Bayesian filtering in incoherent scatter plasma parameter fits
• +2
• Ilkka I. Virtanen,
• Habtamu W. Tesfaw,
• Lassi Roininen,
• Sari Lasanen,
• Anita T. Aikio
Ilkka I. Virtanen
University of Oulu, University of Oulu, University of Oulu

Corresponding Author:ilkka.i.virtanen@oulu.fi

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Habtamu W. Tesfaw
University of Oulu, University of Oulu, University of Oulu
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Lassi Roininen
Lappeenranta-Lahti University of Technology, Lappeenranta-Lahti University of Technology, Lappeenranta-Lahti University of Technology
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Sari Lasanen
University of Oulu, University of Oulu, University of Oulu
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Anita T. Aikio
University of Oulu, University of Oulu, University of Oulu
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## Abstract

Incoherent scatter (IS) radars are invaluable instruments for ionospheric physics, since they observe altitude profiles of electron density ($N_e$), electron temperature ($T_e$), ion temperature ($T_i$) and line-of-sight plasma velocity ($V_i$) from ground. However, the temperatures can be fitted to the observed IS spectra only when the ion composition is known, and resolutions of the fitted plasma parameters are often insufficient for auroral electron precipitation, which requires high resolutions in both range and time. The problem of unknown ion composition has been addressed by means of the full-profile analysis, which assumes that the plasma parameter profiles are smooth in altitude, or follow some predefined shape. In a similar manner, one could assume smooth time variations, but this option has not been used in IS analysis. We propose a plasma parameter fit technique based on Bayesian filtering, which we have implemented as an additional Bayesian Filtering Module (BAFIM) in the GUISDAP analysis package. BAFIM allows us to control gradients in both time and range directions for each plasma parameter separately. With BAFIM we can fit F$_1$ region ion composition together with $N_e, T_e, T_i$ and $V_i$, and we have reached 4~s/900~m time/range steps in four-parameter fits of $N_e, T_e, T_i$ and $V_i$ in E region observations of auroral electron precipitation.
Mar 2021Published in Journal of Geophysical Research: Space Physics volume 126 issue 3. 10.1029/2020JA028700