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Usmanov, Arcadi V. - Earth Physics Department, Institute of Physics, St. Petersburg State University
Three-dimensional MHD modeling of the solar corona and Arcadi V. Usmanov
A Global MHD Model of the Solar Wind: Comparison with Ulysses Data
The Astrophysical Journal, 727:84 (13pp), 2011 February 1 doi:10.1088/0004-637X/727/2/84 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
A three-dimensional MHD solar wind model with pickup protons
Low-density anomalies and sub-Alfvenic solar wind A. V. Usmanov,1,2
A tilted-dipole MHD model of the solar corona and solar wind A. V. Usmanov1
1.1 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 1.2 . . . 25
