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EEV and Electron Corp. Virtual Phase CCDs in the Near IR Region, He I λ 10830 Å
Published online by Cambridge University Press: 07 August 2017
Extract
He I, λ 10830 å observations of late-type stars provide valuable information about the chromospheric and low chromospheric-coronal transition regions. High resolution measurements of the helium λ 10830 å line profile offer a convenient way to survey the coronal emission of the Sun as a point source, as well as a variety of stars (O'Brien and Lambert, 1986, Shcherbakov and Shcherbakova, 1991).
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- Section II — Poster Papers
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- Copyright © Kluwer 1995