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Background
Coflow
laminar diffusion flames (as shown schematically on the left) are
especially valuable for studies of combustion because of the availability
of accurate numerical modeling with that flame configuration. In
particular, excellent agreement can be achieved when the flow conditions
are such that the flame detaches and lifts above (i.e., moves downstream
of) the nozzle. A coupled experimental and numerical investigation
can enable validation and improvements to combustion modeling. For
example, the image to the right is not a photo, but a numerical simulation
of a 40% ethylene flame. Enhanced modeling capability is important
because it can reduce time and cost in the design of practical combustion
devices. Furthermore, flame attachment to (or detachment from)
a burner or condensed-fuel surface is of essential importance in both
combustion systems and fire safety. The flame attachment point
controls the stability of the entire trailing diffusion flame.
Microgravity testing allows for greater temporal
and spatial scales and a broader range of flame characteristics
than can be achieved in normal gravity. As one example of
the NASA-recognized value of such studies, the Coflow Laminar Diffusion
Flame (CLD Flame) experiment of Marshall B. Long and Mitchell D.
Smooke (both of Yale U.) is currently in development for conduct
in the Combustion Integrated Rack (CIR) on the International Space
Station, as part of the Advanced Combustion via Microgravity Experiments
(ACME) project.
The overall goal of the proposed study is to
improve our understanding of the physical and chemical processes
controlling diffusion (i.e., non-premixed) flame structure and lifting
phenomena (i.e., stabilization) and to provide for rigorous testing
of numerical models, including thermal radiation, soot formation,
and detailed chemical kinetics. As
part of this aim, an important purpose of the SLICE investigation
is to conduct preliminary microgravity studies that will maximize
the scientific return of the subsequent CLD Flame experiment and mitigate
associated risks. In other words, SLICE is a precursor
to the CLD Flame experiment.
Objectives
- Identify the lift-off velocity limits in
air for flames of methane, ethylene, and selected dilutions of
each fuel as a function of the nozzle size. When possible,
also identify the blow-out velocities (i.e., when the flame extinguishes). This
will enable refinement of the CLD Flame test matrix where the fuels
for that experiment are those specified here.
- Characterize
the hysteresis of flame lifting and reattachment (i.e., stabilization)
with variations in flow conditions as a function of the fuel and
nozzle size. This will enable further refinement of the CLD Flame
test matrix.
- Characterize
the structure of the lifted flame as a function of the fuel, nozzle
size, and flow conditions. This will enable refinement of the
flame diagnostic settings and test matrix for the CLD Flame experiment. It
will also allow for a preliminary assessment of the numerical codes’ ability
to predict the flame structure under the broader conditions which
are only found in microgravity flames.
- Characterize the structure
of the flame, and especially its base (i.e., stabilizing region),
from attached through lifted conditions as a function of the fuel,
nozzle size, and flow conditions. This
will enable rigorous testing of numerical models beyond that planned
for the CLD Flame experiment, extending capabilities to incorporate
burner heat loss.
Approach
The
experimental hardware for the Smoke Points In Co-flow Experiment (SPICE),
of David L. Urban (NASA Glenn) and Peter B. Sunderland (U. Maryland),
which is currently onboard the International Space Station, was built
to allow studies of coflow laminar diffusion flames. The SPICE
hardware is within the ISS MSG in the image to the right. While
the SPICE investigation has been specifically focused on a study of
soot production and oxidation within flames, the hardware can be used
without modification to conduct the SLICE experiment. In terms
of the experimental hardware, the only additional requirements for
SLICE are more fuel (i.e., gas bottles), recording media, and minor
hardware elements such as new nozzle(s). The three existing
SPICE nozzles are all smaller than the nozzle planned for the CLD
Flame experiment. Of course, the SLICE testing could most benefit
the CLD Flame experiment by bracketing and/or including the same nozzle
size. It is also possible that screen(s) would be flown to alter
the velocity profile of the coflow.
The SLICE operating procedures will have some
differences to the standard SPICE procedures given the differing
objectives. However,
those changes are fully within the capabilities of the SPICE hardware,
as demonstrated by exploratory testing that has already been conducted
on orbit. As a simple example, the standard SPICE procedure
calls for a fixed air velocity and an increase of the fuel flow until
the smoke point is reached. In contrast, SLICE will include
testing where the fuel flow is fixed and the air velocity is incrementally
increased until the diffusion flame detaches and lifts off from the
nozzle. In all cases, still and video measurements of the flame
structure will be made for comparison with detailed numerical computations. Given
that the capture of the lifting processes in normal gravity is extremely
difficult, SLICE will provide valuable photographic observations on
the transient flame behavior.
The lifted nature of the flames can be discerned from the flame
shape in the example images (which are not at the same scale) and
the distance from the nozzle tip (which is not visible). While the
case(s) on the left may look similar to attached flames, the outward
fuel-lean flare of each flame’s base reveals it’s lifted nature.
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