Observations of X-ray emission — a diagnostic tool for the mechanisms driving stellar magnetic fields — from four cool stars call into question accepted models of magnetic-field generation in the Sun and stars. See Letter p.526
Notes
References
Wright, N. J. & Drake, J. J. Nature 535, 526–528 (2016).
Hathaway, D. H. Living Rev. Sol. Phys. 7, 1 (2010).
Noyes, R. W., Hartmann, L. W., Baliunas, S. L., Duncan, D. K. & Vaughan, A. H. Astrophys. J. 279, 763–777 (1984).
Fan, Y. Living Rev. Sol. Phys. 6, 4 (2009).
Cheung, M. C. M., Rempel, M., Title, A. M. & Schüssler, M. Astrophys. J. 720, 233–244 (2010).
Charbonneau, P. Annu. Rev. Astron. Astrophys. 52, 251–290 (2014).
Hotta, H., Rempel, M. & Tokoyama, T. Science 351, 1427–1430 (2016).
Nelson, N. J., Brown, B. P., Sacha Brun, A., Miesch, M. S. & Toomre, J. Astrophys. J. 739, L38 (2011).
Fan, Y. & Fang, F. Astrophys. J. 789, 35 (2014).
Author information
Authors and Affiliations
Corresponding author
Related links
Rights and permissions
About this article
Cite this article
Charbonneau, P. Dynamo theory questioned. Nature 535, 500–501 (2016). https://doi.org/10.1038/535500a
Published:
Issue Date:
DOI: https://doi.org/10.1038/535500a
- Springer Nature Limited
This article is cited by
-
Critical Science Plan for the Daniel K. Inouye Solar Telescope (DKIST)
Solar Physics (2021)