Sun's Seismic Radius as Measured from the Fundamental Modes of Oscillations and its Implications for the TSI Variations
| Autor: | Jain, Kiran, Tripathy, S. C., Hill, F. |
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| Rok vydání: | 2018 |
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| Druh dokumentu: | Working Paper |
| DOI: | 10.3847/2041-8213/aac327 |
| Popis: | In this letter, we explore the relationship between the solar seismic radius and total solar irradiance (TSI) during last two solar cycles using the uninterrupted data from space-borne instruments onboard {\it SoHO} and {\it SDO}. The seismic radius is calculated from the fundamental ({\it f}) modes of solar oscillations utilizing the observations from {\it SoHO}/MDI and {\it SDO}/HMI, and the total solar irradiance measurements are obtained from {\it SoHO}/VIRGO. Our study suggests that the major contribution to the TSI variation arises from the changes in magnetic field while the radius variation plays a secondary role. We find that the solar irradiance increases with decreasing seismic radius, however the anti-correlation between them is moderately weak. The estimated maximum change in seismic radius during a solar cycle is about 5 kilometers, and is consistent in both solar cycles 23 and 24. Previous studies suggest a radius change at the surface of the order of 0.06 arcsecond to explain the 0.1\% variation in the TSI values during the solar cycle, however our inferred seismic radius change is significantly smaller, hence the TSI variations can not be fully explained by the temporal changes in seismic radius. Comment: Accepted for publication in The Astrophysical Journal Letters, includes 5 figures |
| Databáze: | arXiv |
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