Prospects and Challenges for Helioseismology
Author:
Toomre J.,Thompson M. J.
Publisher
Springer Netherlands
Reference110 articles.
1. H.M. Antia, S. Basu, Determining solar abundances using helioseismology. Astrophys. J. 644, 1292–1298 (2006). doi: 10.1086/503707 2. T. Appourchaux, K. Belkacem, A.-M. Broomhall, W.J. Chaplin, D.O. Gough, G. Houdek, J. Provost, F. Baudin, P. Boumier, Y. Elsworth, R.A. García, B.N. Andersen, W. Finsterle, C. Fröhlich, A. Gabriel, G. Grec, A. Jiménez, A. Kosovichev, T. Sekii, T. Toutain, S. Turck-Chièze, The quest for the solar G modes. Astron. Astrophys. Rev. 18, 197–277 (2010). doi: 10.1007/s00159-009-0027-z 3. Astronomical Society of the Pacific Conference Series;M. Asplund,2005 4. M. Asplund, N. Grevesse, A.J. Sauval, C. Allende Prieto, D. Kiselman, Line formation in solar granulation. IV. [O I], O I and OH lines and the photospheric O abundance. Astron. Astrophys. 417, 751–768 (2004). doi: 10.1051/0004-6361:20034328 5. M. Asplund, N. Grevesse, A.J. Sauval, P. Scott, The chemical composition of the Sun. Annu. Rev. Astron. Astrophys. 47, 481–522 (2009). doi: 10.1146/annurev.astro.46.060407.145222
|
|