| Issue |
A&A
Volume 701, September 2025
|
|
|---|---|---|
| Article Number | A290 | |
| Number of page(s) | 9 | |
| Section | Astronomical instrumentation | |
| DOI | https://doi.org/10.1051/0004-6361/202556263 | |
| Published online | 25 September 2025 | |
An improved algorithm for separating clock delays from ionospheric effects in radio astronomy
1
ASTRON, Netherlands Institute for Radio Astronomy,
Oude Hoogeveensedijk 4,
Dwingeloo
7991PD,
The Netherlands
2
Kapteyn Astronomical Institute, University of Groningen,
PO Box 800,
9700 AV
Groningen,
The Netherlands
★ Corresponding author: cordun@astron.nl
Received:
4
July
2025
Accepted:
7
August
2025
Context. Low-frequency radio observations are heavily impacted by the ionosphere, where dispersive delays can outpace even instrumental clock offsets, posing a serious calibration challenge. Especially below 100 MHz, phase unwrapping difficulties and higher-order dispersion effects can complicate the separation of ionospheric and clock delays.
Aims. We address this challenge by introducing a method for reliably separating clock delays from ionospheric effects, even under mediocre to poor ionospheric conditions encountered near solar maximum.
Methods. The approach employs a key technique: we modelled our likelihood space using the circular Gaussian distribution (von Mises random variable) rather than non-circular distributions that suffer from 2π phase ambiguities. This ensures that noisier data are weighted less heavily than cleaner data during the fitting process.
Results. The method reliably separates clock delays and ionospheric terms that vary smoothly in time whilst providing a good fit to the data. A comparison with the clock-ionosphere separation approach used in standard LOFAR data processing shows that our technique achieves significant improvements. In contrast to the old algorithm, which often fails to return reliable results below 100 MHz even under good ionospheric conditions, the new algorithm consistently provides reliable solutions across a wider range of conditions.
Conclusions. This new algorithm represents a significant advance for large-scale surveys, offering a more dependable way to study ionospheric effects and furthering research in ionospheric science and low-frequency radio astronomy.
Key words: atmospheric effects / instrumentation: interferometers
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.