Skew-symmetric solar p modes in low-l BiSON data
Authors:
- W. J. ChaplinWCW. J. Chaplin
- Y. ElsworthYEY. Elsworth
- G. R. IsaakGIG. R. Isaak
- B. A. MillerBMB. A. Miller
- R. NewRNR. New
- 19 September 1999
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 308 (2) , 424-430
Abstract
No abstract availableThis publication has 16 references indexed in Scilit:
- Line Asymmetry of Solarp‐Modes: Properties of Acoustic SourcesThe Astrophysical Journal, 1999
- Line Asymmetry of Solarp‐Modes: Reversal of Asymmetry in Intensity Power SpectraThe Astrophysical Journal, 1999
- An analysis of solar p-mode frequencies extracted from BiSONdata: 1991-1996Monthly Notices of the Royal Astronomical Society, 1998
- The Solar Core: New Low-[CLC][ITAL]l p[/ITAL][/CLC]-Mode Fine-Spacing Results from B[CLC]i[/CLC]SONThe Astrophysical Journal, 1997
- Asymmetries of Solarp‐Mode Line ProfilesThe Astrophysical Journal, 1996
- The Current State of Solar ModelingScience, 1996
- Asymmetries of solar oscillation line profilesThe Astrophysical Journal, 1993
- Effects of diffusion on solar models and their oscillation frequenciesThe Astrophysical Journal, 1993
- Evidence from solar seismology against non-standard solar-core modelsNature, 1990
- The effect of rotation on whole-disc Doppler observations of solar oscillationsMonthly Notices of the Royal Astronomical Society, 1989