Employing analogies for ducted MHD waves in dense coronal structures

Details Employing analogies for ducted MHD waves in dense coronal structures Employing analogies for ducted MHD waves in dense coronal structures

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192..343e&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 343-347. NASA-sponsored research.

Astronomy and Astrophysics

Astrophysics

21

Magnetohydrodynamic Waves, Solar Corona, Wave Propagation

Scientific paper

Analogies of fast MHD waves propagating along a dense coronal structure are exploited to examine how the size and shape of the inhomogeneity affect the properties of the Love- and Pekeris-type waves. The profile's shape determines the dispersive nature of the waves. Excited impulsively, magnetic Love and Pekeris waves give rise to quasi-periodic oscillations with a duration and time scale that depend on the cross-sectional area and strength of the inhomogeneity. More diffuse coronal inhomogeneities support impulsively generated periodic oscillations, with the quasi-periodic signature being absent.

Affiliated with

Also associated with

No associations

Rating

Employing analogies for ducted MHD waves in dense coronal structures 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 Employing analogies for ducted MHD waves in dense coronal structures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Employing analogies for ducted MHD waves in dense coronal structures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1669850