Nonradial and nonpolytropic astrophysical outflows. VII. Fitting ULYSSES solar wind data during minimumC. Sauty, J.~J.~G. Lima, N. Iro, K. TsinganosPosted Mar 1, 2005 Cite DOIAdd the full text or supplementary notes for the publication here using Markdown formatting.Magnetohydrodynamics (Mhd) Solar Wind Sun: Corona Sun: Magnetic Fields Stars: Winds Outflows