Results 31 to 40 of about 1,092,232 (226)
Comments on "Plasma current drive by injection of photons with helicity" [Comm. Plasma Phys. Controlled Fusion 12, 165 (1989)] [PDF]
Ohkawa has proposed a tokamak current-drive scheme [Comm. Plasma Phys. Controlled Fusion 12, 165 (1989)], which relies on the injection of circularly polarized magnetohydrodynamic waves.
Bellan, P. M., Schalit, M. A.
core +1 more source
Can useful toroidal current be driven by classical viscoresistive Alfvén waves? [PDF]
Simple, yet exact, analytic solutions for the shear and compressional Alfvén wave are obtained for helical magnetohydrodynamic (MHD) waves in cylindrical geometry with both resistivity and viscosity included.
Bellan, P. M., Schalit, M. A.
core +1 more source
Previously, Tsurutani and Lakhina (2014, https://doi.org/10.1002/2013GL058825) created estimates for a “perfect” interplanetary coronal mass ejection and performed simple calculations for the response of geospace, including dB/dt.
Daniel T. Welling +5 more
doaj +1 more source
How Transverse Waves Drive Turbulence in the Solar Corona
Oscillatory power is pervasive throughout the solar corona, and magnetohydrodynamic (MHD) waves may carry a significant energy flux throughout the Sun’s atmosphere.
T. Howson
semanticscholar +1 more source
Understanding energetic particle transport due to magnetohydrodynamic instabilities excited by energetic particles is essential to apprehend alpha particle confinement in a fusion burning plasma.
K. Ogawa +12 more
semanticscholar +1 more source
Toward 3D MHD modeling of neoclassical tearing mode suppression by ECCD
We propose a framework to extend the magnetohydrodynamic (MHD) equations to include electron cyclotron current drive (ECCD) and discuss previous models proposed by Giruzzi et al. [2] and by Hegna and Callen [3].
Westerhof E., Pratt J.
doaj +1 more source
High-order coupling of shear and sonic continua in JET plasmas
A recent model coupling the shear-Alfvén and acoustic continua, which depends strongly on the equilibrium shaping and on elongation in particular, is employed to explain the properties of Alfvénic activity observed on JET plasmas below but close to the ...
Paulo Rodrigues +10 more
doaj +1 more source
Tidally driven dynamos in a rotating sphere [PDF]
Large-scale planetary or stellar magnetic fields generated by a dynamo effect are mostly attributed to flows forced by buoyancy forces in electrically conducting fluid layers.
Cébron, David, Hollerbach, Rainer
core +3 more sources
Reconnection Studies Under Different Types of Turbulence Driving [PDF]
We study a model of fast magnetic reconnection in the presence of weak turbulence proposed by Lazarian and Vishniac (1999) using three-dimensional direct numerical simulations. The model has been already successfully tested in Kowal et al.
Kowal, Grzegorz +3 more
core +2 more sources
A reduced magnetohydrodynamic model of coronal heating in open magnetic regions driven by reflected low-frequency waves [PDF]
A reduced magnetohydrodynamic (RMHD) description is employed to examine a suggestion made by W. H. Matthaeus and colleagues in 1999 that coronal heating might be sustained by a cascade of low-frequency MHD turbulence.
Dmitruk, Pablo +5 more
core +2 more sources

