Advanced Combustion via
Microgravity Experiments (ACME)
ACME is now under development with a set of five independent experiments
which are each focused on advancing combustion technology through
fundamental research. Four of the current ACME experiments
are specifically directed at addressing energy and environmental
concerns, while the fifth experiment addresses fire prevention,
especially for spacecraft. The overall goals are to improve
our understanding of materials flammability, combustion at fuel
lean conditions where both optimum performance and low emissions
can be achieved, flame stability and extinction limits, soot control
and reduction, oxygen-enriched combustion which could enable practical
carbon sequestration, and the use of electric fields for combustion
control.
With the exception of the Burning Rate Emulator (BRE) experiment
discussed immediately below, the general goal of the current ACME
experiments is to gain fundamental understanding that can enable improved
efficiency and reduced emissions in practical combustion processes
on Earth, for example through the development and verification of
models for chemical kinetics and transport processes in computational
simulations. In addition to enhanced performance, improved modeling
capability can lead to reductions in the time and cost for combustor
design. In summary, microgravity investigations of non-premixed
flames could lead to eco-friendly combustion systems providing our
nation with green power for the future.
Burning Rate Emulator (BRE)
Image of a normal-gravity
flame ext- ending from a flat burner facing downward at
an angle. In this conceptual test, a liquid fuel is being
burned with a porous wicking burner.
Unlike the other current ACME experiments, the Burning Rate
Emulator (BRE) experiment is focused on fire prevention, especially
in spacecraft. Specifically, BRE’s objective is
to improve our fundamental understanding of materials flammability,
such as ignition and extinction behavior, and assess the relevance
of existing flammability test methods for low and partial-gravity
environments. The burning of solid and liquid fuels will
be simulated by using a flat porous burner fed with gaseous
fuel. The fuel flow rate will be controlled based on the
measured heat flux (at the burner) and surface temperature,
mimicking the dependence of condensed-phase fuel vaporization
on thermal feedback. A small number of gaseous fuels will
be used to simulate the burning of fuels such as paper, plastic,
and alcohol by matching properties such as the surface temperature
and smoke production.
BRE Aircraft Rig Video
Initial Drop Tower Tests of
the BRE Aircraft Rig
April 18, 2012: This video shows the initial drop
tower tests of the BRE Aircraft Rig. The rig has been
designed and built to test the Burning Rate Emulator experiment
concept, one of five major experiments that are planned
for the Advanced Combustion via Microgravity Experiments
(ACME) suite of investigations to be conducted on the International
Space Station in 2016 and 2017. BRE will study and
characterize ignition and flammability of solid spacecraft
materials using a gaseous analog. In the video, the
BRE rig is burning ethanol. The flame is allowed to
burn for a few seconds in 1-g and then it is dropped in
a drop tower which provides reduced gravity. The drop
start is clearly evident as the flame shape changes. The
flame leans to one side (perhaps residual air flow from
the retraction of the igniter) and flashes a couple times. There
are some particle tracers which seem to indicate the general
flow direction from right to left. The flame goes
out at impact. The rig will next be loaded into a
modified Boeing 727-200 aircraft in late April 2012 for
extended parabolic flights that will provide longer periods
of reduced gravity, up to approximately 20 seconds.
Coflow Laminar Diffusion Flame (CLD Flame)
Image of a lifted flame of 50%
propylene in a coflow of air (at ambient pressure) from
an ex-ploratory test conducted on the International Space
Station in 2009 as part of the Smoke Point In Coflow Experiment
(SPICE).
Research, especially including that already conducted in microgravity,
has revealed that our current predictive ability is significantly
lacking for flames at the extremes of fuel dilution, namely for
sooty pure-fuel flames and dilute flames that are near extinction. The
general goal of the Coflow Laminar Diffusion Flame (CLD Flame)
experiment is to extend the range of flame conditions that can
be accurately predicted by developing and experimentally verifying
chemical kinetic and soot formation submodels. The dependence
of normal coflow flames on injection velocity and fuel dilution
will be carefully examined for flames at both very dilute and
highly sooting conditions. Measurements will be made of
the structure of diluted methane and ethylene flames in an air
coflow. Lifted flames will be used as the basis for the
research to avoid flame dependence on heat loss to the burner. The
results of this experiment will be directly applicable to practical
combustion issues such as turbulent combustion, ignition, flame
stability, and more.
Electric-Field Effects on Laminar Diffusion
Flames (E-FIELD Flames)
Image of a gas-jet diffusion
flame (in air at ambient pressure) from a test conducted
in NASA's 2.2 Second Drop Tower. The flame is being forced
downward by the electric field between the burner and an
electrode mesh, which is at +2 kilovolts and is down-stream
of the burner.
