Updated guide to the RTKLIB configuration file

It’s been quite a while since I’ve updated my guide to the RTKLIB configuration file.  Since the last update I’ve added a couple of new features and learned a bit more about some of the existing features.  For previous updates,  I’ve just updated the original post, but this time I thought I would re-publish it to make it easier to find.

One of the nice things about RTKLIB is that it is extremely configurable and has a whole slew of input options available. Unfortunately these can be a bit overwhelming at times, especially for someone new to the software. The RTKLIB manual does briefly explain what each option does, but even with this information it can be difficult to know how best to choose values for some of the parameters.

I won’t try to give a comprehensive explanation of all the input options here, but will explain the ones I have found useful to adjust in my experiments and include a little about why I chose the values I did. I describe them as they appear in the configuration file rather than how they appear in the RTKNAVI GUI menu but the comments apply to both. I created this list by comparing my latest config files to the default config file and noting which settings were different. The values in the list below are the values I use in my config file for a 5 Hz rover measurement rate.  The same config files can be used for either RTKNAVI, RTKPOST, or RNX2RTKP.

The settings and options highlighted in blue below are available only in my demo code and not in the release code but otherwise much of what I describe below will apply to either code.  Most of my work is done for RTK solutions with Ublox M8N and M8T receivers and short baselines and these settings will more directly apply to these combinations but should be useful at least as a starting point for other scenarios.

This post is intended to be used as a supplement to the RTKLIB manual, not as a standalone document, so please refer to it for information on any of the input parameters not covered here.

SETTING1:

pos1-posmode = static, kinematic, static-start, movingbase, fixed

If the rover is stationary, use “static”. If it is moving, use “kinematic” or “static-start”. “Static-start” will assume the rover is stationary until first fix is achieved and then switch to dynamic mode, allowing the kalman filter to take advantage of the knowledge that the rover is not moving initially.  You can use “movingbase” if the base is moving as well as the rover, but it is not required unless the base is moving long distances.  I often find that “kinematic” gives better solutions than “movingbase” even when the base is moving.  “Movingbase” mode is not compatible with dynamics, so be sure not to enable both at the same time.  If the base and rover remain at a fixed distance apart, set “pos2-baselen” and “pos2-basesig” when in “movingbase” mode.   Use “fixed” if you know the rover’s exact location and are only interested in analyzing the residuals.

pos1-frequency = l1

L1 for single frequency receivers,  L1+L2 if the rover is dual frequency GPS/GLONASS/Bediou,  L1+L2+E5b if Galileo is included 

pos1-soltype = forward, backward, combined

This is the direction in time that the kalman filter is run. For real-time processing, “forward” is your only choice. For post-processing, “combined” first runs the filter forward, then backwards and combines the results. For each epoch, if both directions have a fix, then the combined result is the average of the two with a fixed status unless the difference between the two is too large in which case the status will be float. If only one direction has a fix, that value will be used and the status will be fixed. If both directions are float then the average will be used and the status will be float. Results are not always better with combined because a false fix when running in either direction will usually cause the combined result to be float and incorrect. The primary advantage of combined is that it will usually give you fixed status right to the beginning of the data while the forward only solution will take some time to converge. The 2.4.3 code always resets the bias states before starting the backwards run to insure independent solutions. The demo5 code doesn’t reset the bias states to avoid having to lock back up when the rover is moving if ambiguity resolution is set to “continuous” but does reset them if it is set to “fix-and-hold”.  I only use the “backward” setting for debug when I am having trouble getting an initial fix and want to know what the correct satellite phase-biases are.

pos1-elmask = 15 (degrees)

Minimum satellite elevation for use in calculating position. I usually set this to 10-15 degrees to reduce the chance of bringing multipath into the solution but this setting will be dependent on the rover environment. The more open the sky view, the lower this value can be set to.

