EGU24-6237, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-6237
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

SMILE: a new view on the dynamic magnetosphere

C.-Philippe Escoubet1 and the The SMILE team*
C.-Philippe Escoubet and the The SMILE team
  • 1ESA/ESTEC, SCI-S, Noordwijk, Netherlands (philippe.escoubet@esa.int)
  • *A full list of authors appears at the end of the abstract

How the solar wind and the Earth's magnetosphere interact, involving kinetic, fluid and global scales processes, is one of the key questions in space plasma physics. In situ instruments on a fleet of solar wind and magnetospheric constellation missions now provide the most detailed observations of Sun-Earth connections over multiple scales, from the smallest of a few kilometres up to the largest of a few 10s of Earth radii. However, we are still unable to fully quantify the global effects of the drivers of such connections, including the conditions that prevail throughout geospace due to the limitations of point measurements. This information is the key missing link for developing a complete understanding of how the Sun gives rise to and controls Earth's plasma environment and space weather. This is where SMILE (Solar wind Magnetosphere Ionosphere Link Explorer) comes in.

SMILE is a novel self-standing mission dedicated to observing the solar wind - magnetosphere coupling via simultaneous in situ solar ion and magnetic field measurements, soft X-ray imaging of the magnetosheath, magnetopause and polar cusps, and UV imaging of the northern hemisphere auroral oval. Remote sensing of the magnetosheath and cusps with soft X-ray imaging is made possible thanks to solar wind charge exchange (SWCX) X-ray emissions known to occur in the vicinity of the Earth's magnetosphere. SMILE is a joint mission between ESA and the Chinese Academy of Sciences (CAS) due for launch in the middle of 2025. SMILE science objectives as well as the latest scientific and technical developments, jointly undertaken by ESA, CAS and the international instrument teams, will be presented. SMILE will be complemented by ground-based observatories, in particular the newly funded Canada Space Agency SMILE Imaging Science project, as well as by theory and simulation investigations. This presentation will be dedicated to Graziella Branduardi-Raymont, SMILE mission Co-proposer and mission Co-PI, who passed away on 3rd November 2023.

The SMILE team:

C. P. Escoubet (ESA/ESTEC, The Netherlands), G. Branduardi-Raymont (MSSL/UCL, UK), C. Wang (NSSC/CAS, China), S. Sembay (University of Leicester, UK), L. Dai (NSSC/CAS, China), L. Li (NSSC/CAS, China), X.-X. Zhang (NCSW/CMA, China), J. Li (NSSC/CAS, China), D. Agnolon (ESA/ESTEC, The Netherlands), W. Raab (ESA/ESTEC, The Netherlands), C. Runciman (ESA/ESTEC, The Netherlands), B. Vanoutryve (ESA/ESTEC, The Netherlands), S. Vey (ESA/ESTEC, The Netherlands), A. Masson (ESA/ESAC, Spain), W. Chen (IAMC/CAS, China), X. Shi (IAMC/CAS, China), C. Forsyth (MSSL/UCL, UK), A. Read (University of Leicester, UK), E. Donovan (University of Calgary, Canada), E. L. Spanswick (University of Calgary, Canada), J. A. Carter (University of Leicester, UK), H. Connor (NASA/GSFC, USA), T. Sun (NSSC/CAS, China), A. Samsonov (MSSL/UCL, UK), J-H. Zheng (NSSC/CAS, China), S.-Y. Hsieh (JHU/APL, USA), D. Sibeck (NASA/GSFC, USA)

How to cite: Escoubet, C.-P. and the The SMILE team: SMILE: a new view on the dynamic magnetosphere, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6237, https://doi.org/10.5194/egusphere-egu24-6237, 2024.