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Abstract:
We used the GISS/Harvard/UCI3-D CTM on the AER computer platform to perform a number of simulations to obtain the surface area from accumulation of A12O3 particulates from solid rocket motors (SRM), orbital debris, and meteorites. In the calculation, the initial size distribution of the particulates emitted by SRM is represented by a tn-modal distribution with bulk density of 1.7 gm/cm. It is assumed that particles do not interact with each other so that particles in each size bin will evolve independently.
| Limitations: |
 APPROVED FOR PUBLIC RELEASE |
| Pages: |
43 |
| Report Date: |
30 SEP 1999 |
| Contract Number: |
F09603-95-D-0176-0007 |
| Report Number: |
A328314 |
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