Realisations
2031: Spectrometer onboard of ESA’s EnVision mission to Venus. It aims at mapping the atmosphere near the surface and above the cloud deck.
2029: Combined electric and magnetic field sensor onboard ESA's Comet Interceptor mission for use during comet flyby.
2024: To measure the high-energy particle fluxes around the Earth. It is the three dimensional successor of EPT.
2023: Mini solar tracker to follow the Sun during ground based measurements.
2020: Portable spectro-polarimeter, capable of measuring polar aurorae in the optical domain between 427.8 and 630 nm.
2020: Atmospheric remote sensing and in-situ ionospheric plasma measurement with a CubeSat.
2019: DOAS measurement technique "Bike-DOAS" observes the composition of the troposphere from a bicycle.
2019: Small autonomous space instrument on-board a PROBA-satellite, keeping an eye on the amount of ozone.
2016: Spectrometer suite on board ESA’s Trace Gas Orbiter (TGO) satellite.
2015: Parts for the mass spectrometry lab that uses the technique of chemical ionization to study reactions that occur in the atmosphere.
2014: Hardware to study in-situ biogenic components in the lowest layers of our atmosphere and their influence on air pollution.
2013: Samples of NO2 and SO2 locally by observing from small aircrafts or UAVs using a small imaging spectrometer.
2013 - Instrument developed to measure high-energy particle fluxes around the Earth with good energy, angular and mass resolutions.
2012: Uses the Differential Optical Absorption Spectroscopy (DOAS) technique to measure stratospheric and tropospheric trace gases.
2010: Network of radio receivers, spread over Belgium, that makes use of forward scattering techniques to study the meteoroid population.
2005: Compact high-resolution spectrometer, developed for ESA’s Venus Express spacecraft, that operates in the IR wavelength range.
2004: a Bruker Fourier Transform Spectrometer with solar tracker, self-contained liquid nitrogen filling system and meteorological station.
2003: Imaging spectrometer with an UV and IR channel. It aims at measuring the composition of the Martian atmosphere.
1996: Two-channel solar spectrometer. Part of the Russian Mars-96 mission.
1996: Instrument that combined two fluxgate magnetometers and a 3D electron spectrometer. Part of the Russian Mars-96.
1992: Instrument (part of the EURECA mission) able to measure ozone, NO2, aerosols and water vapor in the near infrared, visible and near UV.
1991: SIDAMS and MACSIMS are balloon borne mass spectrometers for the in-situ measurement of ions and neutrals in the stratosphere.