{"id":20637,"date":"2021-05-24T20:44:00","date_gmt":"2021-05-24T14:59:00","guid":{"rendered":"https:\/\/www.revoscience.com\/en\/?p=20637"},"modified":"2021-05-24T20:44:21","modified_gmt":"2021-05-24T14:59:21","slug":"solar-orbiter-captures-first-coronal-mass-ejections","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/solar-orbiter-captures-first-coronal-mass-ejections\/","title":{"rendered":"Solar Orbiter Captures first coronal mass ejections"},"content":{"rendered":"\n<p>ESA\u2014Solar Orbiter launched on 10 February 2020 and is currently in cruise phase ahead\u00a0of the main science mission, which begins November this year. While the four\u00a0in situ instruments have been on for much of the time since launch, collecting science\u00a0data on the space environment in the vicinity of the spacecraft, the operation of the six remote sensing instruments during cruise phase\u00a0is focused primarily on instrument calibration, and they are\u00a0only active during dedicated checkout windows and specific campaigns.<\/p>\n\n\n\n<p>A close perihelion pass of the Sun on 10 February 2021, which took the spacecraft within half the distance between Earth and the Sun, was one such opportunity for the teams to carry out dedicated observations, checking instrument settings and so on, in order to best prepare for the upcoming science phase. In full science mode, the remote sensing and in situ instruments will routinely make joint observations together.<\/p>\n\n\n\n<figure class=\"wp-block-image size-large is-resized\"><img loading=\"lazy\" decoding=\"async\" sizes=\"auto, (max-width: 675px) 100vw, 675px\" src=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-675x477.jpg\" alt=\"\" class=\"wp-image-20638\" width=\"844\" height=\"596\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-675x477.jpg 675w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-566x400.jpg 566w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-768x543.jpg 768w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-1536x1086.jpg 1536w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-164x116.jpg 164w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg 1920w\" \/><\/figure>\n\n\n\n<p>At the same time as the close solar pass, the spacecraft was&nbsp;<a href=\"https:\/\/u7061146.ct.sendgrid.net\/ls\/click?upn=4tNED-2FM8iDZJQyQ53jATUSSvGwXoN-2FqusrCfZkpcKinV1h-2Fz7xwwcJ-2F-2FcFL570DO6ZrLCLaxJV0RbrbT9X5qoVZJdhO9iobbND34h4Kd8z9BoGLM0XDMB3hu8aYRa-2F1LgBNO_atJWz-2F57UhGGlDNlsqnR2CS5p8HPplAuHRkThiVrBX405lh-2Ff7bClnJXaP1gR2z3obRHiJQTkrsSWEF2-2FKEYi8t-2FnzJLGJ2R67NprETPKOlpFxX-2FYbe-2B-2Fn6TXTZKjmbanX39oTnTRBtH56zC5edz0p7dofQ0oXdHgLGKCBcOLoBCLR55sdcs0jHlIyLeknFB5wbyxi5MbSLhOgx9LTwr8LgUjDknxwyke4jjTlWnALBkie8s78EjL9Z23q0DiVzEhkar7IImnJ8bkkjwYEJgvUcjW5RymJ6Wi-2BuPrEBEnLKVzSAiWeKJJO2rCLClcBPnMOFgAeYeeQ83awa-2FGYrUUmD2ECRfE0r0NWsRc7dUvuQ-3D\" target=\"_blank\" rel=\"noreferrer noopener\">\u2018behind\u2019 the Sun<\/a>&nbsp;as viewed from Earth, resulting in very low data transfer rates. The data from the close flyby have therefore taken a long time to be completely downloaded and is still being&nbsp;analysed.<\/p>\n\n\n\n<h4 class=\"wp-block-heading\"><strong>Chance observations<\/strong><\/h4>\n\n\n\n<p>By happy coincidence, three of Solar Orbiter\u2019s remote sensing instruments captured a pair of coronal mass ejections in the days after closest approach. The Extreme Ultraviolet Imager (EUI), the Heliospheric Imager (SoloHI) and the Metis coronagraph captured different aspects of two CMEs that erupted over the course of the day.<\/p>\n\n\n\n<p>The CMEs were also seen by ESA\u2019s Proba-2 and the ESA\/NASA Solar and Heliospheric Observatory (SOHO) from the \u2018front\u2019 side of the Sun, while NASA&#8217;s STEREO-A, located away from the Sun-Earth line, also caught a glimpse,together providing a global view of the events.<\/p>\n\n\n\n<p>For Solar Orbiter\u2019s SoloHI, this was the first coronal mass ejection seen by the instrument; Metis previously detected one on 17 January, and EUI detected one in November last year, while the spacecraft\u2019s in situ detectors bagged their&nbsp;<a href=\"https:\/\/u7061146.ct.sendgrid.net\/ls\/click?upn=4tNED-2FM8iDZJQyQ53jATUd3WQ-2FzXULmuQnWbi51D4wnFKu9B82HKfUZLSmL5-2BYD9x5QWft8jeVHJ-2FbL1N7G8DPIN-2BWeLfm-2F6i0YqGA12l0xx5HePiDf1YIXqRJ9C3jYH9VE0iTYuBcBtayMJXZzR2Q-3D-3DN2g5_atJWz-2F57UhGGlDNlsqnR2CS5p8HPplAuHRkThiVrBX405lh-2Ff7bClnJXaP1gR2z3obRHiJQTkrsSWEF2-2FKEYi8t-2FnzJLGJ2R67NprETPKOlpFxX-2FYbe-2B-2Fn6TXTZKjmbanX39oTnTRBtH56zC5edz0p7dofQ0oXdHgLGKCBcOLoBCLR55sdcs0jHlIyLeknFB5wbyxi5MbSLhOgx9LTwr8OAMOvz9ocp-2FnWxD4C9paTXu5ZfNnr7UDS2YwHkquT-2FERgY42-2BcLfxrUKiu6tHPmjh9igM-2FXdGqccrNy9-2B-2FHo1uytMU1MtcKdfJixfplLHBNK6Siogrl0ChVfL1TLmwF5N2oQduUHPL8ujFUEnA3OcU-3D\" target=\"_blank\" rel=\"noreferrer noopener\">first CME&nbsp;<\/a>soon after launch in April 2020. Many of the in situ instruments also detected particle activity around the February 2021 CMEs; the data are being analysed and will be presented at a later date.