WATER ON THE SUN

被引：108

作者：

WALLACE, L

BERNATH, P

LIVINGSTON, W

HINKLE, K

BUSLER, J

GUO, BJ

ZHANG, KQ

机构：

[1] UNIV WATERLOO, DEPT CHEM, WATERLOO, ON N2L 3G1, CANADA

[2] KITT PEAK NATL OBSERV, NATL OPT ASTRON OBSERV, TUCSON, AZ 85726 USA

[3] UNIV ARIZONA, DEPT CHEM, TUCSON, AZ 85721 USA

[4] NATL OPT ASTRON OBSERV, NATL SOLAR OBSERV, TUCSON, AZ 85726 USA

[5] UNIV WATERLOO, DEPT CHEM, WATERLOO, ON N2L 3G1, CANADA

来源：

SCIENCE | 1995年 / 268卷 / 5214期

关键词：

D O I：

10.1126/science.7761830

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

High-resolution infrared spectra of sunspot umbrae have been recorded with the 1-meter Fourier transform spectrometer on Kitt Peak. The spectra contain a very large number of water absorption features originating on the sun. These lines have been assigned to the pure rotation and the vibration-rotation transitions of hot water by comparison with high-temperature laboratory emission spectra.

引用

页码：1155 / 1158

页数：4

共 28 条

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