{"id":1208,"date":"2021-10-23T13:49:00","date_gmt":"2021-10-23T13:49:00","guid":{"rendered":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/?p=1208"},"modified":"2025-02-26T13:37:27","modified_gmt":"2025-02-26T13:37:27","slug":"major-step-in-uk-contribution-to-space-mission-to-study-solar-wind","status":"publish","type":"post","link":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/2021\/10\/23\/major-step-in-uk-contribution-to-space-mission-to-study-solar-wind\/","title":{"rendered":"Major step in UK contribution to space mission to study solar wind"},"content":{"rendered":"\n<p><strong><em>Space scientists from the University of Leicester have delivered a key component for a new mission to study the impact of the solar wind on Earth\u2019s magnetic field.<\/em><\/strong><br><br><\/p>\n\n\n\n<p>Engineers from the University\u2019s Space Research Centre have completed the structural and thermal model for the UK\u2019s latest X-ray telescope, the Soft X-ray Imager (SXI), destined for space aboard the SMILE (Solar wind Magnetosphere Ionosphere Link Explorer) probe when it launches at the end of 2024.<br><br><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"aligncenter size-large is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/Untitled-1024x575.jpg\" alt=\"\" class=\"wp-image-1210\" width=\"658\" height=\"369\" srcset=\"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/Untitled-1024x575.jpg 1024w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/Untitled-300x168.jpg 300w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/Untitled-768x431.jpg 768w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/Untitled.jpg 1532w\" sizes=\"auto, (max-width: 658px) 100vw, 658px\" \/><figcaption>(L-R) Chris Bicknell, Charlotte Bouldin and Andy Cheney completing final work on the SXI structural and thermal model prior to delivery to Airbus, Spain. Credit: University of Leicester<\/figcaption><\/figure><\/div>\n\n\n\n<p>The model, which has now been delivered to Airbus in Spain for integration and testing within the prototype satellite system, is not the so-called flight model \u2013 but will help engineers understand the extreme requirements for the final design.<br><br><\/p>\n\n\n\n<p>Specialists will subject the prototype to the significant vibrations, shocks and G-forces experienced during launch of the spacecraft, as well as the extreme temperatures it must operate at in space below -150<sup>o<\/sup>C.<br><br><\/p>\n\n\n\n<p>Dr Steven Sembay, Principal Investigator (PI) for the SXI instrument, based at the University of Leicester, said: \u201cThe STM testing is always a slightly nervous time, especially when you see videos of how much the instrument is shaken during testing!\u00a0<br><br><\/p>\n\n\n\n<p>\u201cIt is the first time you go from conceptual design in computer models to a real object in metal. I shouldn\u2019t have worried. It is a testament to the skill of our engineering and manufacturing team that what is a complex piece of kit works as predicted.\u201d<br><br><\/p>\n\n\n\n<p>The SXI consortium is led by the University of Leicester in collaboration with UCL Mullard Space Science Laboratory (UCL MSSL), the Open University and European partners.\u00a0<br><br><\/p>\n\n\n\n<p>UCL MSSL is responsible for building the electronics that operate the SXI detectors and retrieve the signals that produce X-ray images of the space around the Earth.<br><br><\/p>\n\n\n\n<p>The UK Space Agency has committed \u00a310.5 million in funding for UK leadership roles on SMILE, including the SXI instrument. The compact X-ray telescope is the only European instrument planned for the mission.<br><br><\/p>\n\n\n\n<p>SMILE is the first joint project between the European Space Agency (ESA) and the Chinese Academy of Sciences (CAS) from conceptual design to operations, and will study the continuous stream of charged particles emitted by our Sun.\u00a0<br><br><\/p>\n\n\n\n<div class=\"wp-block-image\"><figure class=\"aligncenter size-large is-resized\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/sxi-1024x575.jpg\" alt=\"\" class=\"wp-image-1209\" width=\"660\" height=\"370\" srcset=\"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/sxi-1024x575.jpg 1024w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/sxi-300x168.jpg 300w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/sxi-768x431.jpg 768w, https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/files\/2021\/11\/sxi.jpg 1408w\" sizes=\"auto, (max-width: 660px) 100vw, 660px\" \/><figcaption>SMILE&#8217;s Soft X-ray Imager structural and thermal model arrives at Airbus, Spain. Credit: Airbus<\/figcaption><\/figure><\/div>\n\n\n\n<p><br><br><\/p>\n\n\n\n<p>Professor Graziella Branduardi-Raymont of UCL MSSL, European Co-Principal Investigator for the mission, said: \u201cOne of the most interesting aspects of SMILE SXI is the fact that we are using technology so far applied for looking outwards to X-ray sources in the far Universe to study how our own Earth responds to the impact of the Sun\u2019s activity.