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\t\t\t\t\t\t02\/01\/2024<\/span> Through exquisite, millimetre-scale, formation flying, the dual satellites making up ESA\u2019s Proba-3 will accomplish what was previously a space mission impossible: cast a precisely held shadow from one platform to the other, in the process blocking out the fiery Sun to observe its ghostly surrounding atmosphere on a prolonged basis.<\/p>\n<\/div>\n Ahead of the Proba-3 pair launching together later this year, the scientists who will make use of Proba-3 observations were able to see the satellites with their own eyes. Members of this team will test hardware developed for the mission during an actual terrestrial solar eclipse over Northern America next April.<\/p>\n The two satellites are currently undergoing final integration in the premises of Redwire near Antwerp in Belgium. They were paid a visit by the Proba-3 Science Working Team, a 45-strong group of solar physicists coming from all across Europe and the wider world.<\/p>\n<\/p><\/div>\n Many of these experts are regular visitors to terrestrial solar eclipse around the globe but are looking forward to the new perspective Proba-3 will open up on the faint solar corona. This mysterious region is important as the place where coronal mass ejections are created \u2013 vast eruptions of charged particles that trigger solar storms \u2013 as well as influencing the velocity of the solar wind, which is central to determining space weather.<\/p>\n \u201cThe satellite hardware was quite something in close up,\u201d explains Joe Zender, ESA\u2019s Proba-3 project scientist. \u201cI was particularly struck by how close the camera head on the Coronagraph spacecraft is to the solar array, less than a metre away. While the array relies on high solar illumination, the camera has to remain in complete darkness, with no stray light whatsoever. It really brings it home how precisely that small shadow cast by the Occulter will need to be maintained in place. We also got a peek at the carefully-machined edge of the Occulter spacecraft\u2019s disc \u2013 normally kept under protective cover before launch. The curve of this edge has been specially designed to minimise any spillover of diffracted sunlight that would otherwise impact imaging performance.\u201d<\/p>\n<\/p><\/div>\n Also present was noted US astrophysicist Russell Howard of the John Hopkins University Applied Physics Lab, who played a leading role in NASA\u2019s Parker Solar Probe and the ESA-NASA SOHO mission: \u201cThe spacecraft are smaller than the ones that I have been involved with \u2013 primarily because this is a single solar viewing instrument with two much smaller instruments. But the mission concept is so unique: placing an occulter 150 meters from the telescope to allow imaging extremely close to the limb of the Sun has never been done before, as though the Occulter spacecraft is a mini-Moon. We won\u2019t see quite as close to the solar limb as during a terrestrial eclipse, but having such images for hours on end compared to the 5-10 minutes duration of an eclipse event will be spectacular.\u201d<\/p>\n<\/p><\/div>\n Progressing on to the Royal Observatory of Belgium in Brussels, the team went on to discuss preparations for the mission in Brussels, including plans to process and distribute its data, plan co-observations with other space missions and assess Proba-3\u2019s relative performance compared to existing \u2018coronagraph\u2019 instruments employed for coronal observations.<\/p>\n These are telescopes that incorporate internal occulting discs to obscure the solar disc. The problem is that these internal occulters still experience light spilling around their edges, known as diffraction, blotting out the extremely faint signals of interest.<\/p>\n<\/p><\/div>\n Damien Galano, ESA\u2019s Proba-3 project manager notes: \u201cThe best way to reduce diffraction is to increase the distance between the occulter and the coronagraph, which is precisely what Proba-3 is going to do. We are flying our Coronagraph and Occulter on separate platforms for the first time, flying 150 m apart for up to six hours per orbit, applying an array of positioning technologies to keep them rigidly in place.\u201d<\/p>\n By definition, full-scale end-to-end testing of Proba-3 is impossible here on Earth. But the meeting heard how the same set of filter wheels developed for Proba-3\u2019s ASPIICS (Association of Spacecraft for Polarimetric and Imaging Investigation of the Corona of the Sun) will be used to observe the solar eclipse over Northern America on 8 April 2024, along with a parallel liquid crystal imaging technology.<\/p>\n<\/p><\/div>\n \u201cThe filter wheels allow observation of the corona in different polarisation angles, like switching between different polarised sunglasses,\u201d adds Joe. \u201cThe nice about observing during an actual eclipse is we won\u2019t need any occulter, to gain insight of exactly the kind of results we are going to get back from Proba-3.\u201d<\/p>\n The Science Working Team also discussed Proba-3\u2019s second instrument, the Digital Absolute Radiometer, DARA, which will measure the total solar irradiance \u2013 exactly how much the energy the Sun is putting out at any one time.\u00a0<\/p>\n \u201cAssuming the Sun\u2019s output\u2019s influences Earth\u2019s climate, it\u2019s important to measure any variations as precisely as we can,\u201d notes Joe.<\/p>\n Proba-3 is due for launch in September this year, by PSLV launcher from India.<\/p>\n<\/p><\/div>\n
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