The energy budget of stellar magnetic fields: comparing non-potential simulations and observations

Lehmann, L. T. and Jardine, M. M. and Vidotto, A. A. and Mackay, D. H. and See, V. and Donati, J.-F. and Folsom, C. P. and Jeffers, S. V. and Marsden, S. C. and Morin, J. and Petit, P. (2017) The energy budget of stellar magnetic fields: comparing non-potential simulations and observations. Monthly Notices of the Royal Astronomical Society: Letters, 466 (1). L24-L28. ISSN 0035-8711

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Abstract

The magnetic geometry of the surface magnetic fields of more than 55 cool stars have now been mapped using spectropolarimetry. In order to better understand these observations, we compare the magnetic field topology at different surface scale sizes of observed and simulated cool stars. For ease of comparison between the high-resolution non-potential magnetofrictional simulations and the relatively low-resolution observations, we filter out the small-scale field in the simulations using a spherical harmonics decomposition. We show that the large-scale field topologies of the solar-based simulations produce values of poloidal/toroidal fields and fractions of energy in axisymmetric modes which are similar to the observations. These global non-potential evolution model simulations capture key magnetic features of the observed solar-like stars through the processes of surface flux transport and magnetic flux emergence. They do not, however, reproduce the magnetic field of M-dwarfs or stars with dominantly toroidal field. Furthermore, we analyse the magnetic field topologies of individual spherical harmonics for the simulations and discover that the dipole is predominately poloidal, while the quadrupole shows the highest fraction of toroidal fields. Magnetic field structures smaller than a quadrupole display a fixed ratio between the poloidal and toroidal magnetic energies.


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Item Type: Article (Commonwealth Reporting Category C)
Refereed: Yes
Item Status: Live Archive
Additional Information: Access to Published version in accordance with the copyright policy of the publisher.
Faculty / Department / School: Current - Faculty of Health, Engineering and Sciences - School of Agricultural, Computational and Environmental Sciences
Date Deposited: 21 Jan 2018 23:42
Last Modified: 22 Jan 2018 00:17
Uncontrolled Keywords: stars, magnetic fields, solar-type
Fields of Research : 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
Socio-Economic Objective: E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
Identification Number or DOI: 10.1093/mnrasl/slw225
URI: http://eprints.usq.edu.au/id/eprint/33569

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