Astrophysics (Index)About

COSIE

(Coronal Spectrographic Imager in the EUV)
(EUV spectrograph to analyze the corona)

COSIE (for Coronal Spectrographic Imager in the EUV) is a proposed imager and spectrograph to view the Solar corona in the extreme ultraviolet (EUV). The spectrograph would be a slitless imaging spectrometer, aiming to produce "movies" of two frames per minute, each frame, in effect, a data cube with a spectral energy distribution for each pixel. This would be done by collecting multiple simultaneous 2D spectrums (multiple orders), with spectral and spatial data overlapping twice a minute, with post-processing to untangle the resulting data to produce tidy data cubes. This approach is means of capturing a spatial image, over time, with a SED for each pixel, showing the corona's observed structure and constant changes, and is a current strategy in observation of the corona. The plan is to deploy COSIE on the International Space Station (ISS).


(instrument,spectrograph,Sun,corona,plan)
Further reading:
https://ui.adsabs.harvard.edu/abs/2016AGUFMSH31C..08G/abstract
https://ntrs.nasa.gov/api/citations/20170007376/downloads/20170007376.pdf
https://www.swsc-journal.org/articles/swsc/full_html/2020/01/swsc200031/swsc200031.html
https://pweb.cfa.harvard.edu/facilities-technology/telescopes-instruments/coronal-spectrographic-imager-euv-cosie
https://ui.adsabs.harvard.edu/abs/2019ApJ...882...12W/abstract

Referenced by pages:
International Space Station (ISS)
solar physics

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