November 13, 2008
Satellite Successfully Observes Polar Mesospheric Clouds
The Naval Research Laboratory's Spatial Heterodyne Imager for Mesospheric Radicals (SHIMMER) has successfully observed a second northern season of Polar Mesospheric Clouds (PMCs), which are the Earth's highest clouds. This successful observation fulfills the primary goal of the Space Test Program Satellite-1 (STPSat-1) Extended Mission.
SHIMMER was originally launched as the primary payload of STPSat-1 on March 8, 2007, with the objective to demonstrate the novel optical technique of Spatial Heterodyne Spectroscopy and to obtain global measurements of the hydroxyl (OH) radical in the Earth's mesosphere (50-90 km altitude). After the successful completion of its nominal 1-year mission, STPSat-1 operations were transitioned to NRL, which has been operating the spacecraft since June 1, 2008 using a novel, low cost operations approach.
SHIMMER has now measured the PMC diurnal variation for the two northern seasons of 2007 and 2008, and surprisingly, the variation is quite different. Even though a semidiurnal signature, that is two peaks per day -- one in early morning and one in the late afternoon -- was observed in 2007; in 2008, the variation was diurnal or one peak per day (see figure). This result has important implications for the inference of long-term trends from historical, space-based PMC observations because NASA and NOAA satellites that have observed PMCs over the last 25 years have all been launched into sun-synchronous orbits with different, fixed local times. Until the diurnal variation of these clouds is better understood, the SHIMMER data show that it is premature to make firm conclusions about multi-decadal trends in PMCs.
SHIMMER is a compact, rugged, high-resolution ultraviolet spectrometer designed to image the Earth's atmosphere. It is the first satellite-based instrument to use the spatial heterodyne spectroscopy (SHS) technique, which significantly reduces the instrument's size and weight while retaining the spectral resolution and exceeding the sensitivity of comparable conventional instrumentation. The heart of SHIMMER is a monolithic interferometer, which allows SHIMMER to simultaneously observe the OH solar resonance fluorescence from 32 altitudes at a superior resolving power of 25,000. NRL's Space Science Division developed SHIMMER in cooperation with St. Cloud State University and the University of Wisconsin. NASA's Planetary Instrument Definition and Development Program supported the development of the monolithic interferometer.
Image 1: Polar mesospheric cloud over Lake Saimaa. Courtesy Mika Yrjölä - Wikipedia
Image 2: STPSat-1 (NRL)
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