Atmospheric gravity wave signatures in the infrared hydroxyl OH airglow

被引:23
作者
Frey, HU [1 ]
Mende, SB
Arens, JF
McCullough, PR
Swenson, GR
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Univ Illinois, Urbana, IL 61801 USA
关键词
D O I
10.1029/1999GL010695
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Atmospheric gravity wave induced airglow fluctuations of the hydroxyl OH Meinel and other bands are: routinely observed using CCD imagers operating in the near infrared wavelength region. Farther into the infrared, the intensity of the OH emissions is much greater. Recently, a new IR imaging camera was modified for infrared viewing of the night sky with approximately 1 steradian field of view. The filter had a center wavelength of 1467 nm and a bandwidth of 177 nm to include components of the OH (Delta v = 2) band. The images show good signal-to-noise ratios of 180 with 10 second:exposures. Cross-spectral and wavelet analysis:were used to obtain spatial and temporal information about observed airglow fluctuations, and horizontal wavelengths and wave periods as short as 3.7 km and 3 min, respectively, were determined.
引用
收藏
页码:41 / 44
页数:4
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