SMILE is a space mission which aims to measure Earth's global system responses to solar wind and geomagnetic variations.
SMILE will investigate the dynamic response of the Earth's magnetosphere to the impact of the solar wind in a unique manner, never attempted before: it will combine soft X-ray imaging of the Earth's magnetopause and magnetospheric cusps with simultaneous UV imaging of the Northern aurora.
For the first time we will be able to trace and link the processes of solar wind injection in the magnetosphere with those acting on the charged particles precipitating into the cusps and eventually the aurora.
SMILE will also carry in-situ instrumentation to monitor the solar wind and magnetosheath plasma conditions, so that the simultaneous X-ray and UV images can be compared and contrasted directly, and self-sufficiently, with the upstream and local driving conditions.
SMILE was put forward in March 2015 in response to the European Space Agency and Chinese Academy of Sciences joint call for a small-size space mission. The Executive Summary of the submitted proposal can be found here.
Out of 13 missions originally proposed, SMILE was the one chosen for an initial study phase during the summer of 2015. An initial study of the whole mission was carried out by ESA and CAS at their Concurrent Design Facilities during October 2015, and the conclusion was that the mission is feasible, with no show stoppers. In early November 2015 SMILE was formally selected by the ESA Science Programme Committee. We are now in Phase B of the project, with the objective of reaching mission adoption in 2018. Launch is expected to take place in 2023.
Scientists and engineers from the UK, China, Canada, several European countries and the US are collaborating in order to make SMILE a reality.
Please join our team of supporters by following this link.
Above is a series of simulated images for the SMILE Soft X-ray Imager (SXI). On the left is an image of simulated X-ray emission, constructed using input from a magnetohydrodynamic model of the dayside magnetosheath. This simulation was run for a period of solar wind that followed a southward turning of the interplanetary magnetic field. The middle image shows raw SXI counts, integrated over 300 seconds. On the right hand side is the SXI counts image following a step of image deconvolution to account for blurring by the point spread function of the SXI optical system. The SXI field of view for a nominal pointing position is shown by the white square. The UV Imager field of view is shown by the orange square. The approximate magnetopause and bow shock boundaries, plus the position of the Earth, are also overlaid on the images in white.
More information about the SXI simulations can be found at this link.