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From nano to space #BlueSkies research vs. R&D

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.

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From nano to space #BlueSkies research vs. R&D

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  1. From nano to space#BlueSkies research vs. R&D Alexander Rodin Department for Problems of Power and Energy

  2. Blue skies projects at ‘megagrant labs’: High resolution heterodyne spectroscopy

  3. 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

  4. 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

  5. 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

  6. 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,

  7. “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

  8. Hot electron bolometer as IR mixers SSPD, plasmonic field amplifiers Lobanov et al., 2014 IF range 0.1 – 5 GHz

  9. General circulation models of planetary atmospheres Radiative transfer calculations, inverse problem solutions:

  10. MIPT is openfor versatile cooperation in environmental and planetary missions

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