An Operable Solution Approach to Interplanetary Hydrodynamic Shock Waves

Details An Operable Solution Approach to Interplanetary Hydrodynamic Shock Waves An Operable Solution Approach to Interplanetary Hydrodynamic Shock Waves

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..184..385f&link_type=abstract

Solar Physics, v. 184, Issue 2, p. 385-402 (1999).

Physics

1

Scientific paper

In this paper, an operable solution approach is proposed to solve interplanetary hydrodynamic shock waves propagating in the interplanetary medium of solar wind background derived from Parker's hydrodynamic model. In our case the problem concerned is reduced to a set of ordinary differential equations (ODEs) involving the solar wind background parameters velocity v0(r), density rho0(r), and pressure p0(r). The entire information for the shock can be obtained easily by obtaining the numerical solutions to the set of ODEs.

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