the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Next-generation Ionospheric Model for Operations – Validation and Demonstration for Space Weather and Research
Abstract. The Next-generation Ionospheric Model for Operations (NIMO) is an assimilative geospace model developed to address the space weather operational needs in the ionosphere. NIMO harnesses contributions from both near real-time data and state-of-the-art implementation of ionospheric theory to provide hindcasts, nowcasts, and forecasts for operational or research purposes. NIMO is currently configured to assimilate various types of electron density measurements through the Ionospheric Data Assimilation Four-Dimensional (IDA-4D) data assimilation schema. Information from the neutral atmosphere is provided by empirical models. The ionospheric chemistry and transport calculations are handled within NIMO using a version of SAMI3 is also a Model of the Ionosphere (SAMI3) designed to have a realistic geomagnetic field and work effectively on a parallel processing system. This article discusses how NIMO is configured, demonstrates potential use cases for the research community, and validates hindcast runs using a new suite of metrics designed to allow repeatable, quantitative, model-independent evaluations against publicly available observations that may be adopted by any ionospheric global circulation or regional space weather model.
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Status: open (until 10 Dec 2025)
- RC1: 'Comment on egusphere-2025-4967', Anonymous Referee #1, 04 Nov 2025 reply
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Title: Next-generation Ionospheric Model for Operations (NIMO): Validation and Demonstration for Space Weather and Research
Authors: A. G. Burrell et al.
Journal: EGUsphere
Recommendation: Moderate revision before acceptance
General Comments
This paper presents the Next-generation Ionospheric Model for Operations (NIMO), a data assimilation, physics-based system that combines the SAMI3 model with the IDA-4D framework. The authors provide a detailed description of the model configuration and a validation using multiple data sources, including ionosondes, incoherent scatter radars, GPS TEC, JASON altimetry, and in-situ plasma density from CINDI, DMSP, and ICON.
Overall, this is a well-structured contribution to the ionospheric modelling and space weather community. It demonstrates NIMO’s ability to deliver high-fidelity ionospheric specifications and forecasts and to outperform empirical models such as IRI-2016 under various geomagnetic conditions.
The study is methodologically sound, comprehensive, and of clear relevance for both research and operational use. However, a few issues require clarification or enhancement before publication.
Specifically, the manuscript would benefit from:
With these improvements, I would recommend acceptance after minor to moderate revision.
Specific Comments
Technical Corrections
Summary Recommendation
Decision: Recommended for publication after minor revision.
Suggested Actions Before Acceptance
Overall assessment:
This manuscript represents a valuable contribution to the field of space weather modelling. After addressing the relatively minor methodological clarifications and presentation issues listed above, it will merit acceptance for publication in Annales Geophysicae (or equivalent EGU journal).