What causes p-mode asymmetry reversal?

Astrophysical Journal

Volumn 596, Issue 1 I, 2003, Pages 698-701

  Georgobiani, Dali ^a   Stein, Robert F ^a   Nordlund, Åke ^b  

^a MICHIGAN STATE UNIVERSITY   (United States)

^b THEORETICAL ASTROPHYSICS CENTER   (Denmark)

Author keywords

Convection; Methods: numerical; Radiative transfer; Sun: helioseismology; Sun: oscillations

Indexed keywords

EID: 0142229972     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/377683     Document Type: Article

References (10)

1. Duvall, T. L., Jr., Jefferies, S. M., Harvey, J. W., Osaki, Y., & Pomerantz, M. A. 1993, ApJ, 410, 829
2. Georgobiani, D., Kosoviehev, A. G., Nigam, R., Nordlund, Å., & Stein, R.F. 2000a, ApJ, 530, L139
3. Georgobiani, D., Stein, R. F., & Nordlund, Å. 2000b, in Proc. SOHO 10/GONG 2000 Workshop, Helio- & Asteroseismology at the Dawn of the Millennium, ed. A. Wilson (Tenerife: Esa SP-464), 583
4. Kumar, P., & Basu, S. 1999, ApJ, 519, 389
5. Nigam, R., Kosovichev, A. G., Scherrer, P. H., & Schou, J. 1998, ApJ, 495, L115
6. Nordlund, Å, 1982, A&A, 107, 1
7. Nordlund, Å., & Stein, R. F. 1990, Comput. Phys. Commun., 59, 119
8. -. 1991, in Stellar Atmospheres - Beyond Classical Models, ed. I. Hubeny, D. G. Hummer, & L. Crivellari (NATO ASI Ser. C, 341; Dordrecht: Kluwer), 263
9. Roxburgh, I. W., & Vorontsov, S. V. 1997, MNRAS, 292, L33
10. Stein, R. F., & Nordlund, A. 1998, ApJ, 499, 914