UK Solar System Data Centre
This is an empirical model of the temperature and composition of the atmosphere at heights between 0 and 700km. It is based on mass spectrometer data from various satellites and on incoherent scatter radar data from several sites. Full details are given in the paper by A E Hedin which was published in the Journal of Geophysical Research, Vol 92, pages 4649-4662 (May 1987).
The program implemented here allows you to supply a range and step size for either latitude, longitude, height or time for the geomagnetic conditions prevalent for a particular date. The necessary values of Ap and solar radio flux are retrieved from the WDC C1 databases for a particular day. The values for the non-varying parameters are taken from the minimum for each of the other parameters.
The program produces for each time, altitude, latitude, longitude a table giving temperature, densities for N2, O, He, A, O2, H, N, and total mass density.