Kovalenko, V. A. (1981) Energy balance of the corona and the origin of quasi-stationary high-speed solar wind streams. Solar Physics, 73 (2). 383-403 doi:10.1007/bf00151689

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Reference Type	Journal (article/letter/editorial)
Title	Energy balance of the corona and the origin of quasi-stationary high-speed solar wind streams
Journal	Solar Physics
Authors	Kovalenko, V. A.		Author
Year	1981 (October)	Volume	73
Issue	2
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00151689Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8917085	Long-form Identifier	mindat:1:5:8917085:8
GUID	0
Full Reference	Kovalenko, V. A. (1981) Energy balance of the corona and the origin of quasi-stationary high-speed solar wind streams. Solar Physics, 73 (2). 383-403 doi:10.1007/bf00151689
Plain Text	Kovalenko, V. A. (1981) Energy balance of the corona and the origin of quasi-stationary high-speed solar wind streams. Solar Physics, 73 (2). 383-403 doi:10.1007/bf00151689
In	(1981, October) Solar Physics Vol. 73 (2) Springer Science and Business Media LLC

	*Lindblad, B. A. (1981) Preferred bartels days of high-speed plasma streams in the solar wind. Solar Physics, 74 (1). 187-196 doi:10.1007/bf00151289*
	*Lindblad, B. A., Lundstedt, H. (1981) A catalogue of high-speed plasma streams in the solar wind. Solar Physics, 74 (1). 197-206 doi:10.1007/bf00151290*
	*Smith, Z., Dryer, M. (1991) Numerical simulations of high-speed solar wind streams within 1 AU and their signatures at 1 AU. Solar Physics, 131 (2). 363-383 doi:10.1007/bf00151644*
	Vršnak, Bojan, Temmer, Manuela, Veronig, Astrid M. (2007) Coronal Holes and Solar Wind High-Speed Streams: I. Forecasting the Solar Wind Parameters. Solar Physics, 240 (2). 315-330 doi:10.1007/s11207-007-0285-8
	*Lindblad, B.A., Lundstedt, H. (1983) A catalogue of high-speed plasma streams in the solar wind 1975?78. Solar Physics, 88 (1). doi:10.1007/bf00196200*
	*Cally, P. S. (1987) Magnetohydrodynamic tube waves and high speed solar wind streams. Solar Physics, 108 (1). 183-189 doi:10.1007/bf00152086*
	Obridko, V. N., Shelting, B. D. (2011) Relationship between the Parameters of Coronal Holes and High-Speed Solar Wind Streams over an Activity Cycle. Solar Physics, 270 (1). 297-310 doi:10.1007/s11207-011-9753-2
	*Chashei, I. V. (1997) MHD Waves in Energy Balance of the Solar Wind and the Solar Corona. Journal of geomagnetism and geoelectricity, 49. doi:10.5636/jgg.49.supplement_s39*
	Balthasar, Horst, Sch�ssler, Manfred (1983) Preferred longitudes of sunspot groups and high-speed solar wind streams: Evidence for a ?solar memory?. Solar Physics, 87 (1). 23-36 doi:10.1007/bf00151156
	*Eselevich, V. G. (1992) Relationships of quasi-stationary solar wind flows with their sources on the Sun. Solar Physics, 137 (1). 179-197 doi:10.1007/bf00146583*
	*Nakada, M.P. (1970) A study of the composition of the solar corona and solar wind. Solar Physics, 14 (2). doi:10.1007/bf00221331*

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Kovalenko, V. A. (1981) Energy balance of the corona and the origin of quasi-stationary high-speed solar wind streams. Solar Physics, 73 (2). 383-403 doi:10.1007/bf00151689

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