Wang, Y.-M., Sheeley, N. R., Jr. (1992) On potential field models of the solar corona. The Astrophysical Journal, 392. 310pp. doi:10.1086/171430

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Reference Type	Journal (article/letter/editorial)
Title	On potential field models of the solar corona
Journal	The Astrophysical Journal
Authors	Wang, Y.-M.		Author
Authors	Sheeley, N. R., Jr.		Author
Year	1992 (June)	Volume	392
Publisher	IOP Publishing
DOI	doi:10.1086/171430Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	3331309	Long-form Identifier	mindat:1:5:3331309:4
GUID	0
Full Reference	Wang, Y.-M., Sheeley, N. R., Jr. (1992) On potential field models of the solar corona. The Astrophysical Journal, 392. 310pp. doi:10.1086/171430
Plain Text	Wang, Y.-M., Sheeley, N. R., Jr. (1992) On potential field models of the solar corona. The Astrophysical Journal, 392. 310pp. doi:10.1086/171430
In	(1992) The Astrophysical Journal Vol. 392. IOP Publishing

	*Wang, Y.-M., Sheeley, Jr., N. R. (1995) Solar Implications of [ITAL]Ulysses[/ITAL] Interplanetary Field Measurements. The Astrophysical Journal, 447 (2). doi:10.1086/309578*
	*Sheeley, N. R., Jr., Wang, Y.-M., Nash, A. G. (1992) A new determination of the solar rotation rate. The Astrophysical Journal, 401. 378pp. doi:10.1086/172069*
	*Wang, Y.‐M., Sheeley, Jr., N. R. (2003) On the Topological Evolution of the Coronal Magnetic Field During the Solar Cycle. The Astrophysical Journal, 599 (2). 1404-1417 doi:10.1086/379348*
	*Wang, Y.‐M., Sheeley, Jr., N. R. (2006) Observations of Flux Rope Formation in the Outer Corona. The Astrophysical Journal, 650 (2). 1172-1183 doi:10.1086/506611*
	*Wang, Y.-M., Sheeley, N. R., Jr. (1990) Solar wind speed and coronal flux-tube expansion. The Astrophysical Journal, 355. 726pp. doi:10.1086/168805*
	*Wang, Y.‐M., Sheeley, Jr., N. R. (2006) Sources of the Solar Wind atUlyssesduring 1990–2006. The Astrophysical Journal, 653 (1). 708-718 doi:10.1086/508929*
	*Wang, Y.‐M., Sheeley, Jr., N. R. (2003) On the Fluctuating Component of the Sun’s Large‐Scale Magnetic Field. The Astrophysical Journal, 590 (2). 1111-1120 doi:10.1086/375026*
	*Wang, Y.-M., Sheeley, N. R., Jr. (1991) Why fast solar wind originates from slowly expanding coronal flux tubes. The Astrophysical Journal, 372. doi:10.1086/186020*
	*Sheeley, N. R., Jr., Nash, A. G., Wang, Y.-M. (1987) The origin of rigidly rotating magnetic field patterns on the sun. The Astrophysical Journal, 319. 481pp. doi:10.1086/165472*
	Wang, Y. ‐M., Biersteker, J. B., Sheeley, Jr., N. R., Koutchmy, S., Mouette, J., Druckmuller, M. (2007) The Solar Eclipse of 2006 and the Origin of Raylike Features in the White‐Light Corona. The Astrophysical Journal, 660 (1). 882-892 doi:10.1086/512480
	*Wang, Y.-M., Sheeley, N. R., Jr., Nash, A. G. (1991) A new solar cycle model including meridional circulation. The Astrophysical Journal, 383. 431pp. doi:10.1086/170800*

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Wang, Y.-M., Sheeley, N. R., Jr. (1992) On potential field models of the solar corona. The Astrophysical Journal, 392. 310pp. doi:10.1086/171430

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