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      The International Reference Ionosphere Model: A Review and Description of an Ionospheric Benchmark

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          Abstract

          This paper is a review of the International Reference Ionosphere (IRI) project and model. IRI is recognized as the official standard for the Earth's ionosphere by the International Standardization Organization, the International Union of Radio Science, the Committee on Space Research, and the European Cooperation for Space Standardization. As requested by these organizations, IRI is an empirical (data‐based) model representing the primary ionospheric parameters based on the long data record that exists from ground and space observations of the ionosphere. The core model describes monthly averages of the electron density, electron temperature, ion temperature, and ion composition globally in the altitude range from 60 to 2,000 km. Over time additional parameters were added in response to requests from the user community, this includes the equatorial ion drift, the occurrence probability of spread‐F and of an F1 layer, auroral boundaries and the electron content from the bottom of the ionosphere to user‐specified altitude. IRI has undergone extensive validations and is used for a wide range of applications in science, engineering, and education. This review is the result of many requests we have received for a comprehensive description of the model. It is also meant as a guide for users who are interested in a deeper understanding of the model architecture and its mathematical formalism.

          Plain Language Summary

          The International Reference Ionosphere (IRI) is the international standard for Earth's ionosphere. The ionosphere is the plasma layer of electrons and ions that surrounds the Earth in the 60–2,000 km altitude range. In spite of being a very small constituent of the atmosphere, the important role of the ionosphere lies in its retarding and refractive effect on electromagnetic waves and in particular radio waves in the different frequency bands from very low frequencies (VLFs) to very high frequencies (VHFs). Because of these effects, IRI is needed and has been used for a wide area of applications including spacecraft navigation, telecommunication, radio astronomy, Earth observation from space, visualizations of geo‐space for educational purposes, design of satellites and their payloads, testing data analysis schemes. To support the scientific understanding and operational use, and to explain the limitations of the model, this paper provides a much needed review and description of its scientific background and mathematical formalism.

          Key Points

          • International Reference Ionosphere (IRI): Scientific background and mathematical formalism

          • Description of the latest version of the model: IRI‐2022

          • IRI Achievements and plans for the future

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          Most cited references311

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          Extension of the MSIS Thermosphere Model into the middle and lower atmosphere

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                Author and article information

                Contributors
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                Journal
                Reviews of Geophysics
                Reviews of Geophysics
                American Geophysical Union (AGU)
                8755-1209
                1944-9208
                December 2022
                October 12 2022
                December 2022
                : 60
                : 4
                Affiliations
                [1 ] Department of Physics and Astronomy George Mason University Fairfax VA USA
                [2 ] Heliospheric Laboratory NASA Goddard Space Flight Center Greenbelt MD USA
                [3 ] Istituto Nazionale di Geofisica e Vulcanologia Roma Italy
                [4 ] Institute of Atmospheric Physics of the Czech Academy of Sciences Prague Czech Republic
                [5 ] Observatori de l’Ebre CSIC Universitat Ramon Llull Roquetes Spain
                [6 ] Lowell Digisonde International Lowell MA USA
                [7 ] Space Science Laboratory University of Massachusetts Lowell MA USA
                Article
                10.1029/2022RG000792
                3bf84b28-a41a-41f4-bfc9-4d25eec03672
                © 2022

                http://creativecommons.org/licenses/by-nc-nd/4.0/

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