Pudovkin, M. I., Zaitseva, S. A., Puchenkina, S. P. (1985) Dependence of the flare stream velocity on magnetic field orientation. Solar Physics, 95 (2). 371-380 doi:10.1007/bf00152414

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Reference Type	Journal (article/letter/editorial)
Title	Dependence of the flare stream velocity on magnetic field orientation
Journal	Solar Physics
Authors	Pudovkin, M. I.		Author
	Zaitseva, S. A.		Author
	Puchenkina, S. P.		Author
Year	1985 (February)	Volume	95
Issue	2
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00152414Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8917901	Long-form Identifier	mindat:1:5:8917901:7
GUID	0
Full Reference	Pudovkin, M. I., Zaitseva, S. A., Puchenkina, S. P. (1985) Dependence of the flare stream velocity on magnetic field orientation. Solar Physics, 95 (2). 371-380 doi:10.1007/bf00152414
Plain Text	Pudovkin, M. I., Zaitseva, S. A., Puchenkina, S. P. (1985) Dependence of the flare stream velocity on magnetic field orientation. Solar Physics, 95 (2). 371-380 doi:10.1007/bf00152414
In	(1985, February) Solar Physics Vol. 95 (2) Springer Science and Business Media LLC

	*Pudovkin, M. I., Zaitseva, S. A., Oleferenko, I. P., Chertkov, A. D. (1977) The structure of the solar flare stream magnetic field. Solar Physics, 54 (1). 155-164 doi:10.1007/bf00146432*
	Pudovkin, M. I., Zaitseva, S. A., Besser, B. P. (1995) Magnetopause magnetic barrier parameters in dependence on the solar wind magnetic field orientation. Annales Geophysicae, 13 (8) 828-835 doi:10.1007/s00585-995-0828-y
	*Pudovkin, M. I., Benevolenska, E. E. (1985) The internal magnetic field of the Sun and peculiarities of the solar activity cycles. Solar Physics, 95 (2). 381-390 doi:10.1007/bf00152415*
	Pudovkin, M. I., Besser, B. P., Zaitseva, S. A. (1998) Magnetopause stand-off distance in dependence on the magnetosheath and solar wind parameters. Annales Geophysicae, 16 (4) 388-396 doi:10.1007/s00585-998-0388-z
	Pudovkin, M. I., Zaitseva, S. A. (1986) Comment on “Magnetic field on the sun and the north-south component of transient variation of the interplanetary magnetic field at 1 AU” by F. Tang et al. Journal of Geophysical Research, 91. 13765 doi:10.1029/ja091ia12p13765
	*Antiochos, S. K., Sturrock, P. A. (1976) Influence of magnetic field structure on the conduction cooling of flare loops. Solar Physics, 49 (2). 359-367 doi:10.1007/bf00162458*
	*Pudovkin, M. I., Zaitseva, S. A., Shumilov, N. O., Meister, C.-V. (1998) Solar Physics, 178 (1). Springer Science and Business Media LLC. 125-136 doi:10.1023/a:1004943102679*
	Pudovkin, M. I., Ponyavin, D. I., Chertkov, A. D. (1980) Recurrency and the origin of the vertical component of the interplanetary magnetic field. Solar Physics, 66 (2). 411-416 doi:10.1007/bf00150594
	*Kahler, S. W. (1978) The dependence of solar flare energetics on flare volumes. Solar Physics, 59 (1). 87-104 doi:10.1007/bf00154933*
	*Venkatakrishnan, P. (1990) Loss of magnetic tension in pre-flare magnetic configurations. Solar Physics, 128 (2). 371-376 doi:10.1007/bf00838473*
	*Pudovkin, M.I., Chertkov, A.D. (1976) Magnetic field of the solar wind. Solar Physics, 50 (1). doi:10.1007/bf00206203*

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Pudovkin, M. I., Zaitseva, S. A., Puchenkina, S. P. (1985) Dependence of the flare stream velocity on magnetic field orientation. Solar Physics, 95 (2). 371-380 doi:10.1007/bf00152414

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