Citation: Jjg. Lima et al., An analytical MHD wind model with latitudinal dependences obtained using separation of the variables, ASTRON ASTR, 371(1), 2001, pp. 240-249
Citation: T. Neukirch et Er. Priest, Generalization of a special class of time-dependent solutions of the two-dimensional magnetohydrodynamic equations to arbitrary pressure profiles, PHYS PLASMA, 7(7), 2000, pp. 3105-3107
Citation: Ds. Brown et Er. Priest, Topological differences and similarities between force-free and potential models of coronal magnetic fields, SOLAR PHYS, 194(2), 2000, pp. 197-204
Authors:
Mackay, DH
Galsgaard, K
Priest, ER
Foley, CR
Citation: Dh. Mackay et al., How accurately can we determine the coronal heating mechanism in the large-scale solar corona?, SOLAR PHYS, 193(1-2), 2000, pp. 93-116
Citation: Vs. Titov et al., On the nature of chaotic regions in dissipative hydrodynamics and magnetohydrodynamics, PHYS PLASMA, 6(4), 1999, pp. 1374-1377