pos1-snrmask-r = off, pos1-snrmask-b = off,on

Minimum satellite SNR for rover (_r) and base(_b) for use in calculating position. Can be a more effective criteria for eliminating poor satellites than elevation because it is a more direct measure of signal quality but the optimal value will vary with receiver type and antenna type so I leave it off most of the time to avoid the need to tune it for each application.

pos1-snrmask_L1 =35,35,35,35,35,35,35,35,35

Set SNR thresholds for each five degrees of elevation. I usually leave all values the same and pick something between 35 and 38 db depending on what the nominal SNR is. These values are only used if pos1-snrmask_x is set to on.  If you are using dual frequencies, you will need to also set “pos1-snrmask_L2”

pos1-dynamics = on

Enabling rover dynamics adds velocity and acceleration states to the kalman filter for the rover. It will improve “kinematic” and “static-start” results, but will have little or no effect on “static” mode. The release code will run noticeably slower with dynamics enabled but the demo5 code should be OK. Be sure to set “prnaccelh” and “prnaccelv” appropriately for your rover acceleration characteristics.  Rover dynamics is not compatible with “movingbase” mode, so turn it off when using that mode.

pos1-posopt1 = off, on (Sat PCV)

Set whether the satellite antenna phase center variation is used or not. Leave it off for RTK but you set it for PPP. If set to on, you need to specify the satellite antenna PCV file in the files parameters.

pos1-posopt2 = off, on (Rec PCV)

Set whether the receiver antenna phase center variations are used or not. If set to on, you need to specify the receiver antenna PCV file in the files parameters and the type of receiver antenna for base and rover in the antenna section. Only survey grade antennas are included in the antenna file available from IGS so only use this if your antenna is in the file. It primarily affects accuracy in the z-axis so it can be important if you care about height. You can leave this off if both antennas are the same since they will cancel.

pos1-posopt5 = off, on (RAIM FDE)

If the residuals for any satellite exceed a threshold, that satellite is excluded. This will only exclude satellites with very large errors but requires a fair bit of computation so I usually leave this disabled.

pos1-exclsats=

If you know a satellite is bad you can exclude it from the solution by listing it here. I only use this in rare cases for debugging if I suspect a satellite is bad.

pos1-navsys = 7, 15,

I always include GLONASS and SBAS sats, as more information is generally better.  If using the newer 3.0 u-blox firmware with the M8T I also enable Galileo.

 

SETTING2:

pos2-armode = continuous, fix-and-hold

Integer ambiguity resolution method. “Continuous” mode does not take advantage of fixes to adjust the phase bias states so it is the most immune to false fixes.  “Fix-and-hold” does use feedback from the fixes to help track the ambiguities.  I prefer to use “fix-and-hold” and adjust the tracking gain (pos2-varholdamb) low enough to minimize the chance of a false fix.  If “armode” is not set to “fix-and-hold” then any of the options below that refer to holds don’t apply, including pos2-gloarmode.

pos2-varholdamb=0.001, 0.1 (meters)

In the demo5 code, the tracking gain for fix-and-hold can be adjusted with this parameter. It is actually a variance rather than a gain, so larger values will give lower gain. 0.001 is the default value, anything over 100 will have very little effect. This value is used as the variance for the pseudo-measurements generated during a hold which provide feedback to drive the bias states in the kalman filter towards integer values.  I find that values from 0.1 to 1.0 provides enough gain to assist with tracking while still avoiding tracking of false fixes in most cases.

