Abstract
We investigate the variation of high-degree mode frequencies as a local response to the active regions in two different phases of the solar activity cycle. We find that the correlation between frequency shifts and the surface magnetic activity measured locally are significantly different during the two activity periods.
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Jain, K., Tripathy, S. C., Hill, F., ApJ, in press
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Tripathy, S.C., Jain, K., Hill, F. (2010). Do Active Regions Modify Oscillation Frequencies?. In: Hasan, S., Rutten, R. (eds) Magnetic Coupling between the Interior and Atmosphere of the Sun. Astrophysics and Space Science Proceedings. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-02859-5_34
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DOI: https://doi.org/10.1007/978-3-642-02859-5_34
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