Abstract
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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Berezin, V. Yu., Zuev, A. G, Kiryan, G. V., Rybakov, M. I., Hvilivitsky, A. G., Ilyin, I. V., Petrov, P. P., Savanov, I. S. and Shcherbakov, A. G. 1991 Letters to Soviet AJ 17, 953
O’Brien, Jr. and Lambert, D. 1986 ApJS 62, 899
Shcherbakov, A. G. and Shcherbakova, Z. A. 1991 IAU Colloquium No. 130, The Sun and Cool Stars: Activity, Magnetism, Dynamos, I. Tuominen, D. Moss and G. Rudiger, eds., Lecture Notes in Physics, Springer, p. 252
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© 1995 Springer Science+Business Media Dordrecht
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Shcherbakov, A.G., Shcherbakova, Z.A., Ilyin, I., Tuominen, I. (1995). EEV and Electron Corp. Virtual Phase CCDs in the Near IR Region, He I λ 10830 Å. In: Philip, A.G.D., Janes, K.A., Upgren, A.R. (eds) New Developments in Array Technology and Applications. International Astronomical Union / Union Astronomique Internationale, vol 167. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0383-1_64
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DOI: https://doi.org/10.1007/978-94-011-0383-1_64
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