pos2-gloarmode = on, fix-and-hold, autocal

Integer ambiguity resolution for the GLONASS sats.  If your receivers are identical, you can usually set this to “on” which is the preferred setting since it will allow the GLONASS sats to be used for integer ambiguity resolution during the initial acquire. If your receivers are different or you are using two u-blox M8N receivers you will need to null out the inter-channel biases with this parameter set to “fix-and-hold” if you want to include the GLONASS satellites in the AR solution. In this case the GLONASS sats will not be used for ambiguity resolution until after the inter-channel biases have been calibrated which begins after the first hold. There is an “autocal” option as well, but I have never been able to make this work in the 2.4.3 code.  In the demo5 code I have added the capability to this feature to preset the initial inter-channel bias, variance, and calibration gain.  I then set the biases to known values for the particular receiver pair and set the gain very low.  This defeats the auto calibration aspect of the feature but does provide a mechanism to specify the biases which is otherwise missing in RTKLIB.  When “autocal” is used, the GLONASS satellites will be used for the initial acquire.  The “autocal” feature can also be used to determine the inter-channel biases with a zero or short baseline using an iterative approach.

pos2-gainholdamb=0.01

In the demo5 code, the gain of the inter-channel bias calibration for the GLONASS satellites can be adjusted with this parameter. 

pos2-arthres = 3

This is the threshold used to determine if there is enough confidence in the ambiguity resolution solution to declare a fix. It is the ratio of the squared residuals of the second-best solution to the best solution. I generally always leave this at the default value of 3.0 and adjust all the other parameters to work around this one. Although a larger AR ratio indicates higher confidence than a low AR ratio, there is not a fixed relationship between the two. The larger the errors in the kalman filter states, the lower the confidence in that solution will be for a given AR ratio. Generally the errors in the kalman filter will be largest when it is first converging so this is the most likely time to get a false fix. Reducing pos2-arthers1 can help avoid this.  

pos2-arfilter = on

Setting this to on will qualify new sats or sats recovering from a cycle-slip. If a sat significantly degrades the AR ratio when it is first added, its use for ambiguity resolution will be delayed. Turning this on should allow you to reduce “arlockcnt” which serves a similar purpose but with a blind delay count.

pos2-arthres1 = 0.004-0.10

Integer ambiguity resolution is delayed until the variance of the position state has reached this threshold. It is intended to avoid false fixes before the bias states in the kalman filter have had time to converge. It is particularly important to set this to a relatively low value if you have set eratio1 to values larger than 100 or are using a single constellation solution. If you see AR ratios of zero extending too far into your solution, you may need to increase this value since it means ambiguity resolution has been disabled because the threshold has not been met yet. I find 0.004 to 0.10 usually works well for me but if your measurements are lower quality you may need to increase this to avoid overly delaying first fix or losing fix after multiple cycle slips have occurred.

pos2-arthres2

Relative GLONASS hardware bias in meters per frequency slot.  This parameter is only used when pos2-gloarmode is set to “autocal” and is used to specify the inter-channel bias between two different receiver manufacturers.  To find the appropriate values for common receiver types, as well as how to use this parameter for an iterative search to find values for receiver types not specified, see this post.  This parameter is defined but unused in RTKLIB 2.4.3

pos2-arthres3 = 1e-9,1e-7

Initial variance of the GLONASS hardware bias state.  This parameter is only used when pos2-gloarmode is set to “autocal”.  A smaller value will give more weight to the initial value specified in pos2-arthres2.  I use 1e-9 when pos2-arthres2 is set to a  known bias, and 1e-7 for iterative searches.  This parameter is defined but unused in RTKLIB 2.4.3

pos2-arthres4 = 0.00001,0.001

Kalman filter process noise for the GLONASS hardware bias state.  A smaller value will give more weight to the initial value specified in pos2-arthres2.  I use 0.00001 when pos2-arthres2 is set to a  known bias, and 0.001 for iterative searches.  This parameter is defined but unused in RTKLIB 2.4.3

pos2-arlockcnt = 0, 5  

Number of samples to delay a new sat or sat recovering from a cycle-slip before using it for integer ambiguity resolution. Avoids corruption of the AR ratio from including a sat that hasn’t had time to converge yet. Use in conjunction with “arfilter”. Note that the units are in samples, not units of time, so it must be adjusted if you change the rover measurement sample rate.  I usually set this to zero for u-blox receivers which are very good at flagging questionable observations but set it to at least five for other receivers.  If not using the demo5 RTKLIB code, set this higher since the “arfilter” feature is not supported.

