A5085925218- Ionosphere and magnetosphere dynamics
- Solar and Space Plasma Dynamics
- Earthquake Detection and Analysis
- Geomagnetism and Paleomagnetism Studies
- Astro and Planetary Science
- Astronomical Observations and Instrumentation
- Gamma-ray bursts and supernovae
- Planetary Science and Exploration
- Stellar, planetary, and galactic studies
- Spacecraft Dynamics and Control
- Astrophysics and Cosmic Phenomena
- Advanced Research in Systems and Signal Processing
- Healthcare Systems and Public Health
- HVDC Systems and Fault Protection
- Atmospheric Ozone and Climate
- Spacecraft Design and Technology
- Full-Duplex Wireless Communications
- Acoustic Wave Resonator Technologies
- Astronomy and Astrophysical Research
- Medical and Agricultural Research Studies
- Geophysics and Gravity Measurements
- Energy Harvesting in Wireless Networks
- Geophysics and Sensor Technology
- Space Satellite Systems and Control
Institute of Solar-Terrestrial Physics
2007-2019
Siberian Branch of the Russian Academy of Sciences
2016
Russian Academy of Sciences
2009
We homogeneously analyse $\sim 3.2\times 10^5$ photometric measurements for 1100$ transit lightcurves belonging to $17$ exoplanet hosts. The data cover $16$ years 2004--2019 and include amateur professional observations. Old archival were reprocessed using up-to-date exoplanetary parameters empirically debiased limb-darkening models. also derive self-consistent radial-velocity fits $13$ targets. confirm the nonlinear TTV trend in WASP-12 at a high significance, with consistent magnitude....
Abstract We report on novel features of the saturation process polar cap magnetic flux and Poynting into magnetosphere from solar wind during three superstorms. In addition to well‐known effect interplanetary electric ( E sw ) southward (interplanetary field (IMF) B z fields, we found that depends also ram pressure P d . By means magnetogram inversion technique a global MHD numerical model Piecewise Parabolic Method with Lagrangian Remap, explore dependence magnetopause standoff distance...
A study of intensities large-scale spatial distributions dayside and nightside field-aligned currents (FAC), obtained using the magnetogram inversion technique (MIT) from ground-based magnetometers, during period stationary magnetospheric convection (SMC) on September 24, 1998 is presented. Quantitative qualitative analysis showed that SMC there was a monotonic increase quasi-equilibrium between FACs region 1, while in intensity FAC began before SMC, substorm; end decrease observed.
Within substorm activations during two superstorms (2000 and 2003) from the observations at mid-latitude geomagnetic observatories, we study short-period irregular pulsations airglow in 557.7 nm 630.0 atomic oxygen emission lines, 391.4 ionized nitrogen molecular band. Through genuine magnetogram inversion technique, 1-minute data of ground-based magnetometer global network, investigate distribution dynamics for field-aligned currents (FACs) ionosphere. The relation is shown between...