๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Voltage-intensity relations of 29 lines of the mercury spectrum

โœ Scribed by Paul B. Taylor

Publisher
Elsevier Science
Year
1929
Tongue
English
Weight
457 KB
Volume
207
Category
Article
ISSN
0016-0032

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Relations of intensity in the sodium lin
Relations of intensity in the sodium lines
โœ C. ๐Ÿ“‚ Article ๐Ÿ“… 1881 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 57 KB

Phosphor-Tin.--An allov of tin with phosphorus is much used in (~erlnanv, especially in tile l)reparation of phosphor-bronze. The mixture should contain at least 9 per cent. of phosphoru~ ill order to secure a thorough incorporation of the tin. If more than 9 per cent. is introduced the excess oxidi

The Far Infrared Spectrum of HOCl: Line
The Far Infrared Spectrum of HOCl: Line Positions and Intensities
โœ J.-M. Flaud; M. Birk; G. Wagner; J. Orphal; S. Klee; W.J. Lafferty ๐Ÿ“‚ Article ๐Ÿ“… 1998 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 161 KB

The far infrared spectrum of HOCl has been recorded at high resolution between 20 and 360 cm ฯช1 by means of Fourier transform spectroscopy, and it was possible to observe pure rotation lines involving rotational levels with high K a quantum numbers (up to K a ฯญ 9). These lines combined with microwav

The relative intensities of CI lines in
The relative intensities of CI lines in the solar EUV spectrum
โœ Carole Jordan ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 447 KB

The relative intensity of two CI lines at 1993.6 โ€ข and 1657.4 A, observed in the limb spectrum of the sun, is a factor 2.6 โ€ข 10 a larger than that expected if both lines were optically thin. It is shown that the observed intensity ratio may be explained in terms of the transfer of photons from 2 165