pos2-minfixsats = 4

Minimum number of sats necessary to get a fix. Used to avoid false fixes from a very small number of satellites, especially during periods of frequent cycle-slips.

pos2-minholdsats = 5

Minimum number of sats necessary to hold an integer ambiguity result. Used to avoid false holds from a very small number of satellites, especially during periods of frequent cycle-slips.

pos2-mindropsats = 10

Minimum number of sats necessary to enable exclusion of a single satellite from ambiguity resolution each epoch.  In each epoch a different satellite is excluded.  If excluding the satellite results in a significant improvement in the AR ratio, then that satellite is removed from the list of satellites used for AR.

pos2-rcvstds = on,off

Enabling this feature causes the the measurement variances for the raw pseudorange and phase measurement observations to be adjusted based on the standard deviation of the measurements as reported by the receiver. This feature is currently only supported for u-blox receivers. The adjustment in variance is in addition to adjustments made for satellite elevation based on the stats-errphaseel parameter.  I generally get better results with this turned off.

pos2-arelmask = 15

Functionally no different from the default of zero, since elevations less than “elmask” will not be used for ambiguity resolution but I changed it to avoid confusion.

pos2-arminfix = 20-100  (5-20*sample rate)

Number of consecutive fix samples needed to hold the ambiguities. Increasing this is probably the most effective way to reduce false holds, but will also increase time to first hold and time to reacquire a hold.  As the ambiguity tracking gain is reduced (i.e. as pos2-varholdamb is increased), and the number of observations increases, arminfix can be reduced.  Note that this value should also be adjusted if the rover measurement sample rate changes.

pos2-elmaskhold = 15

Functionally no different from the default of zero, since elevations less than “elmask” will not be used for holding ambiguity resolution results but I changed it to avoid confusion.

pos2-aroutcnt = 100 (20*sample rate)

Number of consecutive missing samples that will cause the ambiguities to be reset. Again, this value needs to be adjusted if the rover measurement sample rate changes.

pos2-maxage = 100

Maximum delay between rover measurement and base measurement (age of differential) in seconds. This usually occurs because of missing measurements from a misbehaving radio link. I’ve increased it from the default because I found I was often still getting good results even when this value got fairly large, assuming the dropout occurred after first fix-and-hold.

pos2-rejionno = 1000

Reject a measurement if its pre-fit residual is greater than this value in meters. I have found that RTKLIB does not handle outlier measurements well, so I set this large enough to effectively disable it. With non-ublox receivers which typically are not as good at flagging outliers, I sometimes have to set this back to the default of 30 or even lower to attempt to handle the outliers but this is a trade-off because it can then cause other issues, particularly with initial convergence of the kalman filter.

 

OUTPUT:

out-solformat = enu, llh, xyz

I am usually interested in relative distances between rover and base, so set this to “enu”. If you are interested in absolute locations, set this to “llh” but make sure you set the exact base location in the “ant2” settings. Be careful with this setting if you need accurate z-axis measurements. Only the llh format will give you a constant z-height if the rover is at constant altitude. “Enu” and “xyz” are cartesian coordinates and so the z-axis follows a flat plane, not the curvature of the earth. This can lead to particularly large errors if the base station is located farther from the rover since the curvature will increase with distance.

out-outhead = on

No functional difference to the solution, just output more info to the result file.

out-outopt = on

No functional difference to the solution, just output more info to the result file.

out-outstat = residual

No functional difference to the solution, just output residuals to a file. The residuals can be very useful for debugging problems with a solution and can be plotted with RTKPLOT as long as the residual file is in the same folder as the solution file.  

