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SOLAR SCIENCE
Smile payload module travels to China
by Staff Writers
Paris (ESA) Mar 17, 2022

Integration onto the Chinese platform is expected to begin in early April. Once the complete satellite is finished, it will undergo a comprehensive five month long qualification test campaign including thermal, mechanical, electromagnetic compatibility testing, and magnetic, deployment and functional tests at system level.

Following a successful test campaign in Europe, the structural thermal model of the Solar wind Magnetosphere Ionosphere Link Explorer (Smile)'s payload module will soon be delivered to China to complete the qualification of the satellite.

Smile is a joint mission between ESA and the Chinese Academy of Sciences (CAS) and will aim to build a more complete understanding of the Sun-Earth connection by measuring the solar wind and its dynamic interaction with the magnetosphere.

The payload module recently completed thermal testing and a deployment test of the magnetometer instrument boom at ESA's technical heart in the Netherlands. The module then returned to Airbus in Spain for mechanical testing, completing the environmental test campaign phase that lasted three months.

Integration onto the Chinese platform is expected to begin in early April. Once the complete satellite is finished, it will undergo a comprehensive five month long qualification test campaign including thermal, mechanical, electromagnetic compatibility testing, and magnetic, deployment and functional tests at system level.


Related Links
Solar wind Magnetosphere Ionosphere at ESA
Solar Science News at SpaceDaily


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Telescopes trained on Parker Solar Probe's latest pass around the Sun
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As NASA's Parker Solar Probe completes its latest swing around the Sun, it's doing so in full view of dozens of other spacecraft and ground-based telescopes. These powerful instruments can't actually see Parker itself - the van-sized spacecraft is far too small for visible detection - but they offer from a distance what the probe is sensing close-up, as it samples and analyzes the solar wind and magnetic fields from as close as 5.3 million miles (8.5 million kilometers) from the Sun's surface. ... read more

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