Medium-term predictions of F10.7 and F30 cm solar radio flux with the adaptive Kalman filter
Elena Petrova, Tatiana Podladchikova, Astrid M. Veronig, Stijn, Lemmens, Benjamin Bastida Virgili, Tim Flohrer

TL;DR
This paper introduces RESONANCE, a novel adaptive Kalman filter-based method for medium-term prediction of solar radio flux indices F10.7 and F30, improving accuracy for space weather and re-entry forecasting.
Contribution
The paper presents a new prediction framework combining noise reduction, initial forecasting, and adaptive Kalman filtering, outperforming existing methods in accuracy.
Findings
Prediction RMSE for F10.7 is 5-27 sfu for 1-24 months ahead.
Prediction RMSE for F30 is 3-16 sfu for 1-24 months ahead.
Improved predictions enhance re-entry epoch forecasts for space debris.
Abstract
The solar radio flux at F10.7 cm and F30 cm is required by most models characterizing the state of the Earth's upper atmosphere, such as the thermosphere and ionosphere to specify satellite orbits, re-entry services, collision avoidance maneuvers and modeling of space debris evolution. We develop a method called RESONANCE ("Radio Emissions from the Sun: ONline ANalytical Computer-aided Estimator") for the prediction of the 13-month smoothed monthly mean F10.7 and F30 indices 1-24 months ahead. The prediction algorithm includes three steps. First, we apply a 13-month optimized running mean technique to effectively reduce the noise in the radio flux data. Second, we provide initial predictions of the F10.7 and F30 indices using the McNish-Lincoln method. Finally, we improve these initial predictions by developing an adaptive Kalman filter with the error statistics identification. The…
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