Resonance develops a two-dimensional imaging correlation spectrometer for plume flux measurements using the DOAS technique.

Resonance develops the charge control system for the Stanford University, ESA and JPL’s LISA Pathfinder (GRS project technology test for the Laser Interferometer Space Antenna (LISA).

Resonance and McGill University Test the Resonance Mini Doas I (RMDI) Differential Optical Absorption Spectrometer at Mt. Etna, Stroboli, Kudryavy Volcanoes.

MicroMAPS flown on the Scaled Composites Proteus High Altitude Aircraft and has retrieved CO Data over North America and Europe for NASA Langley Research Center and Virginia Space Grant Consortium.

Resonance’s WINDO 5 measures Atomic Oxygen and Gravity Waves in the upper Atmosphere (WAVE2004).

Resonance further develops its IR based natural gas remote sensor and performs field tests on gas service leaks.

Resonance develops and delivers a digital COSPEC to JMA.

Resonance and McGill University test the Resonance Mini DOAS I (RMDI) Differential Optical Absorption Spectrometer at Tarumae Volcano in Hokaido Japan.

Resonance develops a miniaturized photoionization bulb for the detection of atmospheric trace constituents.

Resonance’s VUV and UV Lamps are used to measure atmospheric and particulate species in middle atmosphere by VUV induced photo-ionization.

Resonance develops the digital COSPEC.

Resonance’s WINDO 4 measures Atomic Oxygen and Gravity Waves in the upper Atmosphere (WAVE2000) for University of Tokyo.

Resonance wins technology fund bid to develop a gas correlation remote sensor for Natural Gas.

Resonance develops a VUV Atomic Oxygen Absorption System for YBO superconductor research.

Resonance develops a VUV Atomic Nitrogen Absorption System for nitride semiconductor research.

Resonance’s VUV fluorescence detection system measures Troposphere CO in DOE Atmospheric Field Studies (Phoenix 98, Philadelphia 99, Huston 2000, Pennsylvania 04).

Resonance develops space-qualified visible light sources for the Space Station Special Purpose Dexterous Manipulator (SPDM)  OTCM Program.

Resonance’s Tiny WINDO measures Atomic Oxygen in the Middle Atmosphere and Stratosphere.

Resonance develops and space qualifies the thermally-stabilized, fiber-optic UV charge control system used in the Gravity Probe B mission.  This mission will measure the gravitational effects of General Relativity.

Atomic Oxygen exposure and Measurement System for spacecraft materials studies is developed and built for the Canadian Space Agency.

Resonance develops, tests and delivers rocket qualified sodium and potassium line sources for atmospheric concentrations measurements from a payload launched on a Black Brant rocket.

VUV Light Sources used for in-flight calibration of the Advanced Camera for Surveys on the Hubble Space Telescope delivered to Ball Aerospace.

A miniaturized space-qualified gas correlation spectrometer for the remote sensing of atmospheric CO and N2O from orbit is developed and integrated into Clark Spacecraft.  The mission was cancelled and the remote sensor goes into storage before later use as an airborne remote sensor (see below).

Aerospace and Communications Group. D2 and Kr lamps to cover spectral range of 110 to 300 nm for the Space Telescope Imaging Spectrograph.

Resonance develops a space-qualified fiber-coupled UV light source to remove electro-static charge for the Gravity Probe-B mission.

Resonance carries out 37,000 km GASCOFIL remote-sensing survey over North America.   These over flights were concurrent with collection of the CO MAPS data on STS 68 between Oct. 1 and 10, 1994.

Resonance develops and space qualifies an array of 16 space-qualified VUV Kr line sources which are used in the 5 year MSX mission to measure water vapor in low earth orbit.

VUV Xe continuum sources and fiber-optics for in-flight calibration of solar wind detectors on the SWE (Solar Wind Experiment on WIND and on HYDRA on POLAR, 178 to 200nm.

Resonance’s gas correlation spectrometer is modified and used to make cross road measurements of CO across an urban roadway in Albuquerque New Mexico.

Hubble Space Telescope,  VUV D2 sources for in-flight calibration of the Wide Field/Planetary Camera II, 110 to 400nm.

Resonance’s gas correlation spectrometer is used to make pioneering IR remote-sensing measurements of gases from the Andean Volcano Galeras in Southern Columbia.

Resonance’s self-calibrating rocket payload employing resonance fluorescence is used to make the shock-free measurements of atomic oxygen between 70 and 200 km.

Space-qualified array of VUV Krypton line sources for the measurement of water vapor using VUV-induced dissociative fluorescence from a Titan rocket.

Resonance’s gas correlation spectrometer is modified and used to make remote sensing measurements of CO column concentrations around a major urban center.

Resonance’s gas correlation spectrometer is modified and used to simulate remote sensing of CO and CH4 from orbit.

Resonance develops a space-qualified UV-D2 continuum light sources for the in-flight calibration the satellite-borne Ultraviolet Plume Instrument.

Resonance develops an IR Scanning Spectrometer remote sensor and measures trace gases in a large forest fire plume.

Resonance uses GASCOFIL to make measurements of SO2 and NO2 in a large forest fire plume.

UV Kr continuum sources for in-flight calibration of satellite-borne UV camera.

Resonance develops a microprocessor-controlled UV gas correlation spectrometer and successfully measures the SO2 plume-flux from a coal-fueled power generating facility.

Rocket payload employing resonance fluorescence and absorption for the measurement of atomic oxygen and nitrogen between 70 and 200 km.

Atomic oxygen light sources for resonance fluorescence and absorption measurements of the atmosphere between 60 and 250 km.

Resonance starts a project to develop gas correlation spectrometers for tropospheric remote sensing.

Long Path Absorption Experiment (MA-059), VUV resonance lamps for in-situ measurement of oxygen and nitrogen by resonance absorption and fluorescence, 120nm and 130nm