Electric fields can strongly influence flames because of its
effect on the ions present as a result of the combustion reactions. The
direct ion transport and the induced ion wind can modify the
flame shape, alter the soot or flammability limits, direct heat
transfer, and reduce pollutant emission. The purpose
of the Electric-Field Effects on Laminar Diffusion Flames (E-FIELD
Flames) experiment is to gain an improved understanding of flame
ion production and investigate how the ions can be used to control
non-premixed flames. Outside reviewers recently concluded
that the experiment “… will contribute to our critical
understanding to our knowledge of combustion processes in the
presence of electric fields.” The experiment will
be conducted with a normal coflow flame (as in the CLD Flame
experiment) or perhaps with a simple gas-jet flame, where there
is no surrounding coflow. An electric field will be generated
by creating a high voltage (up to 10 kV) differential between
the burner and a flat circular mesh suspended above (i.e., downstream
of) the burner. Measurements, as a function of field strength
and fuel dilution, will be made of the ion current through the
flame and the flame’s response time to electric forcing.
Flame Design
Image of a spherical diffusion
flame on a porous burner (which is also visible) at the
end of a test conducted in NASA’s 2.2 Second Drop
Tower. From the burner, there was 1.51 mg/s of 100% ethylene
flowing into air at atmospheric pressure.
The primary goal of the Flame Design experiment is to improve
our understanding of soot inception and control in order to
enable the optimization of oxygen enriched combustion and the “design” of
non-premixed flames that are both robust and soot free. An
outside review panel recently declared that Flame Design “… could
lead to greatly improved burner designs that are efficient and
less polluting than current designs." Flame Design
will investigate the soot inception and extinction limits of
spherical microgravity flames, created in the same manner as
for the s-Flame experiment. Tests will be conducted with
various concentrations of both the injected fuel (i.e., ethylene
or methane) and the oxygen enriched atmosphere in order to determine
the role of the flame structure on soot inception. The
effect of the flow direction on soot formation will be assessed
with an inverse spherical flame unless such testing is not approved
by the Payload Safety Review Panel (PSRP). If inverse
spherical flame testing is not allowed, the plan is to use a
coflow burner, conducting both normal and inverse flame tests. In
the case of the inverse flames, the oxygen/inert mixture is
injected from a central tube, while the fuel is ejected from
a surrounding annulus. The Flame Design experiment will
explore whether the stoichiometric mixture fraction can characterize
soot and flammability limits for non-premixed flames like the
equivalence ratio serves as an indicator of those limits for
premixed flames.
Structure and Response of Spherical Diffusion
Flames (s-Flame)
Image of a partially-premixed
spher-ical flame on a porous burner (which is also visible).
The microgravity test was conducted in a NASA drop facility.
The gas issuing from the burner was 25% propane, 2% oxygen,
49% argon, and 24% nitrogen.
The purpose of the Spherical Flame (s-Flame) experiment is to
advance our ability to predict the structure and dynamics, including
extinction, of both soot-free and sooty flames. The spherical
flame, which is only possible in microgravity, will be created
through use of a porous spherical burner from which a fuel/inert
gas mixture will issue into the CIR chamber. Flames will
be ignited at non-steady conditions and allowed to transition
naturally toward extinction. Tests will be conducted with
various inert diluents, in both the fuel and chamber atmosphere. The
fuel gases include hydrogen and methane for soot-free flames,
and ethylene for sooty flames. One experiment objective
is to identify the extinction limits for both radiative and convective
extinction (i.e., at high and low system Damkohler numbers, respectively). Another
objective is to determine the existence, onset, and nature of
pulsating instabilities that have been theoretically predicted
to occur in such flames with fuel/diluent mixtures that are above
a critical Lewis number.
ACME Status
February
2013 – Preparations are underway to conduct
evaluation tests for the Burning Rate Emulator (BRE)
experiment in NASA Glenn’s Zero
Gravity Research Facility using a prototype burner developed
by the University of Maryland investigators, Profs. Jim
Quintiere and Peter
Sunderland. This follows forty exploratory tests that
were conducted with a similar gas-fueled burner in November 2012
in NASA Glenn’s 2.2
Second Drop Tower. In each drop facility, apparent weightlessness
is momentarily achieved by letting the self-contained experiment
freely fall down a vertical shaft. The November tests were
conducted in ambient air and sometimes revealed lifting phenomena
and possible tip quenching when the fuel was methane or diluted
methane. Meanwhile, the ethylene flames remained robust throughout
the 2.2-second test duration. The “cup” burner
used in the November tests was equipped with a heater, where its
use had a significant effect on the ethylene flame as can be seen
in the sample images below.
