Wavelet analysis of the long-term activity of V833 Tau
R. Stepanov, N.I. Bondar', M.M. Katsova, D. Sokoloff, P. Frick

TL;DR
This study applies wavelet analysis to over a century of photometric data of V833 Tau to distinguish true stellar activity cycles from stochastic variations, suggesting a possible century-long cycle consistent with stellar dynamo theory.
Contribution
It introduces a wavelet-based method for analyzing long-term stellar activity records, improving the identification of genuine activity cycles.
Findings
V833 Tau shows variations on 2-50 year timescales similar to solar mid-term variations.
The star's true activity cycle, if present, may be around a century or longer.
Results support the consistency of long-term stellar activity with dynamo theory.
Abstract
The bulk of available stellar activity observations is frequently checked for the manifestation of signs in comparison with the known characteristic of solar magnetic modulation. The problem is that stellar activity records are usually an order of magnitude shorter than available observations of solar activity variation. Therefore, the resolved time scales of stellar activity are insufficient to decide reliably that a cyclic variation for a particular star is similar to the well-known 11-yr sunspot cycles. As a result, recent studies report several stars with double or multiple cycles which serve to challenge the underlying theoretical understanding. This is why a consistent method to separate 'true' cycles from stochastic variations is required. In this paper, we suggest that a conservative method, based on the best practice of wavelet analysis previously applied to the study of solar…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
