Corrections of Sun-as-a-star p-mode frequencies for effects of the solar cycle
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/200912286/pdf
Reference14 articles.
1. On understanding the meaning of l = 2 and 3 p-mode frequencies as measured by various helioseismic instruments
2. Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations
3. Variations in the excitation and damping of low- solar p modes over the solar activity cycle
4. On comparing estimates of low-$\textit{l}$ solar p-mode frequencies from Sun-as-a-star and resolved observations
5. Solar p-mode frequencies at $\mathsf{\ell=2}$: What do analyses of unresolved observations actually measure?
Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Seismic Signatures of Solar and Stellar Magnetic Activity;Astrophysics and Space Science Proceedings;2020
2. NGC 6819: testing the asteroseismic mass scale, mass loss and evidence for products of non-standard evolution;Monthly Notices of the Royal Astronomical Society;2017-07-28
3. Low-frequency, low-degree solar p-mode properties from 22 years of Birmingham Solar Oscillations Network data;Monthly Notices of the Royal Astronomical Society;2014-02-07
4. Solar-cycle variations of large frequency separations of acoustic modes: implications for asteroseismology;Monthly Notices of the Royal Astronomical Society;2011-03-25
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