dc.creator |
Guenther, David B. |
|
dc.creator |
Kim, Y.-C. |
|
dc.creator |
Demarque, P. |
|
dc.date.accessioned |
2015-02-19T15:41:25Z |
|
dc.date.available |
2015-02-19T15:41:25Z |
|
dc.date.issued |
1996-05-20 |
|
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://library2.smu.ca/xmlui/handle/01/25962 |
|
dc.description |
Publisher's version/PDF |
en_CA |
dc.description.abstract |
The OPAL equation-of-state tables and the MHD equation-of-state tables are utilized in the calculation of new standard solar models that also include helium diffusion. The structure of the models and their l = 0-100 p-mode oscillation spectra are compared. The p-mode frequencies of the standard solar model are dramatically and nearly identically affected by the inclusion of these detailed equation-of-state formulations. The sensitivities of the p-mode frequencies to other physical uncertainties, in particular the surface conditions, are also discussed. |
en_CA |
dc.description.provenance |
Submitted by Janine Mills (janine.mills@smu.ca) on 2015-02-19T15:41:25Z
No. of bitstreams: 1
Guenther_David_B_1996_a.pdf: 203043 bytes, checksum: f670289b2871b0edb6d8bdc264aed417 (MD5) |
en |
dc.description.provenance |
Made available in DSpace on 2015-02-19T15:41:25Z (GMT). No. of bitstreams: 1
Guenther_David_B_1996_a.pdf: 203043 bytes, checksum: f670289b2871b0edb6d8bdc264aed417 (MD5)
Previous issue date: 1996-05-20 |
en |
dc.language.iso |
en |
en_CA |
dc.publisher |
American Astronomical Society |
en_CA |
dc.relation.uri |
http://dx.doi.org/10.1086/177252 |
|
dc.rights |
Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user. |
|
dc.subject.lcsh |
Helioseismology |
|
dc.subject.lcsh |
Sun -- Internal structure |
|
dc.subject.lcsh |
Solar oscillations |
|
dc.title |
Seismology of the standard solar model: tests of diffusion and the OPAL and the MHD equations of state |
en_CA |
dc.type |
Text |
en_CA |
dcterms.bibliographicCitation |
Astrophysical Journal 463, 382-390. (1996) |
en_CA |