic Fields ◽  
Pulsed Power ◽  
Magnetized Plasma ◽  
Strong Magnetic Fields ◽  
Power Machine

CTR Diagnostics for Laser Produced Electron Beams in MG Magnetic Fields Generated by the 1 Ma Pulsed Power Machine

2021 ◽  
Author(s):  
Noah Huerta ◽  
Vladimir Ivanov ◽  
Alexey Astanovitskiy
Keyword(s):  
Magnetic Fields ◽  
Electron Beams ◽  
Pulsed Power ◽  
Power Machine

Kinetic theory of stimulated Raman scattering from a magnetized plasma

1985 ◽  
Vol 33 (2) ◽  
pp. 303-319 ◽  
Author(s):  
T. J. M. Boyd ◽  
R. Rankin
Keyword(s):  
Magnetic Fields ◽  
Raman Scattering ◽  
Growth Rates ◽  
Stimulated Raman Scattering ◽  
Magnetized Plasma ◽  
Larmor Radius ◽  
Good Growth ◽  
Strong Magnetic Fields ◽  
Bernstein Waves ◽  
Stimulated Raman

Finite Larmor radius corrections have been considered in the effects of strong magnetic fields on stimulated Raman scattering. A nonlinear dispersion relation describing the various channels of decay has been derived from the Vlasov-Maxwell equations and frequencies and growth rates determined for the decay of incident laser light in the extraordinary mode into scattered extraordinary mode radiation and electron Bernstein waves. A relativistic one-and-a-half dimensional particle code has been used to simulate the scattering process and the results from the numerical experiments have been compared with those obtained analytically, the agreement being generally good. Growth rates of the Bernstein waves are substantial when sufficiently strong magnetic fields are present in hot plasmas. Under these conditions the kinetic analysis shows that, in contrast to the predictions of fluid theory, the scattered light emitted from densities well below the quarter-critical layer can have a frequency less than ½ω0 where ω0 is the laser frequency. In an unmagnetized plasma this occurs only when the plasma has a finite temperature.

Strong magnetic fields

1960 ◽  
Vol 70 (4) ◽  
pp. 693-714 ◽  
Author(s):  
G.M. Strakhovskii ◽  
N.V. Kravtsov
Keyword(s):  
Magnetic Fields ◽  
Strong Magnetic Fields

Magnetic molecular nanoclusters in strong magnetic fields

2002 ◽  
Vol 172 (11) ◽  
pp. 1303 ◽  
Author(s):  
Anatolii K. Zvezdin ◽  
Viktor V. Kostyuchenko ◽  
V.V. Platonov ◽  
V.I. Plis ◽  
A.I. Popov ◽  
...  
Keyword(s):  
Magnetic Fields ◽  
Strong Magnetic Fields

scholarly journals The measurement of the energy of cosmic rays - II—The curvature measurements and the energy spectrum

1936 ◽  
Vol 154 (883) ◽  
pp. 573-587 ◽  
Keyword(s):  
Magnetic Field ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
The Earth ◽  
Primary Particles ◽  
Curvature Measurements

Both the penetrating power of the cosmic rays through material ab­sorbers and their ability to reach the earth in spite of its magnetic field, make it certain that the energy of many of the primary particles must reach at least 10 11 e-volts. However, the energy measurements by Kunze, and by Anderson, using cloud chambers in strong magnetic fields, have extended only to about 5 x 10 9 e-volts. Particles of greater energy were reported, but the curvature of their tracks was too small to be measured with certainty. We have extended these energy measurements to somewhat higher energies, using a large electro-magnet specially built for the purpose and described in Part I. As used in these experiments, the magnet allowed the photography of tracks 17 cm long in a field of about 14,000 gauss. The magnet weighed about 11,000 kilos and used a power of 25 kilowatts.

scholarly journals Pseudo-spectral methods for atoms in strong magnetic fields

2010 ◽  
Vol 407 (1) ◽  
pp. 590-598 ◽  
Author(s):  
Jeremy S. Heyl ◽  
Anand Thirumalai
Keyword(s):  
Magnetic Fields ◽  
Spectral Methods ◽  
Strong Magnetic Fields ◽  
Pseudo Spectral

Electromagnetic Polarization in Partially Ionized Plasmas with Strong Magnetic Fields and Neutron Star Atmosphere Models

2004 ◽  
Vol 612 (2) ◽  
pp. 1034-1043 ◽  
Author(s):  
Alexander Y. Potekhin ◽  
Dong Lai ◽  
Gilles Chabrier ◽  
Wynn C. G. Ho
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
Ionized Plasmas ◽  
Partially Ionized Plasmas ◽  
Partially Ionized
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