Using laboratory spectroscopy to identify lines in the K- and L-band spectrum of water in a sunspot

被引：32

作者：

Zobov, NF

Polyansky, OL

Tennyson, J

Shirin, SV

Nassar, R

Hirao, T

Imajo, T

Bernath, PF

Wallace, L

机构：

[1] UCL, Dept Phys & Astron, London WC1E 6BT, England

[2] Nizhnii Novgorod State Univ, Dept Math, Nizhnii Novgorod, Russia

[3] Univ Waterloo, Dept Chem, Waterloo, ON N2L 3G1, Canada

[4] Univ Waterloo, Dept Phys, Waterloo, ON N2L 3G1, Canada

[5] Natl Opt Astron Observ, Tucson, AZ 85732 USA

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 530卷 / 02期

关键词：

molecular data; sunspots; infrared : solar system; infrared : stars;

D O I：

10.1086/308419

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The infrared spectrum of a sunspot is analyzed in the L-band region 3.1-4.0 mu m (2497-3195 cm(-1)) and 2.02-2.35 mu m (4251-4962 cm(-1)) in the K band. A new laboratory emission spectrum covering 2500-6000 cm(-1) is analyzed to help make the assignments. Quantum number assignments are made using linelists computed using variational calculations, assisted by tabulations of experimental energy levels. There are 1207 new H(2)(16)O lines assigned in the L band and 508 new lines in the K band. Vibrational band origins of 11242.8 +/- 0.1 cm(-1) and 12586 +/- 1 cm(-1) are obtained for the (051) and (061) states.

引用

页码：994 / 998

页数：5

共 28 条

[1] THE INFLUENCE OF H2O LINE BLANKETING ON THE SPECTRA OF COOL DWARF STARS [J].