Real-Time UAF Eulerian Parallel Polar Ionosphere Model


Summary of Statistical Validation of the UAF EPPIM presented

at the NATO RTA conference "Characterising The Ionosphere"

IST-056/RSM-002, UAF, Fairbanks, Alaska, June 12-16, 2006


Figures of this section show

- Total number of statistical comparisons per year starting from 2002

- Mathematical definition of RMS & BIAS

- RMS and statistical biases calculated at representative stations for day-time conditions

- RMS and statistical biases calculated at representative stations for night-time conditions

- Comparison of RMS calculated for day and night conditions.

- Kp-dependence of RMS for different seasons and times of the day

- IMF Bz-dependence of RMS for different seasons and times of the day

- Dependence of night-time RMS & BIAS on geographic and deomagnetic latitude

- Dependence of day-time RMS & BIAS on geographic and deomagnetic latitude


Total number of statistical comparisons per year starting from 2002

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Mathematical definition of RMS & BIAS

Back to the list of Figures

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RMS and statistical biases calculated at representative stations for day-time conditions

Back to the list of Figures

Back to Ionospheric Model main page


RMS and statistical biases calculated at representative stations for night-time conditions

Back to the list of Figures

Back to Ionospheric Model main page


Comparison of RMS calculated for day and night conditions

Back to the list of Figures

Back to Ionospheric Model main page


Kp-dependence of RMS for different seasons and times of the day

Back to the list of Figures

Back to Ionospheric Model main page


IMF Bz-dependence of RMS for different seasons and times of the day

Back to the list of Figures

Back to Ionospheric Model main page


Dependence of night-time RMS & BIAS on geographic and deomagnetic latitude

Back to the list of Figures

Back to Ionospheric Model main page


Dependence of day-time RMS & BIAS on geographic and deomagnetic latitude

Back to the list of Figures

Back to Ionospheric Model main page



Back to Ionospheric Model main page