Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1638
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Christensen-Dalsgaard, J | - |
dc.date.accessioned | 2007-06-11T09:18:40Z | - |
dc.date.available | 2007-06-11T09:18:40Z | - |
dc.date.issued | 1996 | - |
dc.identifier.citation | BASI, Vol. 24, No. 2, pp. 103 - 116 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1638 | - |
dc.format.extent | 1296522 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of India | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1996BASI...24..103C | en |
dc.subject | Sun | en |
dc.subject | Helioseismology | en |
dc.title | How are the observed frequencies related to solar structure? | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Paper_2.pdf | 1.27 MB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.