CALCULATION OF RAMAN SHIFT IN VACUUM

被引：11

作者：

STREY, G

机构：

[1] Department of Physics, University of Munich

来源：

SPECTROCHIMICA ACTA PART A-MOLECULAR SPECTROSCOPY | 1969年 / A 25卷 / 01期

关键词：

D O I：

10.1016/0584-8539(69)80182-0

中图分类号：

O433 [光谱学];

学科分类号：

0703 ; 070302 ;

摘要：

A correction table, similar to that of Opler [1], is given to simplify conversion of the wavelengths of Raman lines observed as angstroms (in air) to wave numbers (in vacuum). A more elaborate table for direct conversion is described for some exciting lines of helium arc, helium-neon, argon+, and ruby lasers in addition to the common mercury lines. The computational program was based on the dispersion formula of Edlén [2]. © 1969.

引用

页码：163 / &

共 12 条

[1]

BARRELL H, 1939, T ROY SOC A, V238, P1

[2]

COLEMAN CD, 1960, 3 NAT BUR STAND MON

[3] THE DISPERSION OF STANDARD AIR [J].

EDLEN, B .

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA, 1953, 43 (05) :339-344

[4]

HARRISON GR, 1952, MIT WAVELENGTH TABLE

[5] WAVE-LENGTHS OF MERCURY 198 [J].

MEGGERS, WF ;

KESSLER, KG .

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA, 1950, 40 (11) :737-741

[6]

MEGGERS WF, 1918, BS SCI PAP, V14, P724

[7]

Minnhagen L., 1963, ARK FYS, V25, P203

[8]

OPLER A, 1951, J OPT SOC AM, V41, P349, DOI 10.1364/JOSA.41.000349

[9]

RANK DH, 1959, ADV SPECTROSC, V1, P76

[10]

ROSS D, 1966, LASER LICHTVERSTARKE

← 1 2 →