Brown, G. M. (1981) Possible use of (a) solar faculae and (b) the interplanetary magnetic field as heralds of a solar cycle peak. Solar Physics, 74 (1). 125-129 doi:10.1007/bf00151282

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Reference Type	Journal (article/letter/editorial)
Title	Possible use of (a) solar faculae and (b) the interplanetary magnetic field as heralds of a solar cycle peak
Journal	Solar Physics
Authors	Brown, G. M.		Author
Year	1981 (November)	Volume	74
Issue	1
Publisher	Springer Science and Business Media LLC
DOI	doi:10.1007/bf00151282Search in ResearchGate
	Generate Citation Formats
Mindat Ref. ID	8917104	Long-form Identifier	mindat:1:5:8917104:2
GUID	0
Full Reference	Brown, G. M. (1981) Possible use of (a) solar faculae and (b) the interplanetary magnetic field as heralds of a solar cycle peak. Solar Physics, 74 (1). 125-129 doi:10.1007/bf00151282
Plain Text	Brown, G. M. (1981) Possible use of (a) solar faculae and (b) the interplanetary magnetic field as heralds of a solar cycle peak. Solar Physics, 74 (1). 125-129 doi:10.1007/bf00151282
In	(1981, November) Solar Physics Vol. 74 (1) Springer Science and Business Media LLC

	*Brown, G. M., Evans, D. R. (1980) The use of solar faculae in studies of the sunspot cycle. Solar Physics, 66 (2). 233-243 doi:10.1007/bf00150580*
	*Tritakis, Basil P. (1979) A solar cycle variation of the interplanetary magnetic field configuration. Solar Physics, 63 (1). 207-215 doi:10.1007/bf00155711*
	*Siscoe, G.L., Crooker, N.U., Christopher, L. (1978) A solar cycle variation of the interplanetary magnetic field. Solar Physics, 56 (2). doi:10.1007/bf00152484*
	*Moussas, Xenophon, Tritakis, Basil (1982) Latitudinal and solar-cycle dependence of the interplanetary magnetic field predominant polarity. Solar Physics, 75 (1). 361-375 doi:10.1007/bf00153484*
	*Vainstein, S. I., Kuklin, G. V., Maksimov, V. P. (1977) On a possible mechanism of solar faculae heating. Solar Physics, 53 (1). 15-23 doi:10.1007/bf02260206*
	*Stix, Michael (1981) Theory of the solar cycle. Solar Physics, 74 (1). 79-101 doi:10.1007/bf00151277*
	*Yoshimura, Hirokazu (1977) Coronal general magnetic field evolution as a new parameter of the solar cycle. Solar Physics, 52 (1). 41-52 doi:10.1007/bf00935788*
	Usmanov, A. V. (1993) Interplanetary magnetic field structure and solar wind parameters as inferred from solar magnetic field observations and by using a numerical 2-D MHD model. Solar Physics, 143 (2). 345-363 doi:10.1007/bf00646492
	*Howard, Robert, Labonte, Barry J. (1981) Surface magnetic fields during the solar activity cycle. Solar Physics, 74 (1). 131-145 doi:10.1007/bf00151283*
	*Hawkes, G., Berger, M. A. (2018) Magnetic Helicity as a Predictor of the Solar Cycle. Solar Physics, 293 (7). doi:10.1007/s11207-018-1332-3*
	*Brown, G. M., Evans, D. R. (1980) Latitude variations of photospheric activity areas with particular reference to solar faculae. Solar Physics, 68 (1). 141-149 doi:10.1007/bf00153273*

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Brown, G. M. (1981) Possible use of (a) solar faculae and (b) the interplanetary magnetic field as heralds of a solar cycle peak. Solar Physics, 74 (1). 125-129 doi:10.1007/bf00151282

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