Ionospheric Characterization Over Iran Using Multi‐Frequency IMB HF Transmitters and Global WSPRNET Reception During the 12 November 2025 Geomagnetic Storm

Abstract The Ionospheric Monitoring Beacon network in Iran provides continuous, multi‐frequency high‐frequency (HF) transmissions using WSPRNET modulation, enabling global reception and near–real‐time monitoring of ionospheric propagation conditions. In this study, we analyzed HF signals transmitted from Shiraz, Tabriz, Mashhad, and Birjand across several frequencies spanning 7–18 MHz. Reception reports from worldwide WSPRNET stations were used to characterize frequency‐dependent diurnal behavior, spatial coverage, and temporal variability under geomagnetically quiet conditions and during the ionospheric disturbances associated with the intense geomagnetic storm of 12 November 2025. The observations revealed systematic dependencies of HF propagation on transmission frequency, transmitter location, and storm‐time ionospheric electron density modifications. Lower frequencies exhibited delayed, absorption‐dominated responses consistent with enhanced D‐ and lower F‐region ionization, whereas higher frequencies showed rapid enhancements or disruptions associated with F‐region restructuring and electron density redistribution. Transmitter‐dependent differences reflected variations in latitude, background ionospheric structure, and propagation geometry across Iran. To interpret these results, three‐dimensional ray‐tracing simulations were conducted using physics‐based ionospheric models constrained by GNSS‐derived total electron content. Modified electron density distributions incorporating storm‐time tilts and gradients reproduced the observed multi‐frequency propagation anomalies, including changes in hop structure and geographic reach. These results demonstrated that distributed, multi‐frequency HF beacon networks effectively constrain regional ionospheric structure and its response to geomagnetic forcing, supporting space weather monitoring and HF communication applications.

Authors

Institutions

Publication Details

Journal
Space Weather
Published
2026-05-27
DOI
https://doi.org/10.1029/2025sw004917
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Ionospheric Characterization Over Iran Using Multi‐Frequency IMB HF Transmitters and Global WSPRNET Reception During the 12 November 2025 Geomagnetic Storm

A. Mahmoudian, Mohammad Azimi, Saba Hafizi Lotfabadi
Space Weather
Ionosphere and magnetosphere dynamics
article

Ionospheric Characterization Over Iran Using Multi‐Frequency IMB HF Transmitters and Global WSPRNET Reception During the 12 November 2025 Geomagnetic Storm

A. Mahmoudian, Mohammad Azimi, Saba Hafizi Lotfabadi
article en

Abstract

Abstract The Ionospheric Monitoring Beacon network in Iran provides continuous, multi‐frequency high‐frequency (HF) transmissions using WSPRNET modulation, enabling global reception and near–real‐time monitoring of ionospheric propagation conditions. In this study, we analyzed HF signals transmitted from Shiraz, Tabriz, Mashhad, and Birjand across several frequencies spanning 7–18 MHz. Reception reports from worldwide WSPRNET stations were used to characterize frequency‐dependent diurnal behavior, spatial coverage, and temporal variability under geomagnetically quiet conditions and during the ionospheric disturbances associated with the intense geomagnetic storm of 12 November 2025. The observations revealed systematic dependencies of HF propagation on transmission frequency, transmitter location, and storm‐time ionospheric electron density modifications. Lower frequencies exhibited delayed, absorption‐dominated responses consistent with enhanced D‐ and lower F‐region ionization, whereas higher frequencies showed rapid enhancements or disruptions associated with F‐region restructuring and electron density redistribution. Transmitter‐dependent differences reflected variations in latitude, background ionospheric structure, and propagation geometry across Iran. To interpret these results, three‐dimensional ray‐tracing simulations were conducted using physics‐based ionospheric models constrained by GNSS‐derived total electron content. Modified electron density distributions incorporating storm‐time tilts and gradients reproduced the observed multi‐frequency propagation anomalies, including changes in hop structure and geographic reach. These results demonstrated that distributed, multi‐frequency HF beacon networks effectively constrain regional ionospheric structure and its response to geomagnetic forcing, supporting space weather monitoring and HF communication applications.

Space WeatherVol. 24(6)
Islamic Azad University, Karaj (IR), University of Tehran (IR)
University of Tehran
Openalex Percentile: Top 6%
Ionosphere and magnetosphere dynamics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.