Hu, Y. Q. (2003) A 2.5-dimensional MHD Alfvén-wave-driven solar wind model. Journal of Geophysical Research, 108. doi:10.1029/2003ja009889

Library Home Bookshelves View by Type Using Search

Books Catalogs/Sales Lists Journals Reports Thesis/Dissertation Video

Search for Books Search for Journals Manage Subjects Statistics Books without DDC/LCC Top Unstructured Orphaned Articles

Bookshelves (DDC layout)Bookshelves (LCC layout)Visual Explorer DDC Treemap LCC Treemap DDC/LCC Crosswalk Classification Heatmap Latest Books

Advanced

Search inside 'Journal of ...' only

- Only viewable:

Reference Type	Journal (article/letter/editorial)
Title	A 2.5-dimensional MHD Alfvén-wave-driven solar wind model
Journal	Journal of Geophysical Research
Authors	Hu, Y. Q.		Author
Year	2003	Volume	108
Publisher	American Geophysical Union (AGU)
DOI	doi:10.1029/2003ja009889Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	857710	Long-form Identifier	mindat:1:5:857710:2
GUID	0
Full Reference	Hu, Y. Q. (2003) A 2.5-dimensional MHD Alfvén-wave-driven solar wind model. Journal of Geophysical Research, 108. doi:10.1029/2003ja009889
Plain Text	Hu, Y. Q. (2003) A 2.5-dimensional MHD Alfvén-wave-driven solar wind model. Journal of Geophysical Research, 108. doi:10.1029/2003ja009889
In	(2002) Journal of Geophysical Research Vol. 108. American Geophysical Union (AGU)

	*Li, Bo (2004) A two-dimensional Alfvén wave–driven solar wind model with proton temperature anisotropy. Journal of Geophysical Research, 109. doi:10.1029/2003ja010313*
	*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*
	*Hu, Y. Q. (2003) Are coronal holes the only source of fast solar wind at solar minimum?. Journal of Geophysical Research, 108. doi:10.1029/2002ja009776*
	*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*
	Orlando, S., Lou, Y.-Q., Rosner, R., Peres, G. (1996) Propagation of three-dimensional Alfvén waves in a stratified, thermally conducting solar wind. Journal of Geophysical Research: Space Physics, 101. 24443-24456 doi:10.1029/96ja02304
	*Damiano, P. A. (2005) Two-dimensional hybrid MHD-kinetic electron simulations of an Alfvén wave pulse. Journal of Geophysical Research, 110. doi:10.1029/2004ja010603*
	*Cable, S., Lin, Y. (1998) MHD simulations of oppositely propagating Alfvén waves in the magnetosheath and solar wind. Geophysical Research Letters, 25 (11) 1821-1824 doi:10.1029/98gl01397*
	*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*
	*Ofman, L. (2010) Hybrid model of inhomogeneous solar wind plasma heating by Alfvén wave spectrum: Parametric studies. Journal of Geophysical Research: Space Physics, 115. doi:10.1029/2009ja015094*
	*Chen, Y. (2003) Martian hydrogen exosphere charge exchange with solar wind. Journal of Geophysical Research, 108. doi:10.1029/2002ja009604*
	Lepping, R. P. (2003) Two-dimensional curvature of large angle interplanetary MHD discontinuity surfaces: IMP-8 and WIND observations. Journal of Geophysical Research, 108. doi:10.1029/2002ja009640

版权所有© mindat.org1993年至2026年，除了规定的地方。 Mindat.org全赖于全球数千个以上成员和支持者们的参与。
To cite: Ralph, J., Von Bargen, D., Martynov, P., Zhang, J., Que, X., Prabhu, A., Morrison, S. M., Li, W., Chen, W., & Ma, X. (2025). Mindat.org: The open access mineralogy database to accelerate data-intensive geoscience research. American Mineralogist, 110(6), 833–844. doi:10.2138/am-2024-9486.
隐私政策 - 条款和条款细则 - 联络我们 - Report a bug/vulnerability Current server date and time: 2026.6.7 21:26:39

Go to top of page

Hu, Y. Q. (2003) A 2.5-dimensional MHD Alfvén-wave-driven solar wind model. Journal of Geophysical Research, 108. doi:10.1029/2003ja009889

See Also