<\/p>\n\n\n\n<p>For&nbsp;<a>SoloHI the<\/a>&nbsp;CME sighting was particularly serendipitous&nbsp;, captured during \u2018bonus\u2019 telemetry time. Upgrades in Earth-based antennas made since after the mission was planned allowed the team to downlink data at times they previously didn\u2019t expect to be able to, albeit at lower telemetry rates. They therefore decided to collect just one tile\u2019s worth of data (the instrument has four detector tiles) at a two-hour rate, and happened to capture a CME during that time.<\/p>\n\n\n\n<h4 class=\"wp-block-heading\"><strong>Space weather<\/strong><\/h4>\n\n\n\n<p>CMEs are an important part of \u2018space weather\u2019. The particles spark aurorae on planets with atmospheres, but&nbsp;can cause malfunctions in some technology&nbsp;and&nbsp;can also be harmful to unprotected astronauts. It&nbsp;is&nbsp;therefore&nbsp;important to understand CMEs, and be able to track their progress&nbsp;as they propagate through the Solar System.<\/p>\n\n\n\n<p>Studying CMEs is just one aspect of Solar Orbiter\u2019s mission. The spacecraft will also return&nbsp;unprecedented close-up observations of the Sun and from high solar&nbsp;latitudes, providing the first images of the uncharted polar regions of the Sun. Together with solar wind and magnetic field measurements in the vicinity of the spacecraft, the mission will provide new insight into how our parent star works&nbsp;in terms of the 11-year solar cycle, and how we can better predict periods of stormy space weather.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Solar Orbiter launched on 10 February 2020 and is currently in cruise phase ahead of the main science mission, which begins November this year.<\/p>\n","protected":false},"author":2,"featured_media":20638,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[20],"tags":[],"class_list":["post-20637","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-space-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",1920,1357,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-200x200.jpg",200,200,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-566x400.jpg",566,400,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-768x543.jpg",750,530,true],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-675x477.jpg",675,477,true],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-1536x1086.jpg",1536,1086,true],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",1920,1357,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",1132,800,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",806,570,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",600,424,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",600,424,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-760x490.jpg",760,490,true],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-550x360.jpg",550,360,true],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation-95x65.jpg",95,65,true],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",640,452,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",96,68,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2021\/05\/solarflair-observation.jpg",150,106,false]},"author_info":{"info":["RevoScience"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/news\/space-news\/\" rel=\"category tag\">Space\/ AstroPhysics<\/a>","tag_info":"Space\/ AstroPhysics","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/20637","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=20637"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/20637\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/20638"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=20637"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=20637"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=20637"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}