A first look at the Broadcom BCM47755 dual-frequency receiver

Over the last few months, readers have sent me several data sets collected from cell phones using the Broadcom BCM47755 dual-frequency GNSS chip. In most cases, however, the quality of the data was low and the number of cycle slips made it difficult to do any meaningful analysis. More recently I was sent some BCM4755 data collected from a Xiaomi Mi8 phone mounted on a tripod with a ground plane underneath that was noticeably better quality than the previous data sets. This data came from Julian who is trying to use the phone for forestry applications and has an open project he is working on here. In this post, I will describe my experiences attempting to use RTKLIB to analyze this data.

This is the first time I have worked with L5 data with RTKLIB so I wasn’t quite sure what to expect. Fortunately, with a few minor updates to the code handling code in RTKLIB which I have included in the most recent b33 version of the demo5 code, the code was able to see and process the L5 observations. Both rover and base observation files were sent to me in rinex format.

According to the rover file header, the rover rinex file was generated by Geo++ RINEX Logger App for Android (Version 2.1.3). It contains L1/E1/B1 observations for GPS, Glonass, Galileo, and Bediou and L5/E5a observations for GPS and Galileo. Like L2C, not all of the GPS satellites support L5 yet. In this case, only two of the six GPS satellites supported L5 data. All four of the Galileo satellites supported E1 and E5a observations but the rover was unable to pick up both frequencies for the one satellite between 10 and 15 degrees elevation. Below is a plot of the rover observations using RTKPLOT. Satellites in gray are below 10 degrees elevation. The rest of the colors indicate the frequencies of the observations according to the color key at the bottom of the plot. There is an error in the Galileo plot colors in which E5a-only observations are being plotted in green rather than gray. Overall though, the data is of reasonably good quality and has only a small number of receiver-reported cycle slips (red ticks).

Rover observations for B47755

The base data was from a CORS station about 20 km away and had matching signals for all the rover observations plus many more. Here is a plot of the base observations. This data is very clean.

For my initial attempt to run an RTKLIB solution on this data, I used the same config file I use for u-blox L1-only solutions except I changed the frequency mode from “l1” to “l1+l2+l5” Even though, there is no L2 data in these observations, RTKLIB does not allow you to individually select frequencies, just the number of frequencies, so valid choices are “l1”, “l1+l2”, and “l1+l2+l5”.

This run did not go well and digging into the trace file I found that RTKLIB was detecting many false cycle slips. The code attempts to detect cycle slips using the geometry-free linear combination of the L1 and L5 phase measurements. Either the threshold ( pos2-slipthres) is too tight for this data, or there is something wrong with this check. For the time being, I increased the slip threshold from the default of 5 cm to 50 cm and this eliminated the false slip detections.

Even with this change however, the solution was still very poor. Digging back into the trace debug file, I found more problems with cycle slips. This time I was finding that real cycle slips were not being flagged by the rover receiver in the rinex data. These unreported cycle slips were introducing large errors into the bias states in the kalman filter and preventing convergence. RTKLIB has always had trouble dealing with unflagged cycle slips. The u-blox receivers are very good at consistently flagging cycle slips which is why RTKLIB tends to work better with u-blox receivers than many other receiver types.

RTKLIB has some code to detect and reject outliers, but this code has never worked very well and I have generally recommended setting the outlier threshold (pos2-rejionno) to 1000 meters to effectively disable this feature.

For the BCM47755 receiver however, it was clear that this was not going to work. So I made some changes to the RTKLIB code to more fully ignore the outliers, and to reset the phase bias estimates when an outlier was detected. I also changed the way this threshold is interpreted for phase and code observations. Previously the threshold was used without adjustment for both phase and code observations. Since the code errors are much larger than the phase errors, this meant that the limit had to be set large enough so as to catch code outliers only. For the b33 demo5 code I changed this so that the unadjusted threshold is still used for the phase observations but the threshold is multiplied by the error ratio between phase and code observations (pos2-eratio1) before being used with code observations. This means that it can be set much lower and now becomes useful for detecting cycle slips instead of just code errors.

I have actually been using this fix for custom versions of RTKLIB for a while and usually get good results setting this to roughly one GPS L1 cycle or 20 centimeters. In this case though the rover data appears to be too noisy for this and I had to set the threshold to 50 centimeters (pos2-rejionno=0.50) to avoid triggering an excessive number of outliers.

With this change, the solution was much better and provided a solid fix after about four minutes with a “forward” solution as shown in the plot below. Even though the rover was static, I ran the solution as kinematic to get a better indication of the unfiltered errors. I also verified that this solution is using all the available measurements in the rinex file.

With a “combined” solution, the result was 100% fix.

This appears to be a fairly promising start for the BCM47755. It is still not nearly as solid as a u-blox receiver but some of this can be attributed to the fact that this data was collected with the internal phone antenna which is likely to be fairly low quality.

Unfortunately, other data sets from the same experimental setup did not generate solutions as solid as this. In particular the Galileo observations sometimes were not consistent with observations from the other constellations and prevented the kalman filter from converging.

Overall, my impression is that using BCM47755 and RTKLIB together for PPK solutions is still fairly immature and not ready for any real applications but hopefully this will change with time.

I am very interested in anyone else’s experiences with the BCM47755 for RTK or PPK solutions, particularly in combination with RTKLIB and hoping anyone with experience with this chip will add a comment below.