Publication Year
2024
Abstract
In this paper, we investigate the correlations between a star's internal dynamics due to the Rayleigh-Taylor instability and episodes of stellar wind activity, using both a theoretical model and observational data from the NOAA.% \cite{NOAA}. Besides its relevance as an astrophysics problem, this study is also informative for models of climate change which include secular perturbations in the Sun's internal dynamics, as a potential source of solar activity variability.
Recommended Citation
Klett, Fiona
(2024)
"A study on the correlation between a star's Rayleigh-Taylor characteristic timescale and stellar wind activity,"
Undergraduate Journal of Mathematical Modeling: One + Two:
Vol. 13:
Iss.
1, Article 1.
Available at:
https://digitalcommons.usf.edu/ujmm/vol13/iss1/1
Creative Commons License
This work is licensed under a Creative Commons Attribution-Noncommercial-Share Alike 4.0 License.
Included in
Advisors:
Razvan Teodorescu, Mathematics and Statistics