Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium

Details Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.103...95v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 103, no. 1, Aug. 1984, p. 95-98.

Astronomy and Astrophysics

Astrophysics

2

Coriolis Effect, Interplanetary Medium, Magnetohydrodynamic Waves, Propagation Velocity, Rotating Matter, Shock Wave Propagation, Cylindrical Waves, Equations Of Motion, Interplanetary Gas, Magnetic Fields, Rotating Fluids, Solar Activity Effects, Solar Wind

Scientific paper

Strong cylindrical magnetogasdynamic shock waves in rotating
interplanetary medium have been studied and an analytic solution for
their propagation has been obtained. Using characteristic method and
considering the effect of Coriolis force, the authors have shown that
magnetic field has significant effect on the velocity of the shock wave.

Affiliated with

Also associated with

No associations

Rating

Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium 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 Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Strong cylindrical magnetogasdynamic shock waves in a rotating interplanetary medium will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674018