@article {,
	title = {{The heliospheric magnetic flux, solar wind proton flux, and cosmic ray intensity during the coming solar minimum}},
	journal = {Space Weather},
	volume = {12},
	year = {2014},
	pages = {499-507},
	keywords = {coronal mass ejections, Dalton Minimum, galactic cosmic rays, interplanetary magnetic field, solar cycle, solar minimum, solar wind},
	doi = {10.1002/2014SW001067},
	author = {Smith, C.~W. and McCracken, K.~G. and Schwadron, N.~A. and Goelzer, M.~L.}
}
@article {7,
	title = {{An analysis of heliospheric magnetic field flux based on sunspot number from 1749 to today and prediction for the coming solar minimum}},
	journal = {Journal of Geophysical Research (Space Physics)},
	volume = {118},
	year = {2013},
	pages = {7525-7531},
	keywords = {coronal mass ejections, interplanetary magnetic fields, magnetic reconnection, solar wind},
	doi = {10.1002/2013JA019404},
	author = {Goelzer, M.~L. and Smith, C.~W. and Schwadron, N.~A. and McCracken, K.~G.}
}
@article {,
	title = {{Initiation of Coronal Mass Ejections by Sunspot Rotation}},
	journal = {\solphys},
	volume = {286},
	year = {2013},
	pages = {453-477},
	keywords = {Active regions, corona, coronal mass ejections, initiation and propagation, magnetic fields, models, sunspots, velocity},
	doi = {10.1007/s11207-013-0269-9},
	author = {T{\"o}r{\"o}k, T. and Temmer, M. and Valori, G. and Veronig, A.~M. and van Driel-Gesztelyi, L. and Vr\v snak, B.}
}
