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Why GNSS Can Struggle After Sunset: Ionospheric Scintillation Explained

Ionospheric scintillation can disrupt GNSS by rapidly changing signal amplitude and phase. Its after-sunset pattern is conditional, especially in equatorial regions, and mitigation results depend on the receiver and study conditions.

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Ionospheric scintillation is a real cause of GNSS signal disruption: irregularities in the ionosphere can rapidly change a satellite signal’s amplitude and phase, degrading measurements and, in severe cases, causing a receiver to lose lock. It is especially associated with the hours after sunset in equatorial regions during favorable seasons—not with every sunset or every location. Polar scintillation can occur in a different setting, including during magnetic storms.

What is ionospheric scintillation?

GNSS signals travel through the ionosphere, a region of the upper atmosphere containing charged particles. When those particles form small-scale irregularities, they can disturb a signal as it passes through. The resulting rapid fluctuations in received signal amplitude and carrier phase are called scintillation.

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This is distinct from the broader ionospheric delay and total electron content (TEC) gradients that can affect signal travel time and positioning. Scintillation describes rapid signal fluctuations; it can affect tracking and measurement quality even when the underlying issue is not simply a slowly varying delay.

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Why can GNSS become less reliable after sunset?

Equatorial scintillation is often observed in the hours after sunset during seasonally favorable conditions. The pattern is conditional: it is not a global schedule, and sunset alone does not establish that scintillation is occurring. Polar-region scintillation is a separate context and can occur during magnetic storms. The Institute of Navigation GNSS+ 2024 paper by Kleijer and colleagues describes both settings in those qualified terms: the paper abstract.

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What one evening dataset found

A separate Institute of Navigation GNSS+ 2024 study analyzed five months of observations recorded from 19:00 to 23:59 local time. In that dataset, severe signal-fade statistics peaked around 21:00 local time and declined afterward. The authors also reported stronger intensities near the Equatorial Ionization Anomaly and weaker intensities closer to the dip equator. These are findings for the stations and period studied, not a universal forecast for other locations or nights. Read the study abstract.

How can scintillation affect GNSS positioning?

Rapid amplitude and phase changes can make it harder for a receiver to maintain a stable signal track. Consequences can include degraded range measurements, cycle slips, reduced continuity or availability, and—in severe cases—loss of lock. ESA’s Space Weather Service Network describes the effect on carrier phase and signal amplitude and its implications for GNSS continuity and availability: ESA’s ionospheric scintillation overview. Receiver-monitoring literature from the Institute of Navigation likewise discusses degraded measurements, cycle slips, and possible loss of lock: the monitoring paper abstract.

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Timing by itself cannot diagnose a particular positioning problem. Interference, receiver design, antenna conditions, satellite geometry, and other factors may also affect performance; the cited sources do not establish the cause of an individual user’s outage.

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Which GNSS signals lose lock most often?

There is no universal signal ranking established by the evidence here. Susceptibility depends on the conditions and receiver tracking method, and the cited work does not provide a general comparison that would support saying one GNSS signal always loses lock most often. Scintillation’s amplitude and phase fluctuations can challenge tracking, but users should not treat a particular signal or constellation as invariably the weakest.

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Can a GNSS receiver detect scintillation?

Yes, if it is equipped and configured to collect observations at a sampling rate suitable for scintillation measurements. ESA notes that dedicated GNSS receivers are used for monitoring, but instruments able to sample at the required frequency are less widely available than ordinary GNSS equipment. Monitoring typically uses receiver observations and derived signal indices rather than relying on the time of day alone.

ESA’s MONITOR network uses high-frequency-sampling GNSS receivers deployed mainly at low and high latitudes. Its dataset includes daily scintillation indices, dual-frequency observables, high-frequency raw data, and TEC products. ESA announced the dataset on December 1, 2023; access is restricted and requires an application through the GSSC Helpdesk. See ESA’s MONITOR dataset announcement and the ESA GNSS scintillation information page.

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What mitigation approaches have researchers tested?

Mitigation is an engineering problem, not a single accessory or setting that works for every user. Research has examined changes to receiver estimation and tracking, with results tied to specific methods and test conditions.

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Adjusting the ionospheric-delay model

Kleijer and colleagues reported adapting the stochastic model used for ionospheric-delay estimation. In their 2024 case study, reported RTK performance increased from 55% with a 25 cm P95 error to 90% with a 7–9 cm P95 error. Those figures describe the study’s conditions and metric; they are not a guaranteed improvement for other receivers, sites, or operating conditions. The paper abstract.

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Combining a refined model with TEC maps

Park and colleagues studied estimating residual double-difference ionospheric delay using a refined stochastic model together with accurate TEC maps. Their long-baseline kinematic test under strong scintillation showed significant improvement over conventional approaches. This is evidence from a particular experimental low-latitude study, not a general-purpose correction recipe. The study abstract.

Using multi-frequency tracking methods

Florindo and Antreich compared multi-frequency Kalman-filter methods with single-frequency autoregressive models under synthetic scintillation events. The multi-frequency methods performed better in most tested conditions. Because the events were synthetic, this result should not be read as a guarantee of field performance in every real scintillation environment. The study abstract.

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