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Chromospheric and Coronal Indicators of Stellar Magnetic Structure
Published online by Cambridge University Press: 04 August 2017
Extract
This paper discusses attempts to derive information on magnetic structure in late-type stars, only from emission fluxes in the cores of the Ca II H and K lines, in UV emission lines and in soft X-rays — and from relations between these emission fluxes. However simpleminded and indirect this approach may seem, it brings out stimulating results. Studies of this kind are guided by solar research, so let us look first at the solar data.
- Type
- I. Magnetic Fields in Stellar Photospheres
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- Copyright © Reidel 1983
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