The Reaction Research Society held its monthly meeting at the Compton/Woodley Airport location, 7:30 PM PST.
Agenda topics of the meeting were:
Wolfram launch 5/20
UCLA launch 6/10
It is with great pleasure that the Society declares the Symposium to have been a success. In all, there were 22 presenters present, and approximately 70 to 80 persons in attendance. Likewise, Mary Star High School has told us that they did well on their food service sales, and have already penciled us in to host the Symposium at their location again on April 8th, 2024.
However, there is much room for improvement. For example, we need to have better signage for the presentation room and food service at the next symposium. We could also take advantage of the large screens present in the gymnasium to keep attendees up to date on presentations. It was also noted that we should have a hard deadline for speakers to sign up, probably a few days in advance of the event, to prevent scheduling confusion. The older members of the Society are also in agreement that we should hire some of the students to help us setup and break down the Symposium. We could also Mary Star’s WiFi password, and maybe make it available upon request.
The Society was also pleased to receive a donation of eletrical match blanks from long-time RRS member, Steve Majdali. Our treasurer, Larry Hoffing, is to write a receipt for them.
Prior to the meeting, Society President Dave Nordling had new keys made for the newly opened MTA restrooms. Six pairs of keys were made, the gold one being to open the restroom proper, and the silver to open the container door to the valves and switches.
In regards to the restroom, it was mentioned that the society should probably hire someone to clean the restroom. In the past, society members have graciously handled cleaning and supplies themselves with the porta-potties, but there is a desire to have the restrooms taken care of by someone else. The main problem seems to be the cost of doing so, and how we might extract compensatory fees from anyone who uses the MTA and doesn’t clean up after themselves. A deposit was suggested, but Frank noted that getting such from a school would likely be a hassle.
Thanks to the Society’s generous donors, we are pleased to announce that a 60-foot launch rail for launching liquid rockets, and prefabbed containers for the MTA, have been funded. Polaris has a design for such a launch rail, and the Society is considering hiring them to build it. Also, in light of the struggles around building numerous projects at the MTA, it is expected that the Society will pay contractors to make improvements to the site mifor the forseeable future.
It’s also been recommended that the Society should have portable launch rails at the MTA. Being portable means that they can be moved away when might be necessary, such as if a group’s view of another launch rail is obstructed. Wolfram in particular has requested 1515 launch rails, but others, such as members of ROC, might appreciate these as well, due to the difference between our height waivers.
Steve Majdali mentioned at the meeting that he has 1,000 ft of duplex wire, 18 gauge solid core, which he might donate to the Society for our use. He also apparently has multi-strand, fine gauge wire, and might even have some sulfur to dispose of as well.
In other news, Society Treasurer Larry has received 3 lbs of 400-mesh zinc powder from a supplier in India. The zinc isn’t of the fineness typically used for micrograin rockets, but Larry will test its use regardless. It should be noted that the zinc was bought at $4 per pound, which is a very good deal, and we might consider sourcing from this supplier in the future. US-based suppliers are not as common today as they have been in decades past.
UCLA is currently scheduled to hold their Capstone project launch event at the MTA on June 10th. Likewise, Frank and Larry will simultaeneously be holding launch classes at the site. They will be having two launches, B and C motor model rockets, as well as Baby Bertha.
The Aerospace Corporation is also scheduled to use the MTA for their intern rocket launch event. As of now, there is no conflict on the MTA schedule with their event.
The Society is also receiving more requests for Vice-President Frank to teach more classes. Among past locations requesting his services is Nickerson Gardens.
Also, it has been noted that having underground cable runs between the launch rails and the Garboden Observation Bunker at the MTA would be very valuable. A pull string should be installed along with whatever conduit is put in place, and CAT9 wire should definitely be installed as a good starting point. This facility improvement needs further definition.
The next society meeting will be on June 9th, 2023, at the Compton/Woodley Airport location. Contact the secretary for details.
RRS member, Bill Claybaugh, built and launched his second 6-inch rocket from the RRS Mojave Test Area on Saturday, April 22, 2023. Target apogee was 69,000 feet. Winds were very low that day. Jim Gross was the pyrotechnic operator in charge for the launch event. Dimitri Timohovich and Rushd Julfiker assisted with the efforts. Bill launched from a 24-foot aluminum channel type launch rail using a pair of belly-bands that disconnected from the vehicle after clearing the end of the rail. The following is Bill’s report on the flight.
Six Inch Rocket, Fight II Flight Report
Something fairly violent happen to this vehicle at about 3.4 seconds into flight: onboard data and ground video indicate the rocket pitched at least 30 degrees while traveling at about Mach 2.2 at around 4100 feet above ground level (AGL).
Recovered hardware indicates the vehicle broke up under these conditions. The parachute compartment, which was attached to the top of the motor by four 1⁄4-20 fasteners, was torn away by fracture at all four fasteners (the fasteners remained attached to the motor). The payload, which was attached to the parachute compartment via four 0.250” diameter pneumatic separation system pins, remained attached—indeed, it was recovered with the separation system still functional and still latched to the top of the parachute compartment.
