CATALOG
MDCA GROUP/LIQUID FUEL/CFI
Cool Flames Investigation (CFI)
Prevention
Spacecraft cabinSpace stationSpacesuitAI summary
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Generated from the curated record only. The model is instructed not to invent numbers; verify all values against the source before engineering use.
Experimental setup
FUEL
- Phase
- Liquid
- Material
- Heptane droplets
- Shape
- Spherical droplets burned in a quiescent microgravity environment
- Size
- Millimeter-scale droplets
CONDITIONS
- O2 concentration
- Varied / not specified
- Pressure
- Varied / not specified
- Airflow
- Varied / not specified
Single values are documented test conditions, not flammability limits. Ranges appear under variables tested.
OBJECTIVES
Investigate the cool diffusion flames first observed during ISS droplet experiments in 2012, characterizing low-temperature burning and its role in near-limit extinction.
Sensors & measurements
- High-speed droplet and flame imaging
- Radiometers for low-level flame emission
- Droplet diameter tracking
- Combustion product and temperature diagnostics
Variables tested
- Low-temperature cool flame chemistry in heptane droplets
- Radiative extinction and near-limit burning
- Droplet burning history after the visible flame extinguishes
Key findings
- 01Cool diffusion flames were discovered during ISS droplet combustion experiments in 2012.
- 02CFI examined heptane droplet cool flames, which can burn at low temperature with little or no visible light.
- 03The data test low-temperature chemical kinetic models and help explain extinction near flammability limits.