Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/1803
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Dappen, W | - |
dc.date.accessioned | 2007-09-19T07:05:35Z | - |
dc.date.available | 2007-09-19T07:05:35Z | - |
dc.date.issued | 1996 | - |
dc.identifier.citation | BASI, Vol.24 No. 2 pp. 151-160 | en |
dc.identifier.uri | http://hdl.handle.net/2248/1803 | - |
dc.description.abstract | The helioseismic verification of major nonideal effects in the equation of state of solar matter has become well established. The dominant contribution is the Coulomb pressure, conventionally described in the Debye-Huckel approximation. Recently, the increased precesion of the helioseismic diagnosis has brought significant observational progress beyond the Debye-Huckel approximation. Obviously, progress in the equation of state serves two purposes. For solar physicists, a better equation of state will lead to reduced uncertainty in solar models. For plasma physicists, it will lead to an astrophysical experiment, in a domain where there is not much laboratory competition. | en |
dc.format.extent | 1084659 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..151D | en |
dc.subject | Helioseismology | en |
dc.subject | Equation of state | en |
dc.subject | Solar interior | en |
dc.title | Helioseismic diagnosis of the equation of state | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
dappen.pdf | 1.06 MB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.