Video shows a sudden pitch at about 3.4 seconds after first vehicle motion. The onboard data (which records the initial part of the breakup because the computer was located in the payload section) shows that the gyro tilt went from about 5 degrees to 50 degrees over 0.08 seconds. Measured longitudinal acceleration went from the previous around 26 g’s to 34 g’s in 0.05 seconds, and after returning to around 24 g’s for 0.15 seconds, to -12.7 g’s (the sensor floor) for 0.03 seconds, before recovering to -9 g’s for 0.01 seconds followed by loss of power. (See Chart 1.)
Video shows the vehicle recovering from this pitch maneuver and continuing on a near vertical ascent though burnout at about 6.1 seconds after first motion.
Following failure of the AlClO (Aluminum (III) Chloride Oxide) based head end initiator to successfully ignite the rocket (AlClO based initiators have had this issue previously, AlClO appears to be too energetic for this application, tending to blow the secondary ignition materials out the back of the rocket and on to the ground rather than igniting the grain) a jury-rigged rear end ignitor was substituted and the rocket successfully lifted off about 0.25 seconds after flames first appeared around the vehicle base.
On board data shows the vehicle ascending at about 88 degrees from horizontal to about 50 feet altitude when a lazy “S” turn (first to the northeast, then back to the southwest) is visible in the video and data. This turn starts about the time the belly-bands can be seen on video falling away from the vehicle, however, the second half of this “S” turn cannot be explained by interference from the belly-bands as they are well away from the vehicle when this second turn occurs.
Following this maneuver, the vehicle returns to near vertical flight to the Southwest, turning, with perturbations, from about 88 degrees tilt to an 86-degree gyro tilt over the next two-plus seconds. Acceleration steadily builds from an initial 15.1 g’s at first motion to a maximum of 27.3 g’s at 2.53 seconds; this acceleration broadly follows the curve expected from the combination of the thrust curve and the lessening weight of the vehicle as propellant is consumed, however, the measured acceleration is much higher than expected based on static tests and flight simulations.
Telemetry reported Loss of Signal (LOS) at 2.7 seconds and at an (accelerometer-based) 2313 feet altitude and 2440 ft/sec velocity.
Measured onboard acceleration suddenly jumps from a base around 26.5 g’s at 3.18 seconds to 32.8 g’s at 3.21 seconds; measured onboard acceleration stays above 30g’s for the next 0.06 seconds, peaking at 34.7 g’s at 3.21 seconds and followed by a return to around 24 g’s for 0.15 seconds and a sudden drop to -12.7 g’s (the sensor floor) from 3.42 to 3.44 seconds and a final reading of -9.3 g’s followed by loss of power to the on-board computer.
Onboard data shows the gyro tilt angle moving from around 5 degrees at 3.37 seconds to 50.6 degrees at 3.45 seconds, followed by loss of power.
Video over this period show the vehicle suddenly turning through an apparent (visual) 30 degrees or so before pitching back to a near vertical ascent.
A less energetic initiator is required for this vehicle; a development program will be initiated to achieve both a more reliable and a gentler ignition in future.
Following flight, a single sliver of graphite was found on the ground about 150 feet from the launch tower. This piece of graphite was exactly the correct shape to fit at the very rear of the graphite throat insert where that insert blends into the Titanium nozzle extension.
Recovered nozzle hardware showed that about 1” of the rear of the nozzle insert was missing (see Image 1); assuming the two pieces of the insert found inside the rocket were broken by impact forces, it follows that around one inch at the rear of the insert failed prior to impact. This failure would have induced a flow discontinuity in the rocket’s exhaust which thrust vector could account for the two “S” turns seen in video and in the on-board data. Vehicle roll rate was around 60 degrees per second at this point, which appears consistent with the timing of this maneuver; gyro pitch and yaw data confirm this was an initial perturbation that rolled around the vehicle before straightening. Why the vehicle returned to near vertical ascent is not clear from the data.
Note that the recovered nozzle shows plating of Aluminum Oxide onto the zirconium oxide (ZrO) coated titanium (Ti) nozzle extension above the end of the graphite nozzle extension but not in the area originally covered by the graphite insert. This suggests the insert was present during startup (when Aluminum Oxide would be expected to condense on the nozzle extension surface) and the loss of the about 1” of the bottom of the graphite nozzle insert must have occurred later.
Loss of telemetry at 2.7 seconds appears to be a consequence of the GPS and transmitter antenna assembly failing mechanically; the flight computer was recovered with a clean break at the antenna PCB board. This suggests the need for more robust support of these parts of the payload.
