dc.contributor.author |
Roberts, B |
|
dc.date.accessioned |
2007-09-19T09:27:23Z |
|
dc.date.available |
2007-09-19T09:27:23Z |
|
dc.date.issued |
1996 |
|
dc.identifier.citation |
BASI, Vol.24 No. 2 pp. 199-210 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/1807 |
|
dc.description.abstract |
The influence of chromospheric magnetism on p- and f-modes is examined. The magnetism is modelled as a horizontal canopy field, embedded in an isothermal atmosphere, overlying a field-free polytropic convection zone. Both low and high frequency modes are considered. The recently detected solar cycle variability of p-modes is explored from the view-point of this model. The dual influence of convective motions and magnetism on the f-mode is discussed. |
en |
dc.format.extent |
1187144 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1996BASI...24..199R |
en |
dc.subject |
Magnetic effects |
en |
dc.subject |
p- and f-mode frequency shifts |
en |
dc.subject |
Activity cycle |
en |
dc.title |
The influence of chromospheric magnetism on oscillation frequencies |
en |
dc.type |
Article |
en |