dc.contributor.author |
Gokhale, M. H |
|
dc.date.accessioned |
2008-09-20T11:45:00Z |
|
dc.date.available |
2008-09-20T11:45:00Z |
|
dc.date.issued |
1988 |
|
dc.identifier.citation |
IAU Symposium, No. 123, pp. 219 - 222 |
en |
dc.identifier.issn |
0074-1809 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3746 |
|
dc.description.abstract |
A spherical harmonic Fourier analysis of the maximum areas of sunspot groups listed in Ledgers I and II of Greenwich photoheliographic results for 1933 - 1954 yield significant peaks at the 11 y periodicity for some spherical harmonic modes: especially the mode (l = 6, m = 0). A similar analysis of the daily areas of the spotgroups during 1944 - 1954 yields 11 y periodicity peaks only for some non-axisymmetric modes. These results suggest that the sunspot activity may be physically related to long period global oscillations of the sun. |
en |
dc.language.iso |
en |
en |
dc.publisher |
International Astronomical Union |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1988IAUS..123..219G |
en |
dc.subject |
Global Oscillations |
en |
dc.subject |
Sunspots |
en |
dc.title |
Study of Longperiod Global Oscillations of Sun Through Spherical Harmonic Fourier Analysis of Sunspot Activity |
en |
dc.type |
Article |
en |