stats-eratio1 = 300
stats-eratio2  = 300

Ratio of the standard deviations of the pseudorange measurements to the carrier-phase measurements. I have found a larger value works better for low-cost receivers, but that the default value of 100 often work better for more expensive receivers since they have less noisy pseudorange measurements. Larger values tend to cause the kalman filter to converge faster and leads to faster first fixes but it also increases the chance of a false fix. If you increase this value, you should set pos2-arthres1 low enough to prevent finding fixes before the kalman filter has had time to converge. I believe increasing this value has a similar effect to increasing the time constant on a pseudorange smoothing algorithm in that it filters out more of the higher frequencies in the pseudorange measurements while maintaining the low frequency components.

stats-prnaccelh = 3.0

If receiver dynamics are enabled, use this value to set the standard deviation of the rover receiver acceleration in the horizontal components. This value should include accelerations at all frequencies, not just low frequencies. It should characterize any movements of the rover antenna, not just movements of the complete rover so it may be larger than you think. It will include accelerations from vibration, bumps in the road, etc as well as the more obvious rigid-body accelerations of the whole rover.  It can be estimated by running a solution with this value set to a large value, then examining the accel values in the solution file with RTKPLOT

stats-prnaccelv = 1.0

The comments about horizontal accelerations apply even more to the vertical acceleration component since in many applications the intentional accelerations will all be in the horizontal components. It is best to derive this value from actual GPS measurement data rather than expectations of the rigid-body rover. It is better to over-estimate these values than to under-estimate them.

ant2-postype = rinexhead, llh, single

This is the location of the base station antenna. If you are only interested in relative distance between base and rover this value does not need to be particularly accurate. For post-processing I usually use the approximate base station location from the RINEX file header. If you want absolute position in your solution, then the base station location must be much more accurate since any error in that will add to your rover position error. If I want absolute position, I first process the base station data against a nearby reference station to get the exact location, then use the ”llh” or “xyz”option to specify that location. For real-time processing, I use the “single” option which uses the single solution from the data to get a rough estimate of base station location.

ant2-maxaveep = 1

Specifies the number of samples averaged to determine base station location if “postype” is set to “single”. I set this to one to prevent the base station position from varying after the kalman filter has started to converge since that seems to cause long times to first fix. In most cases for post-processing, the base station location will come from the RINEX file header and so you will not use this setting. However if you are working with RTCM files you may need this even for post-processing.

 

MISC:

misc-timeinterp =off,on

Interpolates the base station observations.  I generally set this to “on” if the base station observations sample time is larger than 5 seconds.

Please help me update this list if you have had success adjusting other options or using different settings for these options, or if you disagree with any of my suggestions. I will treat this as a working document and continue to update it as I learn more.

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Moving-base solutions (part 2)

In my last post I discussed solving for moving-base data sets using the ordinary fixed-base solution modes and promised to discuss solutions using the RTKLIB “movingbase” method in my next post.

Let me start by saying I had hoped to have had more success with this method by the time I got to writing this post but that has not been the case.  I have tried both the most recent demo5 code and the 2.4.3 release code and neither gives me clean reliable solutions if I turn on the “movingbase” option.

In the previous post I had picked a fairly challenging data set to demonstrate with.  In case that was interfering with the solution, I first switched to a cleaner data set for this experiment.  This is a data set taken with two Emlid Reach M8T receivers, one mounted on each end of a kayak while out in the ocean near Sussex England and was sent to me by Matt. Here is the solution using the same input configuration file I used in my previous post, with “movingbase” turned off.

kayak1

The distance between the receivers in this case is larger and the deviations from a circle are very small.  This result should provide very accurate heading measurements.  The two visible deviations from the circle in the plot above are caused by rolling the kayak over an embankment at at launch and retrieval.  These large z-axis movements violate the assumption that movements are all in the x-y direction and cause the solution to leave the circle onto a sphere but are not actual errors.

Here’s a solution using the latest 2.4.3 code with “movingbase” enabled.

kayak2

It may be that I am doing something silly but I did spend a fair bit of time trying to get a decent solution without success.  If anybody more familiar with “movingbase”solutions would like to take a shot at it, I’ve uploaded this data set to here on the rtkexplorer.com website.  Please let me know if you are able to get a decent “movingbase” solution with this data.