October 2012 – Detailed design is underway, where
ACME passed an interim design review in June. A successful
Science Concept Review was held for the Burning Rate Emulator (BRE)
experiment in August, where the external reviewers concluded that
BRE “may offer critical guidance in flammability assessment
in space vehicles.” The Requirements Definition Review
for BRE and the Critical Design Review for ACME are planned for
June and November 2013, respectively. The extra reviews are
necessary for BRE because it wasn’t originally an ACME experiment
and its design isn’t yet fully specified. It is currently
expected that ACME will begin testing on ISS in 2016.
April 2012 – Tests were recently completed on
the International Space Station for the Structure & Liftoff
In Combustion Experiment (SLICE)
which is a precursor to ACME’s Coflow Laminar Diffusion Flame
(CLD Flame) experiment. The SLICE results will enable refinement
of the CLD Flame test matrix and operating procedures so as to maximize
its scientific outcome. You can learn more about SLICE at
its Facebook page.
January 2012 – A fifth experiment was added to the
ACME project, Burning Rate Emulator (BRE), where the investigators
are Profs. J.G. Quintiere and P.B. Sunderland of the University
of Maryland. BRE’s objective is to improve our fundamental
understanding of materials flammability and assess the relevance
of existing flammability test methods for low and partial-gravity
environments. The burning of solid and liquid fuels will be
simulated using a flat porous burner, where the flow rate of gaseous
fuel will be controlled based on the thermal feedback to the burner.
January 2011 - The Advanced Combustion via Microgravity
Experiments (ACME) Preliminary Design Review (PDR) was held on January
28, 2011. The Project team demonstrated that the preliminary
design meets all system requirements with acceptable risk and within
cost and schedule constraints. The review board has recommended
that the project proceed with detailed design.
May 2010 - The Advanced Combustion via Microgravity
Experiments (ACME) Requirements Definition Review (RDR) was held
for two days, May 10-11, 2010 The Science Requirements Document
(SRD) was signed by all parties except for one PI who had to leave
early before the signature page was prepared.
August 2009 - The ACME project is conducting drop tower
testing at the Glenn Research Center’s 2.2 second drop tower
with the ACME E-Fields rig. The drop tower tests are focusing
on the high voltage field effects on flames, these tests were conducted
during the month of July 2009 by the project scientist and summer
intern.
Objective
Modular apparatus designed for gaseous fuel investigations
to study:
combustion structure and stability near flammability
limits,
soot inception, surface growth, and oxidation processes,
emission reduction through nitrogen exchange,
combustion stability enhancements via an electric
field.
Relevance/Impact
Verified computational models that will enable
the design of high efficiency, low emission combustors operating
at near-limit conditions.
Reduced design costs due to improved capabilities
to numerically simulate combustion processes.
Efficient soot control strategies for industrial
applications.
Development Approach
Flight design leverages off previous flight design
heritage.
Multi-user, re-usable apparatus minimizing up-mass/volume,
costs, and crew involvement.
Four flame designs to be studied by ACME
Combustion Integrated Rack (CIR)
Structure and Response of Spherical Diffusion
Flames (s-Flame) Principal Investigaotor: Prof. C. K.
Law, Princeton University Co-Investigators: Prof. Stephen Tse,
Rutgers U.
Dr. Kurt Sacksteder, NASA GRC
Flame Design Principal Investigaotor: Prof. Richard
Axelbaum, Washington University, St. Louis Co-Investigators: Prof. Beei-Huan Chao,
U. Hawaii
Prof. Peter Sunderland, U. Maryland
Dr. David Urban, NASA GRC
Coflow Laminar Diffusion Flame (CLD Flame) Principal Investigaotor: Prof. Marshall
Long, Yale University Co-Investigators: Prof. Mitchell Smooke,
Yale University
Electric-Field Effects on Laminar Diffusion
Flames (E-FIELD Flames) Principal Investigaotor: Prof. Derek
Dunn-Rankin, UC Urvine Co-Investigators: Prof. Felix Weinberg,
Imperial College, London
Dr. Zeng-Guang Yuan, NCSER/GRC
Burning Rate Emulator (BRE) Principal Investigator: Prof. James
Quintiere, U. Maryland Co-Investigator: Prof. Peter Sunderland,
U. Maryland
Project Scientists:Dennis
Stocker, NASA GRC 216-433-2166