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 Reims, 2014.06.26 Space Research Institute (IKI) RAS: Planetary exploration division. Experimental spectroscopy laboratory and other laboratories. MIPT: Department of Problems of Physics and Energetics. Laboratory ISPAVR. GPI RAS: Department of Diode laser spectroscopy. Laboratory of Applied diode laser spectroscopy, laboratory of Spectroscopy of molecular interactions. 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.

4. Housekeeping systems bays Hydrazine tank Mast with TV-complex and UHF antenna (stowed) Doppler Radar ACS Thrusters Landing Gears Scientific instruments Manipulator (stowed) Stationery Landing Platform view M-TDLAS laser & heterodyne spectrometer

5. Telescope D ~ 30 cm Spatial resolution < 1200 км @ 15-20 RJ distance Vertical resolution: < ~ scale height Two spectral bands: 400-600 GHz (550 мкм) 1080-1280 GHz (230 мкм ) Detection capabilities 1 min: line contrast ~ 0.6 – 1.65 K 1 hour: line contrast ~ 0.1 – 0.25 K 5 The Submillimeter Wave Instrument (SWI) will study the Galilean satellites, the chemistry, meteorology and structure of Jupiter’s middle atmosphere and atmospheric and magnetospheric coupling processes. Another large scale international project: Participation in JUICE/SWI experiment (1.2 THz channel)

6. Metaoptics, photonics and metamaterials for M-TDLAS: - 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, 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 IKI design and calculations:

7. Resonators – microspheres, discs, tori Extremely high Q-factor (10 6 - 10 9 ) Exited WGMs emit from the equator For resonators with integrable shapes the emission is isotropic “Whispering-gallery mode” resonators

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

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

10. MIPT is open for versatile cooperation in environmental and planetary missions