THE FIRST REAL-TIME WORLDWIDE IONOSPHERIC PREDICTIONS NETWORK - AN ADVANCE IN SUPPORT OF SPACEBORNE EXPERIMENTATION, ONLINE MODEL VALIDATION, AND SPACE WEATHER
Ep. Szuszczewicz et al., THE FIRST REAL-TIME WORLDWIDE IONOSPHERIC PREDICTIONS NETWORK - AN ADVANCE IN SUPPORT OF SPACEBORNE EXPERIMENTATION, ONLINE MODEL VALIDATION, AND SPACE WEATHER, Geophysical research letters, 25(4), 1998, pp. 449-452
We report on the first realtime ionospheric predictions network and it
s capabilities to ingest a global database and forecast F-layer charac
teristics and ''in situ'' electron densities along the track of an orb
iting spacecraft. A global network of ionosonde stations reported arou
nd-the-clock observations of F-region heights and densities, and an on
-line library of models provided forecasting capabilities. Each model
was tested against the incoming data; relative accuracies were interco
mpared to determine the best overall fit to the prevailing conditions;
and the best-fit model was used to predict ionospheric conditions on
an orbit-to-orbit basis for the 12-hour period following a twice-daily
model test and validation procedure. It was found that the best-fit m
odel often provided averaged (i.e., climatologically-based) accuracies
better than 5% in predicting the heights and critical frequencies of
the F-region peaks in the latitudinal domain of the TSS-1R flight path
. There was a sharp contrast however, in model-measurement comparisons
involving predictions of actual, unaveraged, along-track densities at
the 295 km orbital altitude of TSS-1R In this case, extrema in the fi
rst-principle models varied by as much as an order of magnitude in den
sity predictions, and the best-fit models were found to disagree with
the ''in situ'' observations of Ne by as much as 140%. The discrepanci
es are interpreted as a manifestation of difficulties in accurately an
d self-consistently modeling the external controls of solar and magnet
ospheric inputs and the spatial and temporal variabilities in electric
fields, thermospheric winds, plasmaspheric fluxes, and chemistry.