Detecting deep axisymmetric toroidal magnetic fields in stars: The traditional approximation of rotation for differentially rotating deep spherical shells with a general azimuthal magnetic field

Thumbnail
Fulltext:
250427.pdf
Size:
4.772Mb
Format:
PDF
Description:
Publisher’s version
Download
Publication year
2022
Author(s)
Dhouib, H.
Mathis, S.
Bugnet, L.
Reeth, T. Van
Aerts, C.
Source
Astronomy & Astrophysics, 661, (2022), pp. 1-21, article A133
ISSN
DOI
Publication type
Article / Letter to editor
Please use this identifier to cite or link to this item: https://hdl.handle.net/2066/250427   https://hdl.handle.net/2066/250427
Display more details

Upload full text

Use your RU credentials (u/z-number and password) to log in with SURFconext to upload a file for processing by the repository team.