Wavelengths of clean atmospheric water lines, and some solar lines, in the wavelength interval 10750 A to 10900 A have been measured to an accuracy approaching ~ 1 m/~. Strengths and wavelengths have been measured for all atmospheric water lines with absorption coefficients > 5 • 10 -4 cm -a gm -1 c
Spectrum intensity designation in the vicinity of Fe 3100 Å
✍ Scribed by R. Gerharz
- Publisher
- Elsevier Science
- Year
- 1964
- Weight
- 255 KB
- Volume
- 20
- Category
- Article
- ISSN
- 0371-1951
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
The results of measurements of absolute intensities in the spectrum of the centre of the sun's disk in the wavelength region 2977-4087/~ have already been published (Houtgast 1965(Houtgast , 1968) and use has been made of them on different occasions. The intensities at 206 spectral points have been
High resolution profiles of the Mg xn 8.42 A line in the solar X-ray spectrum were recorded from the Intercosmos 7 satellite. The Mg xaI line intensity provides a sensitive indicator of the hot plasma content (T > 3 • 106K) in coronal condensations and X-ray flare volumes. The ratio of the line inte
Divergence between determinations of the iron abundance from permitted Fe lines and forbidden FeII lines is discussed and a re-examination of the equivalent widths of two of the [Fen] lines is proposed.