Imaging the Earth’s magnetic environment in soft X-rays with SMILE
- 1Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, UK
- 2University of Leicester, Leicester, UK
- 3National Space Science Center, Chinese Academy of Sciences, Beijing, China
- 4University of Alaska, Fairbanks, USA
It is a relatively recent discovery that charge exchange soft X-ray emission is produced in the interaction of solar wind high charge ions with neutrals in the Earth’s exosphere; this has led to the realization that imaging this emission will provide us with a global and novel way to study solar-terrestrial interactions.
In particular X-ray imaging will provide us with the means of establishing the location of the magnetopause and the morphology of the magnetospheric cusps. Variations of the magnetopause standoff distance indicate global magnetospheric compressions and expansions, both in response to solar wind variations and internal magnetospheric processes.
Soft X-ray imaging is one of the main objectives of SMILE (Solar wind Magnetosphere Ionosphere Link Explorer), a joint space mission by ESA and the Chinese Academy of Sciences, which is under development and is due for launch in 2023. This presentation will introduce the scientific aims of SMILE, show simulations of the expected images to be returned by SMILE’s Soft X-ray Imager for different solar wind conditions, and will discuss some of the techniques that will be applied in order to extract the positions of the Earth’s magnetic boundaries, such as the magnetopause standoff distance.
How to cite: Branduardi-Raymont, G., Sembay, S., Sun, T., Connor, H., and Samsonov, A.: Imaging the Earth’s magnetic environment in soft X-rays with SMILE, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-10877, https://doi.org/10.5194/egusphere-egu2020-10877, 2020