Virtual Jets: From Self-Similar to Numerical Solutions

Details Virtual Jets: From Self-Similar to Numerical Solutions Virtual Jets: From Self-Similar to Numerical Solutions

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.293...83f&link_type=abstract

Astrophysics and Space Science, v. 293, Issue 1, p. 83-90 (2004).

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The goal of this contribution is not to describe results on accretion discs launching jets obtained within the self-similar framework. Rather, I would like (1) to emphasize the huge difficulties one has to face when attempting to perform magnetohydrodynamic (MHD) numerical simulations of such discs; (2) to show how self-similar solutions can help to solve these difficulties. In particular, they allow to choose suitable boundary conditions and/or relevant initial conditions. In all cases anyway, they provide a framework for understanding and testing the outcome of numerical simulations.

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