Characterizing ionospheric variability through HF Doppler measurements: a statistical and numerical ray tracing analysis
High-frequency (HF) skywave propagation relies on the ionosphere, making it susceptible to ionospheric variability. This study analyzes long-term Doppler residual measurements of a 10 MHz HF link between Fort Collins, CO, and Newark, NJ, to characterize the impact of ionospheric conditions on the link. We report that daytime measurements of Doppler variability exhibit Cauchy statistics, while nighttime measurements show a combination of exponential and log-normal statistics. These patterns correlate with solar activity and solar zenith angle. We also use PHaRLAP numerical ray tracing simulations through the IRI 2020 ionosphere to provide insights into signal ray paths and the altitudes of the ionosphere contributing to the observed Doppler shifts. By examining diurnal variations and statistical properties of Doppler residuals, this study aims to enhance our understanding of ionospheric dynamics and their influence on HF signal characteristics.
Authors
- G. W. Perry (ORCID: https://orcid.org/0000-0002-4690-5783)
- Kristina Collins (ORCID: https://orcid.org/0000-0002-3816-1948)
- Tiago Trigo
- Nathaniel A. Frissell
- John Gibbons
- Sabastian Fernandes
Institutions
- University of Scranton (US)
- Space Science Institute (US)
- Institute of Solar-Terrestrial Physics (RU)
- Case Western Reserve University (US)
Publication Details
- Journal
- Frontiers in Astronomy and Space Sciences
- Published
- 2026-03-11
- DOI
- https://doi.org/10.3389/fspas.2026.1713968
- Primary Topic
- Ionosphere and magnetosphere dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Science Foundation
- National Aeronautics and Space Administration
- Case Western Reserve University
- Nuclear Safety and Security Commission