Publications
- Why does the total pressure on the subsolar magnetopause differ from the solar wind dynamic pressure?2013 | Faculty of Mathematics and Physics
- Why does the subsolar magnetopause move sunward for radial interplanetary magnetic field?2012 | Faculty of Mathematics and Physics
- Statistical Study of the Solar Wind Velocity Modification Upstream of the Earth's Bow Shock: THEMIS Observations2012 | Faculty of Mathematics and Physics
- Evolution of the Solar Wind Speed from the L1 to Earth2010 | Faculty of Mathematics and Physics
- Analysis of temperature versus density plots and their relation to the LLBL formation under southward and northward IMF orientations2015 | Faculty of Mathematics and Physics
- A new three-dimensional magnetopause model with a support vector regression machine and a large database of multiple spacecraft observations2013 | Faculty of Mathematics and Physics
- Solar Wind Modification Upstream of the Bow Shock2013 | Faculty of Mathematics and Physics
- A new approach to magnetopause and bow shock modeling based on automated region identification2012 | Faculty of Mathematics and Physics
- Dependence of the Magnetopause Position on the Upstream Parameters2012 | Faculty of Mathematics and Physics
- Dependence of Magnetopause Locations on the IMF BZ Component During the Solar Minimum2011 | Faculty of Mathematics and Physics
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