I went back to the more challenging original data set from last post since I actually had slightly more success with that one, although still quite limited.

In my first attempt with “movingbase” enabled, I ran into the same problem as last post where the missing measurements in the base data caused large spikes in the solution.  This was true even with the max age of differential set to less than one sample time, which is what fixed the problem previously.  Looking at the code, this is because the “maxage” input parameter is ignored when “movingbase” is set and a hard-coded value is used instead (more about this below).   I modified the code so that it did check the “maxage” limit for “movingbase” and then got the following solution.

movebase6

The spikes are much smaller now that the missing samples are removed but they are still occurring, this time when both measurements are present.  The spikes are large enough to make this solution useless.  At this point I have given up trying to get useful results with the “movingbase” solution but again would be very interested if someone else can show good results for this data as well.  The raw data is located at the same link as the previous data set.

I am not completely surprised that the “movingbase” solutions are not working well, since the only other case I’m aware of that RTKLIB allows the base to move also has caused me problems.  That occurs when running real-time solutions and setting the base location to “Average of Single Positions” and then setting the number of averages greater than one.   Whenever I have done this, the solution takes a long time to converge.  I get much faster first fixes if I set the number of averages to one which then prevents the base location moving after the first measurement.

Since I did spend some time going through the code to understand how the “movingbase” solution is supposed to work, I thought I would share that here.  Setting the solution mode to “movingbase” sets the opt->mode variable in the code to “PMODE_MOVEB” so I started by searching the code base for this.  There is also a section in the RTKLIB manual in Appendix E that describes the moving-base model.  Here’s a quick summary for the significant differences I found that occur when in “movingbase” mode

  1. Adjust base position every epoch: Based on single point position result.
  2.  Synchronize rover/base measurements:  The measurement times between the two receivers may vary slightly (usually less than 2 msec).  This can degrade accuracy in the case of very fast-moving rovers.  To prevent this, the base measurements are adjusted for their time difference.  Uses a hard-coded value (1.01 sec) for max age of differential instead of the “maxage”input config parameter.
  3. Constrain baseline: Add a pseudo-measurement to the kalman filter measurement update based on the error from the baseline length specified in “pos2-baselen” and “pos2-basesig” input parameters. (Only applied if pos2-baselen>0)
  4. Increase kalman filter update iterations:  Add two iterations to the number of iterations specified by the “pos2-niter” input parameter.  This should improve the response in the case of large non-linearities introduced by short baselines or rotational accelerations.

So, based on these results, my recommendation for processing moving-base data is to use the ordinary fixed-base solution parameters I described in my previous post.  This will usually give good results but be aware that there will be limitations in the cases where the rover moves a very long distance away from it’s starting point or if is moving fast relative to any sampling time deviations between the two rovers.

 

 

Exploring moving-base solutions

Recently, I’ve had several questions about moving-base solutions so that will be the topic for this post.

As you might guess from the name, a moving-base solution differs from the more common fixed-based solutions in that the base station is allowed to move in addition to the rover.   Although it could be used to track the distance between two moving rovers it is more commonly used in a configuration with two receivers attached to a single rover and used to determine heading. Since the receivers remain at a fixed distance from each other, the solution in this case becomes a circle with a radius equal to the distance between the receivers.  The location on this circle corresponds to the rover’s heading which is easily calculated using a four quadrant arctan of the x and y components of the position.  I also used moving base solutions in several of my earliest posts because the circular nature of the solution makes it easier to verify the solution and to measure errors.  Since all solution points should be on the circle, any deviation from the circle can be assumed to be error.

To be more exact, everywhere I mention “circle” above I really should say “sphere” instead since the solution has three dimensions, but if the rover is ground-based, the movements in the z-axis will be relatively small and for simplicity we can assume it is a circle.

