On comparing estimates of low-$\textit{l}$ solar p-mode frequencies from Sun-as-a-star and resolved observations

Author:

Chaplin W. J.,Appourchaux T.,Elsworth Y.,Isaak G. R.,Miller B. A.,New R.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference25 articles.

1. Solar-cycle variation of the sound-speed asphericity from GONG and MDI data 1995-2000

2. Appourchaux, T., Anderson, B., & Sekii, T. 2002, in SOHO 11 Symp. from Solar Min to Max: Half a Solar Cycle with SOHO, ed. C. Fröhlich, & A. Wilson, ESA SP-508, 47

3. Solar internal sound speed as inferred from combined BiSON and LOWL oscillation frequencies

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1. They do change after all: 25 yr of GONG data reveal variation of p-mode energy supply rates;Monthly Notices of the Royal Astronomical Society;2020-10-22

2. The solar benchmark: rotational modulation of the Sun reconstructed from archival sunspot records;Monthly Notices of the Royal Astronomical Society;2019-01-18

3. The Sun’s Interior Structure and Dynamics, and the Solar Cycle;Space Science Reviews;2014-10-01

4. Quasi-biennial variations in helioseismic frequencies: can the source of the variation be localized?;Monthly Notices of the Royal Astronomical Society;2011-12-01

5. Frequency Separation Variations of the Solar Low-Degree p-Modes;Publications of the Astronomical Society of Japan;2009-12-25

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