Submitted:
29 July 2023
Posted:
02 August 2023
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Abstract
Keywords:
1. Introduction
Where there is minimal venting and structural containment (extreme confinement), an [explosion] of the HD 1.3 may occur with effects similar to those of an HD 1.1 explosion. For example, HD 1.3 AE is considered HD 1.1 (mass explosion) for QD purposes when stored in underground chambers.
2. Materials and Methods
- Obtain the max allowable heat flux from the burn time of the test and Equation 1,
- Estimate the factor in the point source model given the average heat flux data (assumed constant over the duration) at various distances by taking the 75th inclusive percentile of the values (the 75th percentile is used to better approximate the area of the curve where the allowable heat flux is expected),
- Using the point source model with the estimated factor and a view factor of 1, determine the ESSD that corresponds to the max allowable heat flux.
2.1. Example Unconfined Test Details
2.2. Modeling Details
2.2.1. Heat flux modeling details
2.2.2. Pressure and debris modeling details
3. Results
3.1. Comparison of ESSD to IBD for Unconfined Scenarios
3.2. ESSD for HD 1.3 Confined Scenarios
4. Discussion
5. Conclusions
Author Contributions
Funding
Data Availability Statement
Acknowledgments
Conflicts of Interest
Abbreviations
| mass of energetic substance, kilograms | |
| d | distance from substance, article, or structure, meters |
| t | time, seconds |
| q | heat flux, kilowatts per square meter |
| point source model parameter, kilowatts | |
| n | moles inside the structure |
| mass of substance, kg | |
| gas generation rate, mol/kg | |
| P | pressure, Pa |
| k | rate constant or atmospheric burn rate |
| H | enthalpy, J/mol |
| U | internal energy, J/mol |
| heat generation from afterburning, W |
References
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| Reference | Propellant Types | # of Tests | # of Measurements | Event Type |
|---|---|---|---|---|
| Hay J. E. et al. [6] | IMR5010, M1-8-SP, M1-8-MP, WC844, WC846, WCBlank | 49 | 206 | Unconfined: Heat Flux |
| Pape R. et al. [7] | M1, WC844 | 46 | 79 | Unconfined: Heat Flux |
| Wyssen [10] | GP11, 35mm prowder | 17 | 176 | Unconfined: Heat Flux |
| Paquet F. et al. [11] | SB1, SB2, DB1, DB2 | 16 | 48 | Unconfined: Heat Flux |
| Harmanny A. [9] | Fireworks | 16 | 16 | Unconfined: Heat Flux |
| Wyssen [12] | 20 mm powder | 6 | 120 | Unconfined: Heat Flux |
| Guymon C. G. [8] | WC814 | 1 | 4 | Unconfined: Heat Flux |
| Guymon C. G. [13] | Model | - | 30 | Unconfined: Heat Flux |
| Williams M. R. et al. [14] | MTV | 12 | 36 | Confined: Heat Flux |
| Trinkler [15] | Cordite | 8 | 35 | Confined: Heat Flux |
| Blankenhagel P. et al. [16] | di-tert-butyl peroxide | 3 | 9 | Confined: Heat Flux |
| Farmer et al. [3] | M1 | 3 | 3 | Confined: Heat Flux |
| Joachim C E [17] | M1 | 3 | 3 | Confined: Heat Flux |
| Allain L. [18] | LB 7 T 72 | 2 | 12 | Confined: Heat Flux |
| Titan Crane Failure [19] | Rocket Propellant | 1 | 1 | Confined: Heat Flux |
| Wilson et al. [20] | Rocket Propellant | 1 | 1 | Confined: Heat Flux |
| Farmer et al. [3] | M1 | 2 | 2 | Confined: Debris |
| Farmer et al. [21] | M1 | 1 | 2 | Confined: Debris |
| Wilson et al. [20] | Rocket Propellant | 1 | 1 | Confined: Debris |
| Guymon C. G. [5] | Model | - | 25 | Confined: Debris |
| Condition | Mass, M (kg) | Relation (m) |
|---|---|---|
| Unconfined | M ≤ 453 | min(3.216·M,22.9) |
| 453 < M ≤ 43,540 | max(22.9,exp[1.4715 + 0.2429·ln(M) + 0.00384·(ln(M))]) | |
| 43,540 < M ≤ 453,590 | exp[5.5938 – 0.5344·ln(M) + 0.04046·(ln(M))] | |
| 453,590 < M | 3.17·M | |
| Confined | M ≤ 10,000 | max(30.5,28.127-2.364·ln(M)+1.577·ln(M)) |
| 10,000 < M | 6.4·M |
| Condition | Mass, M (lb) | Relation (ft) |
|---|---|---|
| Unconfined | M ≤ 1,000 | min(7.73·M,75) |
| 1,000 < M ≤ 96,000 | max(75,exp[2.463 + 0.238·ln(M) + 0.00378·(ln(M))]) | |
| 96,000 < M ≤ 1,000,000 | exp[6.8633 – 0.5418·ln(M) + 0.03828·(ln(M))] | |
| 1,000,000 < M | 7.99·M | |
| Confined | M ≤ 22,050 | max(100,101.61-15.926·ln(M)+5.173·ln(M)) |
| 22,050 < M | 16.13·M |
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