Hot Surface Ignition

Undesirable hot surface ignition of flammable liquids is one of the hazards in ground and air transportation vehicles, which primarily occurs in the engine compartment. In order to evaluate the safety and sustainability of candidate replacement fuels with respect to hot surface ignition, a baseline low lead fuel (Avgas 100 LL) and four experimental unleaded aviation fuels recommended for reciprocating aviation engines were considered. In addition, hot surface ignition properties of the gas turbine fuels Jet-A, JP-8, and JP-5 were measured. A test apparatus capable of providing reproducible data was designed and fabricated to experimentally investigate the hot surface ignition characteristics. A uniform surface temperature stainless steel plate simulating the wall of a typical exhaust manifold of an aircraft engine was used as the hot surface. Temperature uniformity of ±5°C was achieved on the stainless steel plate by virtue of its being bolted to a copper plate in which five automatically controlled 1000 W electrical cartridge heaters were inserted. A programmable syringe pump was used to dispense ~25 μL fuel drops onto the hot surface. Testing was performed in a quiescent environment with the exception of a mild upward flow created by an exhaust fan aiding the buoyant plume created by the hot plate. Ignition and flame propagation events were recorded using visible and mid-infrared still and video imaging. The ignition and flame propagation events are transient and occur at randomly distributed locations on the hot surface. To characterize the ignition event statistically, the surface temperature leading to at least one ignition out of the number of drops and the surface temperature resulting in the ignition of all of the drops were recorded. The results of the experiment confirmed that the experimental variations in the drop size, drop velocity, plume characteristics, surface properties including temperature changes, and the nonlinear dependence of temperature of the chemical reaction rate lead to the probabilistic nature of the ignition event. The results of the experiment are of practical value in designing vehicular ignition and safety systems

Reactivity and Hypergolicity of Liquid and Solid Fuels with Mixed Oxides of Nitrogen

When combined with common fuel binders, solid hypergolic fuels can simplify the overall complexity of hybrid rocket systems, as the fuel grain can be ignited and reignited without an external power source or external fluid. In addition, with the hypergolic additive embedded in the binder, the flame zone can be placed at the surface of the grain itself, thereby providing heat to the fuel, improving fuel regression rate, and combustion stability and sustainability. Coupled with high grades of mixed oxides of nitrogen (MON), such hypergolically ignited hybrid configurations are considered a potential propulsion system for a robotic Mars Ascent Vehicle (MAV). Use of the fuel additives and a suitable choice of oxidizer allows for low temperature stability and operation of the propellants, making it an appealing candidate for a simple and storable hybrid propulsion system. The first half of this work is dedicated to a very application-based study of paraffin-based hypergolic hybrids, while the second half of this work, independent from the first, focuses on how theory could help in developing future hypergolic propulsion systems. The process undertaken to develop a paraffin-based hypergolic hybrid relied heavily on experimental testing of a wide variety of additive-loaded fuels with MON to optimize hybrid motor grain parameters with the goals of minimizing ignition delay, improving combustion stability, and promoting sustainment of the flame. MON-3 and MON-25 (3 wt.% or 25 wt.% nitric oxide mixed with nitrogen tetroxide) were used as oxidizers. Through an initial screening process, we selected two solid hypergolic propellants, sodium amide and potassium bis(trimethylsilyl)amide (PBTSA), as additives to promote hypergolic ignition given their low ignition delays with both grades of MON. Iterations on the grain configuration consisted in minimizing the additive loading to simplify the casting process and increase performance, without losing hypergolicity of the grain or hampering combustion sustainability. Using a 90 wt.% hypergolic additive front segment, we were able to light the grain three times using the hypergolic reaction between the additives and MON-3. Once relights achieved, we mainly focused on demonstrating sustained combustion, and determined that, once the front segment depleted, the lack of heat in the system lead the motor to shut down prior to the end of the targeted burn. This led us to add a reactive additive, sodium borohydride, in the main grain, as a way to generate heat in the motor once the front segment was depleted. With the objective of testing relevant conditions for an actual Mars Ascent Vehicle, one of our final tests was done in an altitude chamber, at a 100,000 ft targeted simulated altitude (equivalent to the atmospheric pressure on Mars), with MON-25 as the oxidizer. Using a mixture of sodium amide, PBTSA, and sodium borohydride, we were able to achieve hypergolic ignition in 425 ms (delay to reach 90% of the maximum chamber pressure) at 102,000 ft simulated altitude, for an average chamber pressure of 113 psia. During testing we determined that an ideal solid additive should exhibit both low ignition delay with the oxidizer considered, to minimize the motor start-up time, and a high heat of combustion, to maximize the energy release and therefore maximize performance. However, the lack of data and theoretical understanding of the reactivity of MONs with non-hydrazine-based fuels made it challenging to find such an ideal solid additive