In fixed-base solutions, the measurement rate of the base station is often lower than the rover both because it’s location is not changing and also because the base data often has to be transmitted over a data link which may be bandwidth limited.  In a moving-base solution, since both receivers are moving, and there is usually no need for a data link since they are both attached to the same rover, it makes sense to use the same data rate for both receivers.

For this exercise, I chose to use a data set I discussed previously in my “M8N vs M8T” series of posts.  It consists of two receivers, an M8N and an M8T, on top of a moving car and another M8T receiver used as a fixed base station.  The car drives on roads with a fairly open sky view for up to a couple kilometers away from the base station.  The base station is located next to some sheds and a tree, so is not ideal, but still has fairly open skies.  All three receivers  ran at 5 Hz sampling rate and both moving receivers have some missing samples.  I’m not sure exactly why this is, it may be because I used a single laptop to collect both data streams.  Regardless of where they come from, I have found occasional missing samples are fairly common whenever I collect data at higher sample rates and believe the solution should be robust enough to handle them.  The rover M8T data also has a simultaneous cycle-slip type receiver glitch near the beginning of the data as described in my last post.  Overall, I would consider this a moderately challenging data set but those are often the best kind for testing the limits of RTKLIB.

union1

Having data from three receivers gives us the luxury of being able to calculate three different solutions (base->rover1, base->rover2, and rover1->rover2) and then compare results between them.  Since the first two solutions are fixed-base and the third is a moving-base, it also allows us to validate the moving-base solution using a combination of the two fixed-base solutions.

To start with, let’s calculate solutions for the distance between each moving receiver relative to the fixed base station using the demo5 code and my standard config files for the M8N and M8T receivers.  The only difference between the two config files is that the GLONASS ambiguity resolution (gloarmode) is set to “fix-and-hold” for the M8N config file and to “on” for the M8T config file for reasons explained in previous posts.   I’ve also done the conversion from raw data to RINEX observation files with the TRK_MEAS and STD_SLIP receiver options set to 2 and 4 respectively, again for reasons previously explained.  I set the solution mode to “static-start” since I knew the data set started with the rover stationary for long enough to get a first fix but I also could have used “kinematic” mode.

Subtracting the two fixed-base solutions gives us the distance between the two rover receivers which should be equal to a moving-base solution calculated directly between the two rovers.  The only difference is that the errors will be larger in the difference of two solutions than they will be in the direct solution because the errors in the combined solutions will accumulate.

Here are the positions and ground track for the difference between the two solutions, using the “1-2” plotting option in RTKPLOT.  As expected we get a circle for the ground track.  From the radius of the circle we can tell that the two rovers were about 15 cm apart.  Usually you would put the two receivers as far apart as possible, since the errors in the heading will decrease as the distance between the rovers increases but in this case I hadn’t intended to use the results this way so had placed the rovers closer together.  Still, it might be representative of a configuration on a small drone or other small rover.

movebase5

Next let’s try to calculate the solution directly between the two moving receivers.  RTKLIB does have a special “moving-base” mode but we won’t use this yet.  The “kinematic” solution calculates the distance between the two rovers regardless of the location of the base, so for now we can ignore the fact that the base is moving.  This will breakdown eventually if the rover gets too far from the base but since in this data set the rover is only a couple kilometers from the base at its farthest point we should be OK.

The only change I made to the config file from the previous M8N run for this run was to reduce the acceleration input parameters “stats-prnaccelh” and “stats-prnaccelv” which are used to describe the acceleration characteristics of the rover in the horizontal and vertical directions relative to the base.  In the fixed-base solution, these need to include both the linear accelerations and rotational accelerations since the rover is moving and the base is fixed, but in the moving-base solution, since we care only about differential acceleration between the receivers, we can ignore the linear accelerations and include only the rotational accelerations.  I just used a rough guess and reduced the numbers from (1,0.25) to (0.25,0.1) but I could have found more exact numbers by looking at the acceleration plot of an initial run of the solution.

