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Usmanov, A. V., Goldstein, M. L. (2006) A three-dimensional MHD solar wind model with pickup protons. Journal of Geophysical Research, 111. doi:10.1029/2005ja011533

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Reference TypeJournal (article/letter/editorial)
TitleA three-dimensional MHD solar wind model with pickup protons
JournalJournal of Geophysical Research
AuthorsUsmanov, A. V.Author
Goldstein, M. L.Author
Year2006Volume111
PublisherAmerican Geophysical Union (AGU)
DOIdoi:10.1029/2005ja011533Search in ResearchGate
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Mindat Ref. ID866019Long-form Identifiermindat:1:5:866019:4
GUID0
Full ReferenceUsmanov, A. V., Goldstein, M. L. (2006) A three-dimensional MHD solar wind model with pickup protons. Journal of Geophysical Research, 111. doi:10.1029/2005ja011533
Plain TextUsmanov, A. V., Goldstein, M. L. (2006) A three-dimensional MHD solar wind model with pickup protons. Journal of Geophysical Research, 111. doi:10.1029/2005ja011533
In(2006) Journal of Geophysical Research Vol. 111. American Geophysical Union (AGU)

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Usmanov, Arcadi V., Goldstein, Melvyn L., Besser, Bruno P., Fritzer, Johannes M. (2000) A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data. Journal of Geophysical Research: Space Physics, 105. 12675-12695 doi:10.1029/1999ja000233
Usmanov, A. V. (2003) A tilted-dipole MHD model of the solar corona and solar wind. Journal of Geophysical Research, 108. doi:10.1029/2002ja009777
Usmanov, Arcadi V., Goldstein, Melvyn L., Matthaeus, William H. (2016) A FOUR-FLUID MHD MODEL OF THE SOLAR WIND/INTERSTELLAR MEDIUM INTERACTION WITH TURBULENCE TRANSPORT AND PICKUP PROTONS AS SEPARATE FLUID. The Astrophysical Journal, 820 (1). 17pp. doi:10.3847/0004-637x/820/1/17
Usmanov, Arcadi V., Goldstein, Melvyn L., Matthaeus, William H. (2012) THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC MODELING OF THE SOLAR WIND INCLUDING PICKUP PROTONS AND TURBULENCE TRANSPORT. The Astrophysical Journal, 754 (1). 40pp. doi:10.1088/0004-637x/754/1/40
Li, Bo, Li, Xing, Labrosse, Nicolas (2006) A global 2.5-dimensional three fluid solar wind model with alpha particles. Journal of Geophysical Research, 111. doi:10.1029/2005ja011303
Usmanov, Arcadi V., Matthaeus, William H., Goldstein, Melvyn L., Chhiber, Rohit (2018) The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating. The Astrophysical Journal, 865 (1). 25pp. doi:10.3847/1538-4357/aad687
Vandas, M. (2002) Three-dimensional MHD simulation of a loop-like magnetic cloud in the solar wind. Journal of Geophysical Research, 107. doi:10.1029/2001ja005068
Usmanov, Arcadi V., Goldstein, Melvyn L., Matthaeus, William H. (2014) THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY. The Astrophysical Journal, 788 (1). 43pp. doi:10.1088/0004-637x/788/1/43
Hu, Y. Q. (2003) A 2.5-dimensional MHD Alfvén-wave-driven solar wind model. Journal of Geophysical Research, 108. doi:10.1029/2003ja009889
Podesta, J. J., Roberts, D. A., Goldstein, M. L. (2006) Power spectrum of small-scale turbulent velocity fluctuations in the solar wind. Journal of Geophysical Research, 111. doi:10.1029/2006ja011834
Barakat, Abdallah R., Schunk, Robert W. (2006) A three-dimensional model of the generalized polar wind. Journal of Geophysical Research, 111. doi:10.1029/2006ja011662
 
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