Abstract

During re-entry of a spacecraft into the atmosphere of a celestial body, large amounts of energy are set free near the surface due to the high entry velocity. This energy leads to dissociation and ionization in the boundary layer and results in a high heat flux on the return body. These re-entry conditions must be simulated in ground test facilities to qualify for the necessary heat protection materials. For this purpose, several plasma wind tunnels were constructed at the Institut für Raumfahrtsysteme (IRS) of the University of Stuttgart and various plasma sources were developed to do justice to many qualification requirements for different missions, which will be presented in this paper.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.