Results 11 to 20 of about 5,126 (305)

Atomic Physics for Hot Plasmas [PDF]

open access: yesInternational Astronomical Union Colloquium, 1988
This report treats some aspects of how to obtain and apply main atomic characteristics responsible for the intensities and satellite structures of spectral lines in hot plasmas.The experimental test, of theoretical methods and calculated cross- sections σ is often possible only in a plasma, especially for highly charged ions.
L.A. VAINSHTEIN
openaire   +4 more sources

Assessment of quasi-linear effect of RF power spectrum for enabling lower hybrid current drive in reactor plasmas [PDF]

open access: yesEPJ Web of Conferences, 2017
The main research on the energy from thermonuclear fusion uses deuterium plasmas magnetically trapped in toroidal devices. To suppress the turbulent eddies that impair thermal insulation and pressure tight of the plasma, current drive (CD) is necessary ...
Cesario Roberto   +10 more
doaj   +2 more sources

Structural Variations of Dust Acoustic Solitary Waves (DASWs) Propagating in an Inhomogeneous Plasma

open access: yesEast European Journal of Physics, 2023
This paper presents our theoretical investigations on the structural variations of dust acoustic solitary waves (DASWs) in inhomogeneous unmagnetized plasmas.
Hirak Jyoti Dehingia, P.N. Deka
doaj   +1 more source

Reduced field Scenario with X3 heating in W7-X [PDF]

open access: yesEPJ Web of Conferences, 2019
In the present work, an ECRH scenario with reduced magnetic field 1.75 T is considered. For 140 GHz, this field corresponds to X3 heating. The high mirror-ratio magnetic configuration, B01/B00 ≃ 0.24, was considered as one from most attractive for long ...
Marushchenko Nikolai B.   +8 more
doaj   +1 more source

Production of a Hot Rotating Plasma [PDF]

open access: yesThe Physics of Fluids, 1962
The design and operation of Homopolar V are described. The device was designed so that there would be no driftvelocity (or voltage) limit as had been encountered in earlier experiments. Experiments with the device show that rotating plasmas need not suffer from a serious velocity limit, at least.
Halbach, Klaus   +2 more
openaire   +2 more sources

Fast and slow magnetosonic shock waves in non-Maxwellian plasmas

open access: yesResults in Physics, 2023
Obliquely propagating nonlinear fast and slow magnetosonic wave modes in a hot non-Maxwellian dissipative plasma are investigated in the current work.
Navaira Izhar   +3 more
doaj   +1 more source

Inner screening corrections to the Debye interaction in hot/dense plasmas in the vicinity of the bound – free transitions

open access: yesPhysical Sciences and Technology, 2021
Considering hot/dense plasmas strongly ionized and still retaining hydrogenic bound states (1 ≤ z ≤ 6), we focus attention on the delocalization features of ion-electron orbitals, such as wide spreading and attending of pertaining wave ...
C. Deutsch, G. Naouri, N.A.Tahir
doaj   +1 more source

Obliquely propagating electron acoustic solitons in magnetized plasmas with nonextensive electrons [PDF]

open access: yesNonlinear Processes in Geophysics, 2013
The problem of small amplitude electron-acoustic solitary waves (EASWs) is discussed using the reductive perturbation theory in magnetized plasmas consisting of cold electrons, hot electrons obeying nonextensive distribution and stationary ions.
H. R. Pakzad, K. Javidan
doaj   +1 more source

Simulation of Electron Acoustic Wave Propagation in Non-Uniform Magnetized Plasma [PDF]

open access: yesIranian Journal of Astronomy and Astrophysics, 2021
The Propagation of electron acoustic solitary waves is studied in a plasmas consisting of hot and cold electrons and stationary ions and in the presence of nonuniform external magnetic field.
Hamid Reza Pakzad
doaj   +1 more source

Opacity calculation for target physics using the ABAKO/RAPCAL code [PDF]

open access: yes, 2010
Radiative properties of hot dense plasmas remain a subject of current interest since they play an important role in inertial confinement fusion (ICF) research, as well as in studies on stellar physics.
Rodriguez, R.   +13 more
core   +2 more sources

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