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Lin, R.P., Anderson, K.A., Ashford, S., Carlson, C., Curtis, D., Ergun, R., Larson, D., McFadden, J., McCarthy, M., Parks, G.K., Reme, H., Bosqued, J.M., Coutelier, J., Cotin, F., D’uston, C., Wenzel, K.-P., Sanderson, T.R., Henrion, J., Ronnet, J.C. and Paschmann, G. (1995) A Three-Dimensional Plasma and Energetic Particle Investigation for the WIND Spacecraft. Space Science Reviews, 71, 125-153.
http://dx.doi.org/10.1007/BF00751328

has been cited by the following article:

• TITLE: Relativity and the Solar Wind: The Maxwell-Equation Origins of the Solar-Wind Motional Electric Field

  AUTHORS: Joseph E. Borovsky

  KEYWORDS: Lorentz Transformation, Electric Field, Induction, Helmholtz Decomposition, Solar Wind, Magnetic Structure, Heliosphere, Plasma

  JOURNAL NAME: Journal of Electromagnetic Analysis and Applications, Vol.8 No.8, August 23, 2016

  ABSTRACT: The motional electric field of the solar wind as seen by the Earth is examined theoretically and with spacecraft measurements. As it flows outward from the sun, the solar-wind plasma carries a spatially structured magnetic field with it. To calculate the motional electric field of the solar wind the spatially structured magnetic field is Lorentz transformed; for a full physical understanding, it is also necessary to Lorentz transform the current densities and charge densities in the solar wind. Referring to Maxwell’s equations, two related questions are asked: 1) Is the source of the solar-wind motional electric field charge density in the solar wind, time derivatives of current densities in the solar wind, or both? 2) Is the solar-wind motional electric field at Earth an electrostatic field, an induction field, or a superposition of the two? A Helmholtz decomposition of the motional electric field of the solar wind is made into a divergence-origin (electrostatic) and a curl-origin (induction) electric field. The global electric field associated with the outward advection of the global Parker-spiral magnetic field is found to be electrostatic with its origin being a distributed charge density in the solar-wind plasma. The electrostatic versus induction nature of the time-varying electric field associated with the advection of mesoscale magnetic structure varies with time as differently shaped magnetic structures in the solar-wind plasma pass the Earth; the mesoscale structure of the solar-wind plasma contains sheets of space charge and sheets wherein the current density has nonzero time derivatives.