A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration

Details A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59..239c&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 2, July 1977, p. 239-248.

Astronomy and Astrophysics

Astrophysics

9

Astronomical Models, Differential Equations, Heat Transfer, Solar Wind, Stellar Winds, Two Fluid Models, Algorithms, Asymptotic Methods, Boundary Value Problems, Critical Point, Numerical Integration, Stellar Models

Scientific paper

A complete numerical solution is obtained for the system of differential equations describing expansion of the stellar wind with heat transfer within the framework of the standard two-fluid solar wind model. The critical point (initial boundary) is numerically linked to the asymptotic range (outer boundary) using the shooting-splitting integration method described by Firnett and Troesch (1972). Results are consistent with asymptotic solutions proposed by Lucas (1973).

Affiliated with

Also associated with

No associations

Rating

A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A complete numerical solution of the two fluid solar wind model using the shooting-splitting method of integration will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1559321