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Discover the innovative use of multichannel diode laser spectroscopy in Martian studies, part of the megagrant labs' international projects. Join top universities and companies in advancing optical technologies for space exploration. Learn about the optical chip design and resonator technology enabling groundbreaking research in planetary atmospheres. Engage in a new era of space exploration and environmental missions with cutting-edge technologies.
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From nano to space#BlueSkies research vs. R&D Alexander Rodin Department for Problems of Power and Energy
Blue skies projects at ‘megagrant labs’: High resolution heterodyne spectroscopy
Implementation in large-scale international projects:Multichannell Diode Laser Spectroscopy for Martian studies Work group • IKI RAS (Moscow),, GPI RAS (Moscow), MIPT (Dolgoprudnyi, Moscow Region), MGTU (Moscow),SPE Astron Electronics Ltd. (Orel) • University of Reims (France), University of Cologne (Germany), University of Edinburgh (Gr. Britain) • Nanoplus, Innoptics and other Companies. Reims, 2014.06.26
M-TDLAS laser & heterodyne spectrometer Stationery Landing Platform view Housekeeping systems bays Mast with TV-complex and UHF antenna (stowed) Manipulator (stowed) Hydrazine tank Scientific instruments Doppler Radar ACS Thrusters Landing Gears
Another large scale international project: Participation in JUICE/SWI experiment (1.2 THz channel) 5 The Submillimeter Wave Instrument (SWI) will study the Galilean satellites, the chemistry, meteorologyand structure of Jupiter’s middle atmosphere and atmospheric and magnetospheric coupling processes. • Telescope D ~ 30 cm Spatial resolution < 1200 км @ 15-20 RJ distance Vertical resolution: < ~ scale height • Two spectral bands: 400-600GHz (550 мкм) 1080-1280GHz (230 мкм) • Detection capabilities 1 min: line contrast ~ 0.6 – 1.65 K 1 hour: line contrast ~ 0.1 – 0.25 K
Metaoptics, photonics and metamaterials for M-TDLAS: IKI design and calculations: Lucas Labadie, Robert R. Thomson et al., Advances in the Development of Mid-Infrared Integrated Devices for Interferometric Arrays. Proc. SPIE 8445, 844515 doi:10.1117/12.925636, 2012 - optical chip calculation at MIPT,- optical chip 3D laser assisted printing in the University of Edinburgh,- optical fiber interfacing of the optical waveguide chip in the University of Cologne,
“Whispering-gallery mode” resonators • Resonators – microspheres, discs , tori • Extremely high Q-factor (106 - 109) • Exited WGMs emit from the equator • For resonators with integrable shapes the emission is isotropic
Hot electron bolometer as IR mixers SSPD, plasmonic field amplifiers Lobanov et al., 2014 IF range 0.1 – 5 GHz
General circulation models of planetary atmospheres Radiative transfer calculations, inverse problem solutions:
MIPT is openfor versatile cooperation in environmental and planetary missions