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The Norwegian University of Science and Technology (NTNU) has developed advanced instrumentation for studying gravity waves and momentum flux in the atmosphere. Featuring a 30 kW SkiyMet system, this setup operates near 35 MHz, allowing for high-accuracy measurements of horizontal winds, temperatures, and polar mesospheric clouds (PMC). Enhanced transmitter arrays enable precise beam forming for gravity wave momentum flux determination. Additionally, low-light-level all-sky imagers and specialized optical filters facilitate comprehensive observations of airglow and auroral structures, with potential for collaborative studies across radar systems.
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New Instrumentation at NTNU P. J. Espy and R. E. Hibbins Norwegian University of Science and Technology Trondheim, Norway Background Picture from D. Fritts
Meteor Radar with Momentum Flux Capabilities • 30 kW SkiyMet system operating near 35 MHz • Standard horizontal winds, temperatures and PMC • Enhanced transmitter array to allow beam forming • Allows gravity wave momentum flux determination
Low-Light-Level All Sky Imager + OH Spectrometer • TE-cooledCCD camera • All sky optics • Filter wheel • Filters: • OH 720-910 nm with O2 notch @ 865 nm • Na 589 nm, 0.2 nm FWHM • N2+ 1NG 428 nm, 2 nm FWHM • OI 630 nm, 2 nm FWHM • H 485.8 nm, 1.6 nm FWHM • 1 Guest Investigator filter. • OH Spectrometer 1500-1700 nm, 2nm res.
22 Feb 2011 OH Temperatures
Possible Collaborative Studies: Imager • Triangulation of airglow structures for 3-D studies • Triangulation of auroral structures for 3-D studies • Proton content of aurora over and equatorward of Andøya • Characteristic energy of precipitating electrons in aurora over and equatorward of Andøya • Comparison of optical vs. radar momentum flux observation • Validation of new tool for momentum flux observations at Andøya
Possible Collaborative Studies: Radar • Current radars (Andøya, NTNU, Kiruna) affected by orographic, auroral and polar vortex shear zone sources. • Andøya vs Kiruna radar • Same sides of the polar vortex and auroral oval, but different sides of the mountains. • NTNU vs Andøya radar • On same side of the mountains but opposite sides of polar vortex and auroral oval • NTNU vs Kiruna radar • Different sides of the mountains, polar vortex and auroral oval • Comparing this triad as a function of polar vortex, auroral and ground-level wind strength and orientation will allow the different sources to be quantified. • Use correlation of NTNU-Andøya-Kiruna radars to extend the climatology of gravity waves to horizontal scales beyond 200 km.