000005328 001__ 5328
000005328 005__ 20210329095214.0
000005328 037__ $$aSCART-2021-0077
000005328 100__ $$aHarra, Louise 
000005328 245__ $$aA Spectral Solar Irradiance Monitor (SoSpIM) on the JAXA Solar-C Space Mission
000005328 260__ $$c2021
000005328 520__ $$aAs a fundamental step towards answer- ing how the plasma universe is creat- ed and evolves, and how the Sun influ- ences the Earth and other planets in our solar system, the JAXA Solar-C mission (Shimizu et al., 2020) is designed to com- prehensively understand how mass and energy are transferred throughout the solar atmosphere. The EUV High-Throughput Spectroscopic Telescope (EUVST) onboard does this by observing all the temperature regimes of the atmosphere from the chromosphere to the corona sim- ultaneously. As well as the EUVST, there will be a Solar Spectral Irradiance Moni- tor (SoSpIM).
000005328 594__ $$aSTCE
000005328 700__ $$aAlberti, Andrea 
000005328 700__ $$aBerghmans, David
000005328 700__ $$aDominique, Marie 
000005328 700__ $$aGissot, Samuel 
000005328 700__ $$aHara, Hirohisa 
000005328 700__ $$aImada, Shinsuke 
000005328 700__ $$aKoller, Silvio 
000005328 700__ $$aKrucker, Säm 
000005328 700__ $$aPfiffner, Daniel 
000005328 700__ $$aRozanov, Eugene 
000005328 700__ $$aShimizu, Toshifumi 
000005328 700__ $$aSukhodolov, Timofei 
000005328 700__ $$aTye, Daniel 
000005328 700__ $$aWatanabe, Kyoko 
000005328 773__ $$c1-2$$pSCOSTEP/PRESTO NEWSLETTER$$v27$$y2021
000005328 8560_ $$fdavid.berghmans@observatoire.be
000005328 905__ $$ain press to
000005328 980__ $$aNONREF