\u201d\u00a0<br><br><\/p>\n\n\n\n<p>The highly variable stream of high energy particles, called the solar wind, impacts on the Earth\u2019s magnetic field. At times of high intensity this stream can be a hazard to space-based instrumentation or even, in rare cases, ground-based electrical systems.<br><br><\/p>\n\n\n\n<p>Fortunately, the Earth\u2019s magnetic field provides protection, but this compresses and expands as it responds to variations in the highly dynamic solar wind.<br><br><\/p>\n\n\n\n<p>SXI will continuously monitor the position of the boundary between the region of space controlled by the Earth\u2019s magnetic field and the solar wind. Its images will, in conjunction with the other instruments on SMILE, help scientists to refine models of how this Sun-Earth connection responds to the most infamous example of so-called \u2018space weather\u2019.<br><br><\/p>\n\n\n\n<p>Dr Caroline Harper, Head of Space Science at the UK Space Agency, said: \u201cSpace weather \u2013 such as the solar wind \u2013 has the potential to disrupt satellites we rely on every day for services such as global communications or managing power grids.<br><br><\/p>\n\n\n\n<p>\u201cThis mission is a prime example of how, by working with our international partners, the UK is doing innovative science in space, while underpinning the broader economy by supporting the development of real-world applications, such as space weather modelling. It is fantastic to see the first full model of the SXI instrument being delivered and we look forward to the completion of the engineering model and eventually the flight instrument, over the next two years.\u201d<br><br><\/p>\n\n\n\n<p>SXI weighs around 36 kg and needed to be compact and relatively low mass to meet the mission level requirements of the spacecraft. To achieve this the telescope employs a very lightweight optical system to focus X-rays; a \u2018lobster-eye\u2019 lens which mimics the mechanism within the eye of a crustacean.<br><br><\/p>\n\n\n\n<p>The University of Leicester\u2019s Space Research Centre is a world leader in the development of X-ray instruments for space and SMILE\u2019s SXI is the third instrument to use similar optics to be built at Leicester following the Mercury Imaging X-ray Spectrometer (MIXS) instrument on ESA\u2019s BepiColombo, which has recently successfully completed its first fly-by of destination planet Mercury, and the soon-to-be-launched MXT instrument on the French-Chinese SVOM mission.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Space scientists from the University of Leicester have delivered a key component for a new mission to study the impact of the solar wind on Earth\u2019s magnetic field. Engineers from the University\u2019s Space Research Centre have completed the structural and thermal model for the UK\u2019s latest X-ray telescope, the Soft X-ray Imager (SXI), destined for [&hellip;]<\/p>\n","protected":false},"author":256,"featured_media":1210,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[6,10,20],"tags":[],"class_list":["post-1208","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-earth","category-planetary","category-space"],"_links":{"self":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1208","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/users\/256"}],"replies":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/comments?post=1208"}],"version-history":[{"count":1,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1208\/revisions"}],"predecessor-version":[{"id":1211,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/posts\/1208\/revisions\/1211"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/media\/1210"}],"wp:attachment":[{"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/media?parent=1208"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/categories?post=1208"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/staffblogs.le.ac.uk\/physicsastronomy\/wp-json\/wp\/v2\/tags?post=1208"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}