AU
Arcadi Usmanov
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0002-0209-152X
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Publications (28)
- Impact of space weather on climate and habitability of terrestrial-type exoplanets Save
- Contextual Predictions for Parker Solar Probe. II. Turbulence Properties and Taylor Hypothesis Save
- Contextual Predictions for the Parker Solar Probe. I. Critical Surfaces and Regions Save
- The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating Save
- Weakened Magnetization and Onset of Large-scale Turbulence in the Young Solar Wind—Comparisons of Remote Sensing Observations with Simulation Save
- Cosmic-Ray Diffusion Coefficients throughout the Inner Heliosphere from a Global Solar Wind Simulation Save
- SOLAR WIND COLLISIONAL AGE FROM A GLOBAL MAGNETOHYDRODYNAMICS SIMULATION Save
- A FOUR-FLUID MHD MODEL OF THE SOLAR WIND/INTERSTELLAR MEDIUM INTERACTION WITH TURBULENCE TRANSPORT AND PICKUP PROTONS AS SEPARATE FLUID Save
- RECONSTRUCTING THE SOLAR WIND FROM ITS EARLY HISTORY TO CURRENT EPOCH Save
- THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY Save
- THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC MODELING OF THE SOLAR WIND INCLUDING PICKUP PROTONS AND TURBULENCE TRANSPORT Save
- SOLAR WIND MODELING WITH TURBULENCE TRANSPORT AND HEATING Save
- TRANSPORT EQUATION FOR MHD TURBULENCE: APPLICATION TO PARTICLE ACCELERATION AT INTERPLANETARY SHOCKS Save
- A three-dimensional MHD solar wind model with pickup protons Save
- Low-density anomalies and sub-Alfvénic solar wind Save
- NUMERICAL SIMULATIONS OF SOLAR WIND TURBULENCE Save
- A tilted-dipole MHD model of the solar corona and solar wind Save
- Three-dimensional MHD modeling of the solar corona and solar wind Save
- A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data Save
- A view of the inner heliosphere during the May 10-11, 1999 low density anomaly Save