Abstract
Using the variability of solar acoustic oscillation mode frequencies, we investigate the width and timing of last three solar minima at various depths in the solar interior. We find that the current minimum is as deep as the previous minimum, however, more data are needed to reveal the true depth of the current minimum.
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References
Jain, K., Tripathy, S. C., & Hill, F. (2011). How peculiar was the recent extended minimum: A hint toward double minima. The Astrophysical Journal, 739, 6. https://doi.org/10.1088/0004-637X/739/1/6, arXiv:1107.0049.
Jain, K., Tripathy, S., Komm, R., Hill, F., & Simoniello, R. (2018). 22 Year solar magnetic cycle and its relation to convection zone dynamics. In D. Banerjee, J. Jiang, K. Kusano, & S. Solanki (Eds.). IAU Symposium (Vol. 340, pp. 9–10). https://doi.org/10.1017/S1743921318001242, arXiv:1805.05371.
Acknowledgements
This work utilizes GONG data from NSO, which is operated by AURA under a cooperative agreement with NSF.
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Jain, K., Tripathy, S.C., Hill, F. (2020). Comparing Solar Activity Minima Using Acoustic Oscillation Frequencies. In: Monteiro, M.J.P.F.G., GarcÃa, R.A., Christensen-Dalsgaard, J., McIntosh, S.W. (eds) Dynamics of the Sun and Stars. Astrophysics and Space Science Proceedings, vol 57. Springer, Cham. https://doi.org/10.1007/978-3-030-55336-4_19
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DOI: https://doi.org/10.1007/978-3-030-55336-4_19
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