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The top documents tagged [ionized plasmas]
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Acoustic waves (case k = 0 ) -- Important for non-magnetized regions in the low solar atmosphere: Eqs. (10),(6) = (12) Fig. 3: Defined by Eq(12) variation
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The CHIANTI database Adding Ionization and Recombination to CHIANTI Dr Peter Young CCLRC/Rutherford Appleton Laboratory, UK Dr Ken Dere George Mason University,
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Progress and New Results from the H-1NF Scanning Interferometer Scott Collis, George Warr, John Howard
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Relativistic MHD Simulations of Relativistic Jets Yosuke Mizuno NASA Postdoctoral Program Fellow NASA Marshall Space Flight Center (MSFC) National Space
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3D GRMHD code RAISHIN and Relativistic Jet Simulations Yosuke Mizuno Center for Space Plasma and Aeronomic Research University of Alabama in Huntsville
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Relativistic MHD Simulations of Relativistic Jets
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Fig.4: Typical values of the collisional and viscous damping time ratios for propagating a) Alfvén and fast magnetoacoustic waves and b) acoustic wave
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The Propagation Distance and Sources of Interstellar Turbulence
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