A Study of the Cross-Scale Dispersion Relation of the Fast-mode,Intermediate-mode and Slow-mode Waves in Space PlasmaA Study of the Cross-Scale Dispersion Relation of the Fast-mode, Intermediate-mode and Slow-mode Waves in Space Plasma
碩士 === 國立中央大學 === 太空科學研究所 === 99 === The magnetohydromagnetic (MHD) plasma model ignores the ion inertial effect, so it cannot explain the meso-scale and micro-scale plasma phenomena observed in the space. At the long-wavelength limit, the ion-electron two-fluid plasma model is equivalent to the MH...
Main Authors: | Yu-Chun Huang, 黃郁淳 |
---|---|
Other Authors: | Ling-Hsiao Lyu |
Format: | Others |
Language: | zh-TW |
Published: |
2011
|
Online Access: | http://ndltd.ncl.edu.tw/handle/67427666872152651903 |
Similar Items
-
Plasma frequency demand for mode conversion processes from slow Z-mode to LO-mode waves in an inhomogeneous plasma
by: Mohammad Javad Kalaee, et al.
Published: (2020-07-01) -
Plasma depletion layer: the role of the slow mode waves
by: Y. L. Wang, et al.
Published: (2004-12-01) -
Separating fast and slow modes in coupled chaotic systems
by: M. Peña, et al.
Published: (2004-01-01) -
Quasinormal modes and dispersion relations for quarkonium in a plasma
by: Nelson R. F. Braga, et al.
Published: (2019-01-01) -
Modeling the Dispersion of the Nonlinearity in Slow Mode Photonic Crystal Waveguides
by: S. Roy, et al.
Published: (2012-01-01)