Physics – Quantum Physics
Scientist
Physics
Quantum Physics
Scientist
Institute of Magnetism, Kiev, Ukraine
Institute for Dynamics of Geospheres, Russian Academy of Sciences, Moscow, Russia 117939
Institute for Dynamics of Geospheres, Leninsky Prospect, 38, Bldg. 1, 119334 Moscow, Russia
Institute for Dynamics of Geospheres, Russian Academy of Sciences, Moscow, Russia 119334
Institute for the Dynamics of Geospheres, Russian Academy of Sciences, Moscow, Russia 117939.
Institute for Geodynamics and Geospheres, Russian Academy of Science, Leninsky Prospect, 38, 119334 Moscow, Russia
Institute for Dynamics of Geospheres, Russian Academy of Science, Leninsky pr. 38, Bldg.1, Moscow 119334, Russia; Planetary Science Department, The University of Arizona, Tucson, Arizona 85721, USA
AN SSSR, Institut Fiziki Zemli, Moscow, USSR
Institute for Dynamics of Geospheres, Russian Academy of Sciences, 117939, Moscow, Russia
California Institute of Technology
Jet Propulsion Lab., California Institute of Technology
Jet Propulsion Laboratory, Pasadena, California, USA
Jet Propulsion Laboratory, MS 168-514, 4800 Oak Grove Dr., Pasadena, CA 91109 Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, ca 91109 Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109-8099, USA Propulsion Laboratory, MS 168-414 4800 Oak Grove Drive, Pasadena, CA 91109 Science Institute, Tucson, AZ, USA
NASA / Jet Propulsion Laboratory, Pasadena, California, USA
Jet Propulsion Laboratory, 4800 Oak Grove Dr, Pasadena, CA 91109
Ukraine Academy of Sciences
Institute of Dynamics of Geospheres, Russian Academy of Sciences, Moscow, 117939 Russian Federation for Dynamics of Geospheres, Russian Academy of Sciences, Leninskii pr. 38, Moscow, 117979 Russia
Institute for Dynamics of Geospheres, Moscow,
A Comparison of Lunar Crater Size Frequency Distribution and Near-Earth Asteroid Population Characteristics: Strong Evidence for the Stability of their Size Frequency Distribution
A Lower Limit on the Thickness of Europa's Ice Shell from Numerical Simulations of Impact Cratering
A pulsed magnetic field at the time of shock polarization of rocks as a possible cause of lunar magnetic-field anomalies associated with craters
Abrikosov vortex lattice nonlinear dynamics and its stability in the presence of weak defects
Access to Mars Global Surveyor data through the Planetary Image Atlas.
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