Breakup of the vehicle began about 3.41 seconds after launch. The recovered pieces indicate separation of the parachute compartment from the motor was due to the upper part of the vehicle being pulled longitudinally forward, away from the (thrusting) rocket motor; further, the fracture pattern indicates an abrupt failure rather than a slightly slower swaging of the metal. Based on the acceleration data indicating at least four hundredths of a second of significant negative g’s just before loss of power, coupled with gyro data showing the payload being thrown through an about 45 degree turn over the last 0.08 seconds of data, we can guess that the mechanical failure was a consequence of rather than the cause of the sudden turn of the vehicle. It remains uncertain what caused that turn, but a partial nozzle failure associated with the missing rear of the graphite nozzle insert appears the most probable cause.
Development of a gentler and more consistent initiator is required; an effort focused on BKNO3/V (Potassium Nitrate with Boron held in a Viton matrix) has been started.
The vehicle nozzle has been redesigned to use a single piece Titanium throat insert support structure and nozzle extension. The angle of the joint between the graphite insert and the Titanium shell has been increased to the conventional 5 degrees. The flight nozzle used a 3- degree angle that may have been too thin at the very end of the throat insert.
Heat paint testing of the Titanium nozzle extension on the flight nozzle indicated a maximum heat soak temperature of about 800 degrees Fahrenheit on the outside surface; this is well below the maximum working temperature of 6Al-4V Titanium alloy under these loads and the new nozzle is accordingly designed to allow for greater heating of the shell.
Analysis based on the maximum Ti temperature of about 800 F indicates a maximum possible temperature of about 1200 degrees at the ZrO / Ti interface and about 2150 F at the inside surface of the graphite insert, implying a surface temperature at the nozzle throat of about 4500 F. A similar analysis indicates a maximum possible temperature at the inside surface of the nozzle exit of about 2300 F.
The above temperatures suggest a maximum thermal expansion of the graphite at the nozzle throat of about 0.012” assuming an average temperature of 3325 F. Note that if thermal expansion of the nozzle throat was at 0.012”, one half of that would have been in the radial direction of the throat surface, but the same thing would be happening at the opposite side of the throat. Therefore the actual throat diameter during firing would be about 1.488” rather than the machined 1.500”; simulation indicates this would have increased chamber pressure for this propellant and grain design from an estimated 635 psia to about 670 psia but this increase is far too little to explain the apparent 125% higher than expected thrust on this flight.
The high temperature RTV layer between the graphite insert and the ZrO layer was originally 0.005” in thickness in two sections separated by a 0.030” cork layer (a total of 0.010” of RTV); it thus may not have had sufficient space, after pyrolysis of that layer, to accommodate the thermal expansion of the Graphite Nozzle Insert although the cork layer does appear to have had sufficient additional spacing to allow for that expansion.
The payload internal fiberglass support structure for the flight computer failed both at the base and at the antennae. This structure will be redesigned in aluminum so as to provide even more robust support to the flight computer assembly. Making this change will reduce the sensitivity of the GPS antenna and will absorb some of the transmitted energy from the telemetry antenna which was the reason for going with fiberglass previously. The effects of lower sensitivity will have to documented once that hardware is available and assembled.
The measured in-flight acceleration is significantly higher than that expected from static testing and modeling of the flight trajectory; further, the burn time indicated from video is about 75% of that demonstrated in the previous static test and acceleration about 125% of expected value. Before another flight is attempted, a flight configuration static test with the new nozzle design will be performed to try an reconcile the on-board data to the demonstrated in-flight performance of the motor.
Strengthening the joint between the motor and the parachute compartment is relatively easy. Additional fasteners and a thicker section to the joint should reduce the probability of a failure similar to that which occurred on this flight. Alternatively, the motor tube could be extended by six inches to avoid having a separate parachute compartment altogether, albeit with some induced operational inconvenience when placing the initiator into the forward bulkhead.
Partial nozzle failure appears to be the main concern with this vehicle design; a secondary issue is strengthening internal components and some joints to better survive the extremely harsh conditions encountered on this flight.
After a three week testing period, the Reaction Research Society is pleased to announce that the containerized restroom facility is ready for use by our guests and members. Several modifications and improvements were made which have been demonstrated sufficiently. This project has been a few years in the making but well worth the effort.
The electrical, water and sewage systems in both rooms are in working order which means sinks, urinals and flushing toilets are ready for our next event. Some of the interior fixtures are still in work. The interior shower, hot water system and external safety shower are coming soon.
This much-requested and much-desired infrastructure upgrade was built by the hard work of several members over many weekends in all seasons over a couple years. We have many to thank including Dimitri Timohovich, Osvaldo Tarditti, Waldo Stakes, Dave Nordling, Keith Yoerg, Joe Dominguez, Bill Inman, Manuel Marquez, Wilbur Owens and Larry Hoffing,
There’s still more work to go including the floors, shower and hot water system, but we do want to recognize this milestone in our campaign to upgrade our facilities for our membership and our invited guests. Our pit toilet will remain as a backup but many will appreciate a little modern convenience in our remote location.