A5071020334- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
- Neutrino Physics Research
- Atmospheric Ozone and Climate
- Ionosphere and magnetosphere dynamics
- Particle Detector Development and Performance
- Atmospheric aerosols and clouds
- Lightning and Electromagnetic Phenomena
- Robotics and Sensor-Based Localization
- Gaze Tracking and Assistive Technology
- Calibration and Measurement Techniques
- Solar and Space Plasma Dynamics
- IoT-based Smart Home Systems
- Atmospheric and Environmental Gas Dynamics
- Gamma-ray bursts and supernovae
- Advanced Neural Network Applications
- Robot Manipulation and Learning
- Atomic and Subatomic Physics Research
- Photocathodes and Microchannel Plates
- Hand Gesture Recognition Systems
Skolkovo Institute of Science and Technology
2024
Joint Institute for Nuclear Research
2019
University of Turin
2019
Lomonosov Moscow State University
2019
Authorised Association Consortium
2013
Regatta (Norway)
2013
S. P. Korolev Rocket and Space Corporation Energia (Russia)
2007
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 (Tracking Ultraviolet Set-up) is the world's first orbital detector of ultra-high-energy cosmic rays (UHECRs). It was launched into orbit on 28th April 2016 as a part scientific payload Lomonosov satellite. The main aim mission to test technique measuring ultraviolet fluorescence and Cherenkov radiation extensive air showers generated by primary with energies above ∼100 EeV in Earth atmosphere from space. During its operation for 1.5 years, registered almost 80,000 events few them...
The orbital detector TUS (Tracking Ultraviolet Setup) with high sensitivity in near-visible ultraviolet (tens of photons per time sample 0.8 μ s wavelengths 300–400 nm from a detector’s pixel field view) and the microsecond-scale temporal resolution was developed by Lomonosov-UHECR/TLE collaboration launched into orbit on 28 April 2016. A variety different phenomena were studied measuring signals atmosphere: extensive air showers ultra-high-energy cosmic rays, lightning discharges, transient...
The automation of the car charging process is motivated by rapid development technologies for self-driving cars and increasing importance ecological transportation units. Automation this requires implementation Computer Vision (CV) techniques. However, it remains challenging to precisely position charger plug autonomously due sensitivity CV algorithms lighting weather conditions. We introduce a novel robotic operation system based on hand gesture recognition through teleconferencing...
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.
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.
TUS (Tracking Ultraviolet Set-up) is the world’s first orbital detector of ultra-high-energy cosmic rays (UHECRs). It was launched into orbit on April 28, 2016, as a part scientific payload Lomonosov satellite. The main aim mission to test technique measuring ultraviolet fluorescence and Cherenkov radiation extensive air showers generated by primary with energies above $\sim$100 EeV in nocturnal atmosphere Earth from space. During its operation period, registered almost 80,000 events, few...