## Abstract Large solar telescopes built at places with a quite excellent seeing, equipped with a sophisticated optics and control system are too expensive and unique to be used currently in hunting of sudden and short‐lasting activity events, e.g. flares and eruptive prominences. For a systematic
✦ LIBER ✦
Hydrogen Hα line emission and radiative losses in the impulsive solar events
✍ Scribed by V.A Kobylinskii; V.V Zharkova
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 557 KB
- Volume
- 17
- Category
- Article
- ISSN
- 0273-1177
No coin nor oath required. For personal study only.
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## Abstract From measurements of the __H__~α~ and __H__~β~ spectral line profiles in a plasma, a method is developed which allows to separate the contributions of Doppler and Stark broadening. This method is superior to the deconvolution of Voigt profiles, in particular, when the lines are of low i