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.
The CHIANTI database Adding Ionization and Recombination to CHIANTI Dr Peter Young CCLRC/Rutherford Appleton Laboratory, UK Dr Ken Dere George Mason University,
Progress and New Results from the H-1NF Scanning Interferometer Scott Collis, George Warr, John Howard.
3D GRMHD code RAISHIN and Relativistic Jet Simulations Yosuke Mizuno Center for Space Plasma and Aeronomic Research University of Alabama in Huntsville.
Relativistic MHD Simulations of Relativistic Jets
Fig.4: Typical values of the collisional and viscous damping time ratios for propagating a) Alfvén and fast magnetoacoustic waves and b) acoustic wave.
The Propagation Distance and Sources of Interstellar Turbulence
Relativistic MHD Simulations of Relativistic Jets Yosuke Mizuno NASA Postdoctoral Program Fellow NASA Marshall Space Flight Center (MSFC) National Space.
