This phenomenon is governed by the ODE  ["rho u dee u dee r equals d p d r minus rho g m over r-squared"], where ? and u are its density and velocity, M is the Sun's mass, G is the gravitational constant, and r is the distance from the Sun.  This almost completely ionized stream creates a bow shock at Earth's magnetosphere since is it supersonic at Earth, corresponding to a class 2 solution of the above ODE, which Eugene 
This phenomenon is governed by the ODE  ["rho u dee u dee r equals d p d r minus rho g m over r-squared"], where ? and u are its density and velocity, M is the Sun's mass, G is the gravitational constant, and r is the distance from the Sun.  This almost completely ionized stream creates a bow shock at Earth's magnetosphere since is it supersonic at Earth, corresponding to a class 2 solution of the above ODE, which Eugene Parker first solved.  FTP, identify this diffuse, radial-flowing stream of ions ejected from the Sun and constantly pushing everything in space.
This phenomenon is governed by the ODE  ["rho u dee u dee r equals d p d r minus rho g m over r-squared"], where ?
solar wind