Abstract
We characterize the spatio-temporal power distribution around the active region 12683 as a function of height in the solar atmosphere, wave frequencies, magnetic field strength and inclination of the magnetic field.
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References
Schunker, H., & Braun, D. C. (2011). Newly identified properties of surface acoustic power. Solar Physics, 268, 349–362. https://doi.org/10.1007/s11207-010-9550-3
Tripathy, S. C., Jain, K., Kholikov, S., Hill, F., Rajaguru, S. P., & Cally, P. S. (2018). A study of acoustic halos in active region NOAA 11330 using multi-height SDO observations. Advances in Space Research, 61(2), 691–704. https://doi.org/10.1016/j.asr.2017.10.033
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SDO data courtesy of SDO (NASA) and the HMI and AIA consortium.
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Tripathy, S.C., Jain, K., Kholikov, S., Hill, F., Cally, P. (2020). Study of Acoustic Halos in NOAA Active Region 12683. 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_13
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DOI: https://doi.org/10.1007/978-3-030-55336-4_13
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