International Reference Ionosphere (IRI) is a common permanent scientific project of the Committee on Space Research and the International Union of Radio Science started 1968/69. It is the international standard for the terrestrial ionosphere since 1999.
Karl Rawer, first chairman of the URSI/COSPAR Task group on the IRI (1968-`84) specified as goal of the IRI to establish a (monthly) average model of the terrestrial ionosphere based on reliably measured data obtained with ground- and space-based methods. Contradictions between these had to be resolved in critical discussions. After a decade filled with data collection a first set of tables was given out in 1978. PC-codes in ALGOL and Fortran followed. 1986 the code became available on Floppy disk, later in the Web. It is yearly improved according to the results obtained at the meetings of the task group.Since 1999 the IRI is "International Standard" for ionosphere.
The IRI used (and yet uses as an option) an ITU-R-model that had been developed in respect to Radio propagation via the ionosphere, specifying two parameters of which one is narrowly related to the peak electron density and the other to the peak altitude of the ionosphere. Both have been and are regularly determined from Ionograms at all Ionospheric sounding stations. The authors R.M.Gallet and W.B.Jones had world-wide analyzed a wealth of such data by a method combining Fourier- analysis in time with world-wide Legendre-analysis of the Fourier-coefficients. Meanwhile regional models are often applied because they reach better local performance.
The IRI-model specifies vertical profiles of electron density, Electron and Ion temperature and the relative share of the different positive ions. Vertical Electron content may be derived (A snapshot is shown in the (latitude vs. longitude) map) aside).[1]