A climatological model of the ionospheric foF2 and hmF2 covariance for OTHR

Ionospheric models are used extensively to understand how the ionosphere affects radio wave propagation, and how this impacts radar, satellite communications and navigation systems.Most widely used models either provide a monthly median model of the ionosphere or ingest realtime data to provide a real-time model.In this paper, work to incorporate ionospheric variability into monthly median models is presented.This is done through the development of a global covariance model of the critical frequency (foF2) and the height of the peak electron density (hmF2) of the ionospheric F2 layer.A method of incorporating this into over-the-horizon radar (OTHR) modelling is then presented.

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Publication Details

Published
2025-01-01
DOI
https://doi.org/10.46620/ursiaprasc25/swpj5164
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

A climatological model of the ionospheric foF2 and hmF2 covariance for OTHR

Danielle Edwards, M. A. Cervera
Ionosphere and magnetosphere dynamics
article

A climatological model of the ionospheric foF2 and hmF2 covariance for OTHR

Danielle Edwards, M. A. Cervera
article en

Abstract

Ionospheric models are used extensively to understand how the ionosphere affects radio wave propagation, and how this impacts radar, satellite communications and navigation systems.Most widely used models either provide a monthly median model of the ionosphere or ingest realtime data to provide a real-time model.In this paper, work to incorporate ionospheric variability into monthly median models is presented.This is done through the development of a global covariance model of the critical frequency (foF2) and the height of the peak electron density (hmF2) of the ionospheric F2 layer.A method of incorporating this into over-the-horizon radar (OTHR) modelling is then presented.

Department of Science and Technology, Ministry of Science and Technology, India
Openalex Percentile: Top 83%
Ionosphere and magnetosphere dynamics
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