Dryer, Murray (1996) Comments on the origins of coronal mass ejections. Solar Physics, 169 (2). doi:10.1007/bf00190618

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Reference Type	Journal (article/letter/editorial)
Title	Comments on the origins of coronal mass ejections
Journal	Solar Physics
Authors	Dryer, Murray		Author
Year	1996 (December)	Volume	169
Issue	2
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00190618Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8920503	Long-form Identifier	mindat:1:5:8920503:9
GUID	0
Full Reference	Dryer, Murray (1996) Comments on the origins of coronal mass ejections. Solar Physics, 169 (2). doi:10.1007/bf00190618
Plain Text	Dryer, Murray (1996) Comments on the origins of coronal mass ejections. Solar Physics, 169 (2). doi:10.1007/bf00190618
In	(1996, December) Solar Physics Vol. 169 (2) Springer Science and Business Media LLC

	*Kuijpers, Jan, Fletcher, Lyndsay (1996) Are coronal mass ejections caused by magnetic pumping?. Solar Physics, 169 (2). doi:10.1007/bf00190617*
	*MacQueen, R. M. (1993) The three-dimensional structure of ?loop-like? coronal mass ejections. Solar Physics, 145 (1). 169-188 doi:10.1007/bf00627992*
	*Maxwell, Alan, Dryer, Murray (1981) Solar radio bursts of spectral type II, coronal shocks, and optical coronal transients. Solar Physics, 73 (2). 313-329 doi:10.1007/bf00151684*
	Wu, Chin-Chun, Dryer, Murray (1996) predicting the initial IMF Bzpolarity's change at 1 AU caused by shocks that precede coronal mass ejections. Geophysical Research Letters, 23 (14) 1709-1712 doi:10.1029/96gl01721
	Harrison, R. A., Waggett, P. W., Bentley, R. D., Phillips, K. J. H., Bruner, M., Dryer, M., Simnett, G. M. (1985) The X-ray signature of solar coronal mass ejections. Solar Physics, 97 (2). 387-400 doi:10.1007/bf00165998
	*Shanmugaraju, A., Moon, Y.-J., Cho, K.-S., Dryer, M., Umapathy, S. (2006) Origin of Coronal Shocks without Mass Ejections. Solar Physics, 233 (1). 117-127 doi:10.1007/s11207-006-2095-9*
	*Sawyer, C. (1985) Visibility and rate of coronal mass ejections. Solar Physics, 98 (2). 369-378 doi:10.1007/bf00152466*
	*Webb, D.F., Hundhausen, A.J. (1987) Activity associated with the solar origin of coronal mass ejections. Solar Physics, 108 (2). 383-401 doi:10.1007/bf00214170*
	*Wright, C.S., McNamara, L.F. (1983) The relationships between disappearing solar filaments, coronal mass ejections, and geomagnetic activity. Solar Physics, 87 (2). doi:10.1007/bf00224849*
	*Song, M.T., Wu, S.T., Dryer, M. (1987) A linear MHD instability analysis of solar mass ejections with gravitation. Solar Physics, 108 (2). 347-382 doi:10.1007/bf00214169*
	*Beckers, JacquesM. (1996) Comments on the next generation of ground-based solar telescopes. Solar Physics, 169 (2). doi:10.1007/bf00190619*

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Dryer, Murray (1996) Comments on the origins of coronal mass ejections. Solar Physics, 169 (2). doi:10.1007/bf00190618

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