Concept · RTK Fundamentals

How far can you be from the base station?

Baseline length — the distance between your rover and the nearest reference station — directly affects whether you get RTK Fix, how fast you get it, and how accurate it is. Here is what every RTK user needs to know.

On this page

  1. What is baseline length?
  2. Practical limits by setup type
  3. What happens as baseline grows
  4. How VRS solves long baselines
  5. Limits by device type
  6. Tips for long baseline situations

What is baseline length?

The baseline is the straight-line distance between your RTK rover and the reference station providing corrections. In a base-rover setup, that is your own base station. When using an NTRIP correction service, it is the nearest physical reference station in the network.

The shorter the baseline, the more similar the satellite signals seen by both rover and base — which means corrections are more accurate and Fix is faster. As the baseline grows, atmospheric differences (ionosphere and troposphere) between rover and base increase, making it harder for the receiver to resolve carrier phase ambiguities.

Baseline length and RTK performance

Typical performance ranges — exact values depend on your receiver, environment and correction service

0 km 30 km 60 km 100 km+
Fast Fix, cm accuracy
Slower Fix, use VRS
Fix unlikely without VRS

Practical limits by setup type

Setup type Recommended max Absolute max Status
Own base station
Single base, radio or NTRIP
10–15 km ~30 km Best accuracy
NTRIP network, standard mountpoint
Nearest physical station
20–30 km ~50 km Good in dense networks
NTRIP network, VRS mountpoint
Virtual reference station
Any distance in network Network coverage area Recommended for >30 km
NTRIP network, no VRS
Sparse station coverage
20 km ~40 km with degraded accuracy Use VRS if available
PPP (Precise Point Positioning)
No local base needed
Global Global Minutes to converge, cm post-fix

What happens as baseline grows

Longer baselines introduce three problems that affect RTK performance:

1. Ionospheric decorrelation

The ionosphere is a layer of charged particles that delays satellite signals. At short baselines, rover and base see nearly identical ionospheric conditions, so the corrections cancel out the delay well. Beyond roughly 20–30 km, ionospheric conditions diverge enough to degrade corrections, especially during high solar activity.

2. Tropospheric decorrelation

The lower atmosphere (troposphere) also delays signals based on temperature, pressure and humidity. These vary across terrain. At longer baselines, especially with significant altitude differences between rover and base, tropospheric errors become significant.

3. Slower ambiguity resolution

RTK Fix depends on resolving carrier phase ambiguities — an integer number that is the same for both rover and base. At longer baselines, this calculation becomes harder and takes longer, or may not converge at all. The result is Float instead of Fix.

Watch for this sign

If you are consistently stuck on Float and your environment is good (open sky, strong signal), long baseline is often the cause. Check the distance to the nearest reference station in your NTRIP sourcetable.

How VRS solves long baselines

VRS (Virtual Reference Station) is a network feature where the NTRIP server computes a synthetic correction stream as if a real base station existed right next to your rover — typically within 1–2 km. It achieves this by interpolating data from multiple physical stations across the network.

To use VRS, your NTRIP client must send your position (a GGA sentence) to the server. The server uses that position to generate the virtual corrections and streams them back. If GGA is not sent, the VRS cannot generate a local correction and you will receive no data.

VRS setup checklist

To use a VRS mountpoint: (1) enable GGA transmission in your NTRIP client, (2) select a mountpoint labelled VRS, MAC or RTCM3_VRS, (3) ensure you have a SINGLE or FLOAT solution first so GGA contains a valid position.

Limits by device type

Different receivers handle long baselines differently depending on their processing engine and the signals they track.

Emlid Reach RS2+ / RS3 / RS4
~60 km
Multi-band. Use VRS mountpoint beyond 30 km.
Emlid Reach RX / RX2
~30 km
Pure network rover. VRS strongly recommended.
Trimble / Leica
~100 km
Advanced engines. VRS or MAC required >30 km.
DJI RTK drones
~30 km
Use MSM5 mountpoint. VRS for longer baselines.
u-blox ZED-F9P
~20 km
Entry-level multi-band. Sensitive to baseline.
Single-frequency receivers
~10 km
Short baselines only. No ionospheric correction.

Tips for long baseline situations

Use VRS first

If your NTRIP service offers a VRS or MAC mountpoint, switch to it. This eliminates baseline as a factor entirely and is the single most effective change you can make.

If VRS is not available or you are using your own base station, here are additional steps:

Accuracy degrades with baseline even at Fix

RTK Fix does not guarantee centimetre accuracy at long baselines. At 50+ km without VRS, horizontal errors of 5–10 cm are common even with a Fix solution. For precision work, always verify with known control points.

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