IRTAM
Version: NECTAR v0.2A_D3/1IRI-based Real-Time Assimilative Model (IRTAM) is a collection of global 3D ionospheric electron density (Ne) computations produced every 15 minutes to follow the timeline of the ionospheric weather dynamics. IRTAM 3D belongs to a class of "assimilative IRI" models that replace the internal coefficients of International Reference Ionosphere (IRI), an empirical quiet-time model of ionospheric climate, with updated coefficients. Updated coefficients are obtained by smoothly transforming ("morphing") IRI into agreement with available measurements. The morphing algorithm is called NECTAR (Non-linear Error Correction Technique with Associative Restoration); the version 0.2A computations for CCMC assimilate near-real-time measurements by the Global Ionosphere Radio Observatory (GIRO) ionosondes. NECTAR is a 4D-Var assimilative model whose single computation best fits a sliding window of the 24-hour history of GIRO observations prior to the analysis time. IRTAM’s underlying formalism of representing Ne distributions is the same as in IRI: a set of 2D surface maps are computed to obtain the "anchor" points of the 1D vertical extent of Ne at any location and time.
Caveats:
(1) IRTAM shows little advantage in the temporal forecast mode, gradually losing its advantage over IRI at the forecast horizon above 4 hours.
(2) The spatial coverage of GIRO ionosondes is fragmentary; data gaps are especially wide over the ocean and at high latitudes. Where observations are missing, IRTAM smoothly returns to the quiet-time climatology. A better version of IRTAM is in the early stage of development that uses radio occultation data to fill the data gaps.
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Inputs
Single run of IRI-2020 requires 4 sets of IRTAM weather coefficients for foF2, hmF2, B0, and B1. Replacing the default IRI climatology coefficients/formulas with IRTAM coefficients makes it a weather model.
Outputs
IRI-2020 provides the updated electron density outputs.
Domains
- Global Ionosphere
Space Weather Impacts
- Ionosphere variability (navigation, communications)
Phenomena
- Variablility of Plasma Density
- Equatorial Anomaly
Publications
- Galkin, I. A., B. W. Reinisch, X. Huang, and D. Bilitza (2012), Assimilation of GIRO data into a real-time IRI, Radio Sci., 47, RS0L07, doi:10.1029/2011RS004952.
- Galkin, I. A., Reinisch, B. W., Vesnin, A. M., Bilitza, D., Fridman, S., Habarulema, J. B., & Veliz, O. (2020). Assimilation of sparse continuous near-Earth weather measurements by NECTAR model morphing. Space Weather, 18, e2020SW002463. https://doi.org/10.1029/2020SW002463
- Reinisch, B. W., and I. A. Galkin, Global ionospheric radio observatory (GIRO), EPS, 63, 377-381, doi:10.5047/eps.2011.03.001, 2011.
- Forsythe, V. V., Galkin, I., McDonald, S. E., Dymond, K. F., Fritz, B. A., Burrell, A. G., et al. (2024). PyIRTAM: A new module of PyIRI for IRTAM coefficients. Space Weather, 22, e2024SW003965. https://doi.org/10.1029/2024SW003965
Code
Code Languages: Fortran, Python
Relevant Links
- GAMBIT home page
- Lowell GIRO Data Center (LGDC) Rules of the Road
- IRI Real-Time Assimilative Mapping (IRTAM) Page
- PyIRTAM
- IRI model
Contacts
- Ivan Galkin, Global Ionosphere Radio Observatory (GIRO), University of Massachusetts Lowell (Model Contact)
- Min-Yang Chou, NASA/GSFC (CCMC Model Host)
Publication Policy
In addition to any model-specific policy, please refer to the General Publication Policy.