International Reference Ionosphere Software (Oct 12, 2021) ---------------------------------------------------------- ================================================================================ The IRI is a joined project of the Committee on Space Research (COSPAR) and the International Union of Radio Science (URSI). IRI is an empirical model specifying monthly averages of electron density, ion composition, electron temperature, and ion temperature in the altitude range from 50 km to 1500 km. This directory includes the FORTRAN program, coefficients, and indices files for the latest version of the International Reference Ionosphere model: IRI2012. This version includes several options for different parts and parameters. A logical array JF(30) is used to set these options. The IRI-recommended set of options can be found in the COMMENT section at the beginning of IRISUB.FOR. IRITEST.FOR sets these options as the default. The compilation/link command in Fortran 77 is: f77 -o iri iritest.for irisub.for irifun.for iritec.for iridreg.for igrf.for cira.for iriflip.for Directory Contents: ----------------------------------------------------------------------------------- 00_iri.tar TAR file that includes all files from this directory and that was created in UNIX using 'tar -cvf 00_iri.tar *'. UNIX command to unpack is "tar -xvf 00_iri.tar". irisub.for This file contains the main subroutine iri_sub. It computes height profiles if IRI output parameters (Ne, Te, Ti, Ni, vi) for specified date and location. Also included is the subroutine iri_web that computes output parameters versus latitude, longitude (geog. or geom.), year, day of year, hour (LT or UT), and month. An example of how to call and use iri_web is shown in iritest.for. Compilation of iritest.for requires irisub.for, irifun.for, iritec.for, iridreg.for, igrf.for, and cira.for. irifun.for This file contains the subroutines and functions that are required for running IRI. iriflip.for Subroutines for the FLIP-related new model for the bottomside ion composition of Richards et al. iridreg.for Subroutines for the D region models of Friedrich-Torkar and of Danilov et al. iritec.for This file includes the subroutines for computing the ionospheric electron content from 60km up to a specified upper limit. cira.for This file includes the subroutines and functions for computing the COSPAR International Reference Ionosphere (NRLMSIS-00) neutral temperature and densities. igrf.for This file includes the subroutines for the International Geomagnetic Reference Field (IGRF). dgrf%%%%.dat Definitive IGRF coefficients for the years 1945 to 2010 in steps of 5 years (%%%%=1945, 1950, etc.)(ASCII). igrf%%%%.dat Prelimenary IGRF coefficients for most recent year (ASCII). igrf%%%%s.dat IGRF coefficients for extrapolating 5 years into the future (ASCII). MCSAT%%.dat Monthly coefficient files for the Shubin(2015) COSMIC-based hmF2 model %%=month+10 iritest.for Test program indicating how to use of the IRI subroutines. Requires irisub, irifun, iritec, iridreg, igrf,and cira. IN ADDITION THE FOLLOWING FILES ARE REQUIRED THAT ARE NOT INCLUDED IN THIS DIRECTORY. THESE FILES ARE AVAILABLE ON THE IRI HOMEPAGE IRIMODEL.ORG: At http://irimodel.org/indices/: ig_rz.dat This file(s) contains the solar and ionospheric indices (IG12, Rz12) for the time period from Jan 1958 onward. The file is updated quarterly. It is read by subroutine tcon in irifun.for (ASCII). [This file will be updated at close to quarterly intervals] apf107.dat This file provides the 3-hour ap magnetic index and F10.7 daily 81-day and 365-day index from 1960 onward (ASCII). [This file will be updated at close to quarterly intervals] Daily updates of these two files are available from the ECHAIM website (David Themens) as described on irimodel.org. At http://irimodel.org/COMMON_FILES/: CCIR%%.dat Monthly coefficient files for the CCIR foF2 and M(3000)F2 models %%=month+10 URSI%%.dat Monthly coefficient files for the URSI foF2 model %%=month+10 ----------------------------------------------------------------------------------- ----------------------------------------------------------------------------------- NOTE: Please consult the 'listing of changes' in the comments section at the top of each one of these programs for recent corrections and improvements. More information about the IRI project can be found at irimodel.org including access to sites that allow online computation and plotting of IRI parameters. ----------------------------- dbilitza@gmu.edu -------------------------------------