A proposed solution for test case one using the SESAM code

Details A proposed solution for test case one using the SESAM code A proposed solution for test case one using the SESAM code

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.533..121l&link_type=abstract

In: Proceedings of the First International Workshop on Radiation of High Temperature Gases in Atmospheric Entry, 8-10 October 20

Physics

1

Space Probes, Planetary Atmospheres: Entry, Simulations

Scientific paper

The line-by-line spectral code SESAM used for the simulation of the radiative emission of entry-type plasmas is presented in this paper and applied to the simulation of the measured radiative spectrum proposed as test-case 1 defined in the workshop. A good overall agreement between simulation and experience is achieved. However, some minor differences arise in specific regions of the spectrum. These can be attributed partly to calibration errors in the experimental spectrum, but also to a lesser accuracy of the numerical code concerning the NO bands in the near-UV region.

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