@article {,
	title = {{Inferring the Heliospheric Magnetic Field Back through Maunder Minimum}},
	journal = {\apj},
	volume = {837},
	year = {2017},
	pages = {165},
	keywords = {Sun: coronal mass ejections: CMEs, Sun: heliosphere, Sun: magnetic fields, sunspots},
	doi = {10.3847/1538-4357/aa6191},
	author = {Rahmanifard, F. and Schwadron, N.~A. and Smith, C.~W. and McCracken, K.~G. and Duderstadt, K.~A. and Lugaz, N. and Goelzer, M.~L.}
}
@article {,
	title = {{Global Numerical Modeling of Energetic Proton Acceleration in a Coronal Mass Ejection Traveling through the Solar Corona}},
	journal = {\apj},
	volume = {778},
	year = {2013},
	pages = {43},
	keywords = {acceleration of particles, magnetohydrodynamics: MHD, shock waves, Sun: coronal mass ejections: CMEs, Sun: heliosphere, Sun: particle emission},
	doi = {10.1088/0004-637X/778/1/43},
	author = {Kozarev, K.~A. and Evans, R.~M. and Schwadron, N.~A. and Dayeh, M.~A. and Opher, M. and Korreck, K.~E. and van der Holst, B.}
}
@article {,
	title = {{The Interaction of Two Coronal Mass Ejections: Influence of Relative Orientation}},
	journal = {\apj},
	volume = {778},
	year = {2013},
	pages = {20},
	keywords = {magnetohydrodynamics: MHD, methods: numerical, shock waves, Sun: corona, Sun: coronal mass ejections: CMEs, Sun: heliosphere},
	doi = {10.1088/0004-637X/778/1/20},
	author = {Lugaz, N. and Farrugia, C.~J. and Manchester, W.~B. and Schwadron, N.}
}
@article {,
	title = {{Weakest Solar Wind of the Space Age and the Current {\textquoteleft}{\textquoteleft}Mini{\textquoteright}{\textquoteright} Solar Maximum}},
	journal = {\apj},
	volume = {779},
	year = {2013},
	pages = {2},
	keywords = {dynamo, solar wind, Sun: activity, Sun: corona, Sun: heliosphere, sunspots},
	doi = {10.1088/0004-637X/779/1/2},
	author = {McComas, D.~J. and Angold, N. and Elliott, H.~A. and Livadiotis, G. and Schwadron, N.~A. and Skoug, R.~M. and Smith, C.~W.}
}
