Physics
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsa21a0233h&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SA21A-0233
Physics
0310 Airglow And Aurora, 3379 Turbulence (4490), 3384 Acoustic-Gravity Waves
Scientific paper
Small scale (less than 15 km horizontal wavelength) wavelike structures, known as ripples are a common occurrence in OH airglow images. Recent case studies attribute their origin to the presence of either convective or dynamical instabilities. However, little is known about their frequency of occurrence and characteristics such as period and wavelength. The Maui-MALT Observatory, located on Mt. Haleakala is instrumented with a Na wind/temperature lidar which allows the determination of whether the atmosphere is dynamically or convectively unstable, and a fast OH airglow camera which takes images every 3 seconds with a sensitivity high enough to see the ripples. This study reports on two months of observations in October/November 2003 and August 2004, 8 nights of which also included Na lidar measurements. The nominal observed period for the ripples is between 2 and 4 minutes. The results suggest that instability features occur in the 85 to 90 km region of the atmosphere around 20 percent of the time. While there are clear night to night variations the average is similar for both the 2003 and 2004 observations. In addition a few of the small-scale structures are not ripples caused by instabilities, but rather are short horizontal wavelength evanescent waves. Their fractional intensity fluctuations are as large or larger than those of the ripple instabilities. Unlike the instabilities, the origin of the evanescent waves is not determined.
Franke Steven J.
Hecht James H.
Liu Alan Z.
Pautet P.
Rudy Richard J.
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