UhClem
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I have never heard of the NAR imposing this requirement. Is this documented anywhere?In the US, angle lockouts are required by both NAR & TRA for multi-stage flights.
I have never heard of the NAR imposing this requirement. Is this documented anywhere?In the US, angle lockouts are required by both NAR & TRA for multi-stage flights.
Long ago I read the data sheet for the AD623 instrumentation amplifier which has a nice section on EMI. RF gets into the input and causes trouble. The solution is to keep RF out via some RC input filters.I figured out it was the sensor and not the traces when I didn't see the same effect in the IMU. For whatever reason it seems to affect some ADCs and not others. I get the same interference problem when I sample the MCU ADC for the Teensy3.5.
The statement I made was incorrect. When this was being considered, there wasn't sufficient technology available to HPR fliers to make it a requirement.I have never heard of the NAR imposing this requirement. Is this documented anywhere?
For my 32KSPS Teensy 3.6 logger I found that I had just enough time to handle the SPI transfer in an assembly language interrupt service routine.
I really should have used DMA but that looked like a big can of worms best left unopened.
One of the little details of the MPU9250 is that you can use a higher SPI clock frequency when accessing the data registers. 20MHz vs. 1MHz. Which really speeds things up.If I can get the sensors on my next board to use the SPI bus, then I may try this library out. That would dramatically free up processing time.
Yes. The optical relays are for the pyros (Omron G3VM-31AR). I've got one for arming/safety, four pyros, and the last one is to switch my camera on/off (overkill for that purpose). These are beefy 4 amp relays. I prefer the optical relays for the extra layer of isolation (vs transistor or mosfet), but I am no electrical engineer (but I did stay in a Holiday Inn last night). I also have a 3.5 amp auto-resetting fuse in-line. My tests of e-matches show MJG's consistently fire under about 1/2 an amp, while the cheap "orangies" take up to 2.5 amps or more. My fear is firing a pyro with a hard short, so I designed and tested to make sure an accidental short on a pyro didn't screw anything else up on the board when it fired.1. It looks like you have a row of optos on your board. Are you using those for deployment or are there a set of transistors I don't see?
That is a novel idea, but I'm not sure if it would be accurate under different flight profiles. I'd have to do the math or run scenarios. Yesterday, our new quaternion tilt routine worked perfect. We took off the pad at 2 degrees and twenty seconds in we were only at 5 degrees. At apogee we could see the turn over and subsequent tumbles. We could also see perfect spin/roll data on the way up. So, I'm pretty happy with using it as our tilt lock-out.3. Off axis detection / lockout. I have done this by comparing barometric altitude with the integrated accelerometer values with the thought that some large difference means that the rocket is not moving in line with vertical.
Yep. I need to order some Lora radios and run the same tests. I see a lot of advantages.4. I still maintain that there is a 10db advantage of LORA over the standard GFSK modulation schemes.
The flight yesterday is not the best dataset, as we switched velocity/altitude integration over to the 32G accelerometer and it maxed out in the first 1.5 seconds. Also, due to the very high G's the GPS did not come back online until it dropped 3-4K feet from apogee. that said, below is data from the previous flight. My accelerometer altitude also runs ahead or "hot" from the barometer. Intuitively that makes sense, as the barometer takes longer to sense/adjust, but even with that consideration it does seem like the accelerometer is always "more generous" with altitude. After apogee, the accelerometer data is useless. The GPS and the barometer tend to track very close, but the GPS is only working in "low speed" situations, so the barometer has less lag. I only log the GPS every 5 seconds on the way up and often get an anomalous 2D reading when it regains lock, as in the graph below. You can also see in the graph the "mach dip" in the first few seconds and more lagging and sagging of the barometer during the fastest phase of flight.Mike, I saw the graphs your put up of your integrated accelerometer data. Can you put up graphs of your integrated accelerometer altitude, barometric altitude and GPS altitude from the flight you just did, so I can get a sense of how these match up for you?
I prefer the optical relays for the extra layer of isolation (vs transistor or mosfet)
I am going to have to do more work on my integrated altitude and up my logging rates.
That graph is very typical of flilghts that are close to mach transition. You can see the baro do a dip and then come back. With a high-G single-axis accelerometer (such as the one in the Eggtimer Proton) you can do decent off-axis check by comparing the two computed altitudes, and if they are sufficiently close then you're probably pointing "up". This works best a few seconds after burnout and in the early coast phase... which is when you generally are going to be lighting a sustainer.The flight yesterday is not the best dataset, as we switched velocity/altitude integration over to the 32G accelerometer and it maxed out in the first 1.5 seconds. Also, due to the very high G's the GPS did not come back online until it dropped 3-4K feet from apogee. that said, below is data from the previous flight. My accelerometer altitude also runs ahead or "hot" from the barometer. Intuitively that makes sense, as the barometer takes longer to sense/adjust, but even with that consideration it does seem like the accelerometer is always "more generous" with altitude. After apogee, the accelerometer data is useless. The GPS and the barometer tend to track very close, but the GPS is only working in "low speed" situations, so the barometer has less lag. I only log the GPS every 5 seconds on the way up and often get an anomalous 2D reading when it regains lock, as in the graph below. You can also see in the graph the "mach dip" in the first few seconds and more lagging and sagging of the barometer during the fastest phase of flight.
View attachment 449823
My particular interest is launcher interactions. That happens pretty fast and I want as much data as possible during that time. The MPU9250 had the highest data rate on gyros that I could find so that determined the sample rate.what were you logging at 32K? motor burns? That is like watching atoms split.
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