Computer Science
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cath.rept.....w&link_type=abstract
Final Report, 1 Jun. 1986 - 31 May 1989 Catholic Univ. of America, Washington, DC. Dept. of Mechanical Engineering.
Computer Science
Interplanetary Space, Magnetohydrodynamics, Shock Waves, Solar Corona, Stellar Mass Ejection, Parameterization, Solar Activity, Solar Wind, Wave Propagation
Scientific paper
Shock waves of the solar terrestrial medium in coronal and interplanetary space was studied. The understanding on the propagation of large amplitude disturbances from the solar corona through the interplanetary space is enhanced. Work accomplished during the past three years includes: (1) a demonstrating example showing the formation of slow shock pairs associated with Coronal Mass Ejections (CMEs) in a coronal environment; (2) a parametric study of slow shocks in the entire domain of a 3-D parameter space, the A, theta, beta-space; (3) the large scale geometry of traveling interplanetary shocks; (4) the transition of slow shocks to fast shocks in the inner solar wind; and (5) the evolution of CME associated shocks and their interplanetary manifestations.
No associations
LandOfFree
MHD (Magnetohydrodynamic) slow shocks in coronal and interplanetary space does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with MHD (Magnetohydrodynamic) slow shocks in coronal and interplanetary space, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MHD (Magnetohydrodynamic) slow shocks in coronal and interplanetary space will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1515427