The modeling of spacecraft glow surrounding a small clean satellite is discussed. A direct simulation Monte Carlo (DSMC) technique was used to model the flowfield and included both surface and gas-phase chemical reactions. It has been suggested that emission from excited NO2 molecules produces the spacecraft glow. The DSMC calculations included chemical reactions in the flowfield to produce NO, as well as surface chemical reactions to generate the NO2. The orbit-dependent optical radiation was calculated and compared with data from the Atmosphere Explorer experiment over the 140-200-km altitude range. The results show that the surface model can account for the observed data in magnitude and altitude dependence for suitable choices of the surface heat of absorption and freestream NO concentration.
|Original language||English (US)|
|Number of pages||10|
|State||Published - Apr 1999|
ASJC Scopus subject areas
- Aerospace Engineering