A5029907846- Ion-surface interactions and analysis
- Astrophysics and Cosmic Phenomena
- Silicone and Siloxane Chemistry
- Polymer Nanocomposite Synthesis and Irradiation
- High-Velocity Impact and Material Behavior
- Dark Matter and Cosmic Phenomena
- Neutrino Physics Research
- Graphite, nuclear technology, radiation studies
- Laser Material Processing Techniques
- Particle Detector Development and Performance
- Ionosphere and magnetosphere dynamics
- Field-Flow Fractionation Techniques
- Radioactivity and Radon Measurements
- Diamond and Carbon-based Materials Research
- Carbon Nanotubes in Composites
- Geomagnetism and Paleomagnetism Studies
- Spacecraft Design and Technology
- Gas Dynamics and Kinetic Theory
- Microstructure and mechanical properties
- Integrated Circuits and Semiconductor Failure Analysis
- Gas Sensing Nanomaterials and Sensors
- Catalytic Processes in Materials Science
- Fuel Cells and Related Materials
- Atmospheric aerosols and clouds
- Earthquake Detection and Analysis
Lomonosov Moscow State University
2012-2024
Russian Academy of Sciences
2014
Moscow State University
2011
TUS (Tracking Ultraviolet Set-up), the first orbital detector of extreme energy cosmic rays (EECRs), those with energies above 50 EeV, was launched into orbit on April 28, 2016, as a part Lomonosov satellite scientific payload. The main aim mission is to test technique registering fluorescent and Cherenkov radiation extensive air showers generated by EECRs in atmosphere space telescope. We present preliminary results its operation mode dedicated period from August 16, November 4, 2016. No...
TUS (Track Ultraviolet Setup) is the first space experiment aimed to check possibility of registering extreme energy cosmic rays (EECRs) at E>50 EeV by measuring fluorescence signal extensive air showers in atmosphere. The detector operates as a part scientific payload Lomonosov satellite for more than year. We describe an algorithm searching EECR events data and briefly discuss number candidates selected formal criteria.
Magnetosphere plasma electron and proton fluxes in the energy range 0.04–11.3 keV were measured using electrostatic spectrometers established onboard geostationary Electro-L2 spacecraft (point of standing 76° EL). Measurements done lit orbit segments Earth shadow during periods vernal autumn equinox 2016–2017. In terms observation data, fluxes, parameters particles for different geomagnetic activity levels potentials metal base determined. The values negative potential achieve 5–10 kV...
On April 28, 2016, the Lomonosov satellite, equipped with a number of scientific instruments, was launched into orbit. Here we present briefly some results obtained first orbital telescope extreme energy cosmic rays TUS and by group detectors aimed at multi-messenger observations gamma-ray bursts.
The possibilities of applying a femtosecond laser-plasma source X-ray radiation for modelling the effect single nuclear particles based on principle equivalent charge generation are analysed. parameters experimental individual effects validated. setup forming is described. results comparative ionisation response in simple electronic devices using FLUKA and FEANT codes presented.
Atomic oxygen (AO) exposure and hard microparticle impact on polyimide nanocomposites were performed by a ground-based magnetoplasmodynamic accelerator electrostatic accelerator, respectively. The computer simulation of the AO erosion was carried out with Monte Carlo method. It is found that are significantly more durable to than pure material. Besides, in case combined exposure, regions around craters created etched intensively undamaged areas nanocomposite sample surface.