The steady isothermal Parker wind differential equation also has positive solutions describing subsonic flow at every radius. Write their first integral as , where and . On the small- branch at large radius, , so . Constant spherical mass flow rate then gives nonzero limiting mass density and hence finite external pressure. This distinguishes a pressure-confined breeze from an escaping wind into vanishing pressure. Specifying outward motion alone does not select the supersonic asymptotic branch.
For unattenuated isotropic radiation from a point source, the radiation pressure force on each absorbing particle is . Dividing by its mass changes the effective inverse-square inward acceleration to . The wind equation therefore places the maximum of a subsonic isothermal breeze at the displayed radius, provided the bracket is positive. If it is nonpositive, the positive-temperature subsonic outflow decreases in speed throughout its domain and has no interior speed maximum. A cross section per particle requires that particle's mass; an opacity per unit mass instead absorbs this conversion.
A steady spherical subsonic isothermal breeze with isothermal sound speed obeys . Since , its finite-radius speed maximum lies at . Spherical mass conservation then gives the displayed density, where is the peak Mach number. This free parameter is selected by a boundary condition, not by , and alone. Therefore , while a peak Mach number of order unity gives that expression as a characteristic scale.
A direct demonstration of the free parameter comes from the first integral . Its additive constant remains free for a breeze; imposing the regular transonic branch would be a different condition.
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