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Effects of precursor heating on chemical and radiation nonequilibrium viscous flow around a jovian entry body
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Szema, K. Y. Tiwari, S. N. |
| Copyright Year | 1978 |
| Description | The influence of precursor heating on viscous chemical nonequilibrium radiating flow around a Jovian entry body is investigated. Results obtained for a 45-degree hyperboloid blunt body entering Jupiter's nominal atmosphere at zero angle of attack indicate that the nonequilibrium radiative heating rate is significantly higher than the corresponding equilibrium heating. The precursor heating, in general, increases the radiative and convective heating to the body, and this increase is slightly higher for the nonequilibrium conditions. |
| File Size | 1580228 |
| Page Count | 55 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19790009713 |
| Archival Resource Key | ark:/13960/t77t2h46t |
| Language | English |
| Publisher Date | 1978-12-01 |
| Access Restriction | Open |
| Subject Keyword | Astrodynamics Convective Heat Transfer Nonequilibrium Flow Jupiter Atmosphere Chemical Reactions Blunt Bodies Angle of Attack Atmospheric Entry Radiative Heat Transfer Viscous Flow Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
