2018/02/28 by Shravan Hanasoge
Computer Science · Physics and Astronomy · #Component (thermodynamics) #Coupling (piping) #Harmonics #Helioseismology #Noise (video) #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #Spherical harmonics #Stellar, planetary, and galactic studies #Visibility #astro-ph.SR
paper · pdf · doi:10.3847/1538-4357/aac3e3
23 pages, 11 figures, ApJ
openalex created_date 2018/02/23 · arxiv created 2018/05/09 · openalex publication_date 2018/06/29 · arxiv updated 2018/07/18 · openalex updated_date 2026/08/05
Abstract Normal modes are coupled by the presence of perturbations in the Sun, providing a novel and underappreciated helioseismic technique with which to image the solar interior. The process of measuring coupling between normal modes is straightforward, much more so when compared with other prevalent helioseismic techniques. The theoretical framework to interpret these measurements is well developed with the caveat that it applies only in the case where the entire surface of the Sun is observed. In practice, however, the limited visibility of the Sun and line-of-sight-related effects diminish the resolution of the technique. Here, we compute realistic sensitivities of normal-mode coupling measurements to flows in the solar interior and describe how to mitigate the sometimes-overwhelming effect of leakage. The importance of being able to isolate individual spherical harmonics and observe the full Sun, to which future solar observatories may aspire, is thus highlighted in our results. In the latter part of the article, we describe the noise model for the variance of coupling coefficients, a critical component to the process of inference.