Abstract
Aluminum agglomeration and agglomerate sizes of NEPE propellants were studied by cinephotomicrography at pressures of 3 and 5 MPa. Accumulation, aggregation, and agglomeration of aluminum particles similar to that at pressures below 1 MPa were observed. Coalescence of two agglomerates on the burning surface is obtained for the first time. A decrease in the burning rate from 8 to 5 mm s−1 leads to about 20 % increase in the agglomerate diameter. The pressure is found to have no direct influence on the agglomerate diameter when the burning rate is kept constant. The evolution of the agglomerate diameter according to the increase of the virgin aluminum size from 16 to 36 μm is convex in shape and reached its maximum at a particle diameter of 29 μm. Increasing the amount of RDX crystals added in the propellants causes a larger agglomerate diameter. The experimental mass average agglomerate diameters were compared with various agglomeration models. It is found that Hermsen and Salita empirical models have a higher accuracy for NEPE propellants rather than Becksted, Liu, or pocket models.
| Original language | English |
|---|---|
| Pages (from-to) | 260-268 |
| Number of pages | 9 |
| Journal | Propellants, Explosives, Pyrotechnics |
| Volume | 42 |
| Issue number | 3 |
| DOIs | |
| State | Published - 1 Mar 2017 |
Keywords
- Agglomerate diameter
- Agglomeration
- Agglomeration models
- Aluminum particle
- NEPE propellants
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