EGU25-12224, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-12224
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Using novel remote sensing techniques to enhance local prediction models of ionosphericresponse to space weather: a RISER project approach
Paul Kinsler1, Biagio Forte2, Tianchu Lu2, Mario Bisi3, Steve Milan4, David Jackson5, Richard Fallows3, Bernard Jackson6, Dusan Odstrcil7, Edmund Henley5, David Barnes3, Oyuki Chang3, Matthew Bracamontes6, and Siegfried Gonzi5
Paul Kinsler et al.
  • 1Electronic and Electrical Engineering, University of Bath, United Kingdom (dr.paul.kinsler@physics.org)
  • 2Electronic and Electrical Engineering, University of Bath, United Kingdom
  • 3Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
  • 4University of Leicester, Leicester, United Kingdom
  • 5Met Office, Exeter, United Kingdom
  • 6University of California San Diego, CA, United States
  • 7George Mason University, Fairfax, United States

Novel remote-sensing techniques can be used to inject vital "oncoming storm" data into upgraded prediction models. Here we present several possibilities being investigated under the auspices of the RISER project, whose goal is to improve space weather forecast times by up to four days, as well as their accuracy. Here, in this early stage of the project one strand is to investigate how best to integrate such new data. We describe how to leverage the capabilities of our existing IONwork software to produce GNSS-based TEC disturbance maps, and use that processed data in concert with information from the heliosphere to create remote-plus-local combined prediction models, comparing both traditional and machine learning techniques. Heliospheric information can be extracted, for example, from L1 monitors: however, within the RISER project we aim at expanding the heliospheric information available by including observations of interplanetary scintillation and corresponding tomographic reconstructions to map solar-wind or CME features structures present in the Sun-Earth interplanetary space. Such extended data will also provide longer lead times than the approximately one hour advance notice given by L1 data, making it easier to create forecasts that are both timely and more accurate.

How to cite: Kinsler, P., Forte, B., Lu, T., Bisi, M., Milan, S., Jackson, D., Fallows, R., Jackson, B., Odstrcil, D., Henley, E., Barnes, D., Chang, O., Bracamontes, M., and Gonzi, S.: Using novel remote sensing techniques to enhance local prediction models of ionosphericresponse to space weather: a RISER project approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12224, https://doi.org/10.5194/egusphere-egu25-12224, 2025.