A global 3-D electron density reconstruction model based on radio occultation data and neural networks. (15th September 2021)
- Record Type:
- Journal Article
- Title:
- A global 3-D electron density reconstruction model based on radio occultation data and neural networks. (15th September 2021)
- Main Title:
- A global 3-D electron density reconstruction model based on radio occultation data and neural networks
- Authors:
- Habarulema, John Bosco
Okoh, Daniel
Burešová, Dalia
Rabiu, Babatunde
Tshisaphungo, Mpho
Kosch, Michael
Häggström, Ingemar
Erickson, Philip J.
Milla, Marco A. - Abstract:
- Abstract: The accurate representation of the ionospheric electron density in 3-dimensions is a challenging problem because of the nature of horizontal and vertical structures on both small and large scales. This paper presents the development of a global three-dimensional (3-D) electron density reconstruction based on radio occultation data during 2006–2019 and neural networks. We demonstrate that the developed model based on COSMIC dataset only is capable of reproducing different ionospheric features when compared to independent datasets from ionosondes and incoherent scatter radars (ISR) in low, middle and high latitude regions. Following some existing modelling efforts based on similar or related datasets and technique we divided the problem into fine resolution grid cells of 5 ∘ × 1 5 ∘ (geographic latitudes/longitudes) followed by development of the neural network subroutine per cell and later combining all the 864 sub-models to compile one global model. This approach has been demonstrated to be appropriate in enabling neural networks to learn, reproduce and generalise local and global behaviour of the ionospheric electron density. Based on ISR data, the 3D model improves maximum electron density of the F2 layer ( NmF2 ) prediction by 10%–20% compared to IRI 2016 model during quiet conditions. For estimation of ionosonde ordinary critical frequency of the F2 layer ( foF2 ) in 2009 at 1200 UT (universal time), the developed 3-D model gives average root mean square errorAbstract: The accurate representation of the ionospheric electron density in 3-dimensions is a challenging problem because of the nature of horizontal and vertical structures on both small and large scales. This paper presents the development of a global three-dimensional (3-D) electron density reconstruction based on radio occultation data during 2006–2019 and neural networks. We demonstrate that the developed model based on COSMIC dataset only is capable of reproducing different ionospheric features when compared to independent datasets from ionosondes and incoherent scatter radars (ISR) in low, middle and high latitude regions. Following some existing modelling efforts based on similar or related datasets and technique we divided the problem into fine resolution grid cells of 5 ∘ × 1 5 ∘ (geographic latitudes/longitudes) followed by development of the neural network subroutine per cell and later combining all the 864 sub-models to compile one global model. This approach has been demonstrated to be appropriate in enabling neural networks to learn, reproduce and generalise local and global behaviour of the ionospheric electron density. Based on ISR data, the 3D model improves maximum electron density of the F2 layer ( NmF2 ) prediction by 10%–20% compared to IRI 2016 model during quiet conditions. For estimation of ionosonde ordinary critical frequency of the F2 layer ( foF2 ) in 2009 at 1200 UT (universal time), the developed 3-D model gives average root mean square error (RMSE) values of 0.83 MHz, 1.06 MHz and 1.16 MHz compared to the IRI 2016 values of 0.92 MHz, 1.09 MHz and 1.01 MHz over the Africa–European, American and Asian sectors respectively making their performances statistically comparable. Compared to ionosonde data, the IRI 2016 model consistently shows a better performance for the hmF2 modelling results in almost all sectors during the investigated periods. Highlights: A 3D electron density reconstruction model is developed based only on radio occultation data and artificial neural networks. When benchmarked on the ISR, the developed model improves NmF2 prediction by 10%–20% compared to IRI 2016 model during quiet conditions. We suggest that the new model is applicable for future assimilation efforts especially over areas which are not sufficiently covered by ground-based instrumentation such as ionosondes. … (more)
- Is Part Of:
- Journal of atmospheric and solar-terrestrial physics. Volume 221(2021)
- Journal:
- Journal of atmospheric and solar-terrestrial physics
- Issue:
- Volume 221(2021)
- Issue Display:
- Volume 221, Issue 2021 (2021)
- Year:
- 2021
- Volume:
- 221
- Issue:
- 2021
- Issue Sort Value:
- 2021-0221-2021-0000
- Page Start:
- Page End:
- Publication Date:
- 2021-09-15
- Subjects:
- 3-dimensional electron density model -- Radio occultation data -- Artificial neural networks -- IRI 2016 model -- Incoherent scatter radar and ionosonde observations
Geophysics -- Periodicals
Atmospheric physics -- Periodicals
Géophysique -- Périodiques
Météorologie physique -- Périodiques
Electronic journals
551.51 - Journal URLs:
- http://www.sciencedirect.com/science/journal/13646826 ↗
http://www.elsevier.com/journals ↗ - DOI:
- 10.1016/j.jastp.2021.105702 ↗
- Languages:
- English
- ISSNs:
- 1364-6826
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4947.950000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 17611.xml