Here’s the solution using this configuration.  It looks reasonable except for the occasional large spikes.

movebase2

After a little debugging, I found that the spikes were occurring wherever there was a missing sample in the base data.  When this occurs, RTKLIB just uses the previous base sample.  This works fine when the base is not moving, but in this case that’s no longer true, and the previous base measurements are not good estimates of the current position.  We can tell RTKLIB to skip these measurements by setting the maximum age of differential to something less than one sample time.  This is done with the “pos2-maxage” input parameter.  I set it to 0.1 which is half of one sample time.

With this change, I got the following solution for the position.  Much better!

movebase3

The ground track for this solution is shown below on the right, on the left is the previous ground track derived by subtracting the two fixed-base solutions.  As expected, the solutions look very similar except the moving-base solution has smaller errors which appear as deviations from a perfect circle.

movebase1

To further validate this solution we can compare the heading calculated from the moving-base position with the heading determined from the velocity vector of the fixed-base solution.  This wouldn’t work if the rover were a boat, drone, or person, but in the case of a car there are no external lateral drifts and the car will move in the direction it is pointed (unless it’s in reverse of course).   This won’t work if the velocity is zero or near zero but for reasonably high velocities we should get a good match.  The top plot below shows the difference between the two.  The blue line is for all velocities and the red is for when the velocity drops below 5 m/s.  The bottom plot shows the distance from the base to the rover.

movebase4

As expected, the errors are large when the velocities are low but we get a good match otherwise.  There also appears to be no correlation between the errors and the base to rover distance which suggests we are well below the maximum base to rover distance before we start to see issues with our assumption that the base did not move.

Overall, this solution looks excellent, with 100% fix and based on deviations from the circle, very small errors.  In fact, I recommend this configuration over the RTKLIB “moving-base” solution if you are able to live within the maximum baseline constraints.  I don’t know how large that is, but it looks like it may be significantly larger than 2 kilometers which is probably large enough for most applications.

In the next post I will explore what happens when the RTKLIB solution mode is set to “movingbase” in more detail but for now let me bring up just one of its effects since it is something we can also do here without invoking “movingbase” mode and it may have some benefit.

RTKLIB uses an extended kalman filter which is designed to handle non-linearities in the system by linearizing around the current operating point.  This generally works quite well but as the system becomes more non-linear, the errors introduced by this approximation grow larger.  One way to deal with this is to run multiple iterations of the kalman filter every measurement sample to converge on the correct answer.  As we get closer to the correct answer, we will operate closer to the point around which the system has been linearized and the errors will be smaller.  There is an input parameter in RTKLIB called “pos2-niter” that specifies the number of filter iterations for each sample.  The default value is one but when “posmode” is set to “movingbase” two iterations are automatically added to whatever this value is set to.  In the default case, we would get three iterations every sample instead of one.  Since the kalman filter assumes all velocities are linear and in the moving-base case we have been looking at, they are all rotational and non-linear, it might make sense to do this.  In my example, the sample rate is quite high relative to the rate of rotation and I found it did not help, but in other cases where the rate of rotation is higher relative to the sample rate, it might be a good idea.

So, let me finish by summarizing the changes I recommend for moving-base solutions.

  1.  Set measurement sample rate for both rover and base to the same value
  2. Leave “pos1-posmode” set to “kinematic” or “static-start”
  3. Set “pos2-maxage” to half the sample time (e.g 0.1 for 5 samples/sec)
  4. Reduce “stats-prnaccelh” and “stats-prnaccelv” to reflect differential accelearation
  5. Experiment with increasing “pos2-niter” from 1 to 3

These recommendations are based on my fairly limited experience with moving-base solutions so if anybody else has other recommendations, please respond in the Comments section.

I have added the data set I used here to the data sets available for download on rtkexplorer.com for anyone who would like to experiment further with this data.

In the next post, I will talk more about what happens when “pos1-posmode” is set to “movingbase”.