dc.contributor.author |
Satya Narayanan, A |
|
dc.contributor.author |
Ramesh, R |
|
dc.date.accessioned |
2008-07-15T11:38:44Z |
|
dc.date.available |
2008-07-15T11:38:44Z |
|
dc.date.issued |
2002-09 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 3, pp. 573 - 576 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2690 |
|
dc.description.abstract |
The combined effect of non-parallel propagation, steady :flow
and inclined magnetic field on the . propagation characteristics of hydromagnetic
surface waves is examined. The fluid is assumed to be perfectly conducting,
infinite in extent with an interface which supports body modes as well as surface
modes. This model also supports fast, Al:fven and slow modes depending on
the parametric values of the system. These modes have interesting applications
in the solar corona and solar wind. |
en |
dc.format.extent |
96346 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Hydromagnetic Waves |
en |
dc.subject |
Corona |
en |
dc.subject |
Solar Wind |
en |
dc.title |
Interfacial hydromagnetic waves with shear and inclined magnetic fields |
en |
dc.type |
Article |
en |