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📡 Amateur Radio & Satellites

Doppler Shift (Satellite Radio)

Also known as: Doppler Effect, Doppler Correction, Frequency Shift

📘 Definition
Doppler shift is the change in a radio signal's received frequency caused by the relative motion between a satellite and a ground station — the effect that makes a passing siren rise then fall in pitch. As a satellite in low Earth orbit races towards you at roughly 7.5 km/s it compresses the radio waves, so the received frequency climbs; after the closest point it recedes and the frequency drops. Because the shift is proportional to the transmit frequency, it grows with band — about ±3.5 kHz on the 2 m VHF band (145 MHz) and ±10 kHz on the 70 cm UHF band (435 MHz), falling to zero at the moment of closest approach. Wideband FM receivers absorb most of it, but SSB and CW users on a linear transponder must retune continuously. Run in reverse, the same physics is exploited by satellite navigation and lets ground stations measure a spacecraft's range rate for orbit determination.
±3.5 kHz
Shift on 2 m (145 MHz)
±10 kHz
Shift on 70 cm (435 MHz)
~7.5 km/s
LEO orbital speed
Tune the higher band
Correction rule

Understanding Doppler Shift

Doppler across a pass

A satellite's Doppler traces a smooth S-curve over a single pass. At acquisition of signal, when it first rises above the horizon and is heading towards you, the received frequency sits at its highest — the full positive shift. As the satellite climbs the shift shrinks, passing through zero at the point of closest approach — the highest-elevation moment of the pass, where the satellite is moving sideways rather than towards or away from you. It then turns negative and steepens as the satellite sinks back to the horizon. A high, near-overhead pass swings through the whole range fastest and demands the quickest tuning; a low pass that only grazes the horizon shifts more gently.

Why higher bands shift more

The Doppler shift is directly proportional to the carrier frequency, so the same 7.5 km/s of motion barely nudges a VHF signal yet drags a microwave one a long way. That is why the 2 m band is forgiving while operators working 23 cm and above must retune almost constantly. The figures below are approximate peak shifts for a good overhead pass; they are quoted as ± from the published frequency, so the full swing from the start of a pass to the end is about double. Slower-moving, more distant MEO and geostationary satellites shift far less, because their range rate relative to the ground is much lower.

Amateur bandFrequencyPeak Doppler (LEO)
2 m (VHF)145 MHz±3.5 kHz
70 cm (UHF)435 MHz±10 kHz
23 cm (L-band)1.26 GHz±30 kHz
13 cm (S-band)2.40 GHz±55 kHz

Correcting Doppler in practice

On wideband FM satellites the receiver's bandwidth swallows most of the shift, so a 2 m downlink often needs no tuning and a 70 cm link only occasional 5 kHz nudges — many operators just store split-frequency memories for the start, middle and end of a pass. SSB and CW on a linear transponder are far less forgiving: a drift of even 100 Hz is audible, so you must retune continuously. The long-standing rule is to tune the higher-frequency band and leave the lower one fixed — for a typical 70 cm-up, 2 m-down transponder that means adjusting the uplink. Many transponders also invert the passband (you transmit lower sideband and hear upper sideband), which makes the uplink and downlink shifts partly cancel. In practice most operators let rig-control software such as Gpredict or SatPC32 apply full correction to both links automatically. The ISS makes a good first target — its 145.800 MHz SSTV downlink shows gentle 2 m Doppler, while its 437.800 MHz FM cross-band repeater shows the larger 70 cm swing.

Doppler as a tool: navigation and tracking

The same effect is as much an instrument as a nuisance. The 1960s TRANSIT system — the first satellite-navigation network — worked purely by Doppler: a receiver watched a satellite's stable carrier rise and fall in frequency as it passed overhead and solved backwards for its own position. Modern GNSS receivers still contend with Doppler, searching a window of roughly ±5 kHz to lock onto each GPS signal and using the measured shift to compute your velocity. Ground stations run the physics in reverse for orbit determination, deriving a spacecraft's range rate from two-way Doppler, while systems such as Argos locate wildlife tags and ocean buoys from the Doppler curve of their transmissions.

🛰️ See the next pass
Doppler follows the geometry of a pass — steepest near the horizon, zero overhead. Look up the next pass of the ISS or any satellite, with its rise, peak-elevation and set times, so you know exactly when to start correcting.
Open pass predictions →
📖 Learn More

Frequently Asked Questions

Doppler shift is caused by the relative motion between the satellite and your ground station along the line of sight. As a satellite approaches, each wave crest is sent from slightly closer, so the crests arrive more often and the received frequency rises; as it moves away they arrive less often and the frequency falls. Only the radial (towards-or-away) part of the satellite's velocity counts, which is why the shift peaks near the horizon and vanishes overhead.
For a low Earth orbit satellite moving at about 7.5 km/s, the peak shift is roughly ±3.5 kHz on the 2 m band (145 MHz), ±10 kHz on 70 cm (435 MHz), ±30 kHz at 23 cm and ±55 kHz at 13 cm. These are the extremes seen near the horizon; the total swing from the start of a pass to the end is about double. Geostationary satellites barely shift at all because they scarcely move relative to the ground.
Because the size of the shift is directly proportional to the operating frequency. The 70 cm band (435 MHz) is almost exactly three times higher than the 2 m band (145 MHz), so the same satellite motion produces roughly three times the shift — about ±10 kHz instead of ±3.5 kHz. The trend continues upwards: microwave bands such as 13 cm can shift by ±50 kHz or more, which is why they demand constant automatic tuning.
Not much on the 2 m band, but usually yes on 70 cm. An FM receiver's bandwidth (around 15 kHz) is wide enough to tolerate the ±3.5 kHz shift of a 2 m downlink, so it often needs no tuning. The larger ±10 kHz shift on a 70 cm link does drift out of the passband, so most operators step the frequency in a few 5 kHz increments across the pass, or store split memories for its start, middle and end.
The standard rule is to tune the higher-frequency band and leave the lower one fixed — for a typical 70 cm-up, 2 m-down linear transponder that means continuously adjusting your uplink so your downlink stays put. A drift of even 100 Hz is audible on SSB, so most operators use rig-control software such as Gpredict or SatPC32 to apply full correction to both links automatically from the predicted orbit.
The shift is zero at the point of closest approach, which for a symmetric pass is the moment of highest elevation. At that instant the satellite is moving neither towards nor away from you — its velocity is purely sideways — so there is no compression or stretching of the waves and you receive the true transmitted frequency. Either side of that point the shift is positive (approaching) or negative (receding).

Sources & References

Definitions are reviewed against primary sources. Last reviewed: 2026-08-26.