EGU24-13334, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-13334
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The RADiation Impacts on Climate and Atmospheric Loss Satellite (RADICALS) Mission

Louis Ozeke1, Ian Mann1, Christopher Cully2, David Milling1, Michael Lipsett1, Robert Ranking1, Kathryn McWilliams3, Robyn Fiori4, David Cullen1, Robert Fedosejevs1, Greg Enno1, Robert Zee5, Martin Conners6, William Ward7, Leonid Olifer1, Robert Marshall8, David Barona1, Andrew Yau2, and Andrew Howarth2
Louis Ozeke et al.
  • 1Department of Physics, University of Alberta, Edmonton, Canada (lozeke@ualberta.ca)
  • 2University of Calgary Calgary, Canada
  • 3University of Saskatchewan Saskatoon, Canada
  • 4Natural Resources Canada Ottawa, Canada
  • 5University of Toronto Toronto, Canada
  • 6Athabasca University Athabasca, Canada
  • 7University of New Brunswick Fredericton, Canada
  • 8University of Colorado at Boulder, Boulder, United States

The RADiation Impacts on Climate and Atmospheric Loss Satellite (RADICALS) is a low-Earth orbiting Canadian small satellite mission investigating the transport of space radiation into the atmosphere, and its impact on Earth’s climate. Scheduled for launch in late 2026, the mission will launch into a polar orbit with an integrated payload comprising two back-to-back look direction High Energy Particle (HEP) telescopes, an X-Ray Imager (XRI) to remote sense energetic particle precipitation using back-scattered Bremsstrahlung X-rays, and a boom mounted FluxGate Magnetometer (FGM) and Search Coil Magnetometer (SCM). Using an innovative Thomson spin-stabilized configuration, the satellite will sample the pitch angle distributions in the spin-plane twice per spin. The back-to-back HEP look directions allow for a contemporaneous view of the down-going and back-scattered up-going electrons, at the same time as XRI remote-senses the related Bremsstrahlung, and the magnetometers provide in-situ magnetic signatures of a range of plasma waves. The key measurement of the pitch angle resolved energetic electron precipitation (EEP) and related back-scatter, including a resolved loss cone, will allow a detailed assessment of the energetic particle energy input to the atmosphere. Measurements of EEP, in addition to measurements of solar energetic particle (SEP) precipitation, will represent a critical data set for assessing the role of space radiation in the climate system, for example through the catalytic destruction of ozone in the middle atmosphere by NOx and HOx. Accurately quantifying the impacts of this space radiation on climate requires accurate and loss cone-resolved characterization of the flux of these precipitating energetic particles for inclusion into whole atmosphere models. The RADICALS explorer will also enable research into potentially catastrophic space-weather radiation effects on satellite infrastructure, and assess impacts on space weather-related interruptions to high frequency radio communications including in relation to aircraft operations in polar regions. Additional cube- and micro-satellite missions, together with the RADICALS, could form a powerful mini--constellation exploring the space weather-climate system.

How to cite: Ozeke, L., Mann, I., Cully, C., Milling, D., Lipsett, M., Ranking, R., McWilliams, K., Fiori, R., Cullen, D., Fedosejevs, R., Enno, G., Zee, R., Conners, M., Ward, W., Olifer, L., Marshall, R., Barona, D., Yau, A., and Howarth, A.: The RADiation Impacts on Climate and Atmospheric Loss Satellite (RADICALS) Mission, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13334, https://doi.org/10.5194/egusphere-egu24-13334, 2024.