The First Flight of the Marshall Grazing Incidence X-Ray Spectrometer (MaGIXS)

Author:

Savage Sabrina L.ORCID,Winebarger Amy R.ORCID,Kobayashi KenORCID,Athiray P. S.ORCID,Beabout Dyana,Golub LeonORCID,Walsh Robert W.ORCID,Beabout Brent,Bradshaw StephenORCID,Bruccoleri Alexander R.ORCID,Champey Patrick R.ORCID,Cheimets Peter,Cirtain Jonathan,DeLuca Edward E.ORCID,Del Zanna GiulioORCID,Dudík JaroslavORCID,Guillory Anthony,Haight Harlan,Heilmann Ralf K.ORCID,Hertz EdwardORCID,Hogue William,Kegley Jeffery,Kolodziejczak Jeffery,Madsen ChadORCID,Mason HelenORCID,McKenzie David E.ORCID,Ranganathan Jagan,Reeves Katharine K.ORCID,Robertson Bryan,Schattenburg Mark L.ORCID,Scholvin Jorg,Siler Richard,Testa PaolaORCID,Vigil Genevieve D.ORCID,Warren Harry P.ORCID,Watkinson Benjamin,Weddendorf Bruce,Wright Ernest

Abstract

Abstract The Marshall Grazing Incidence X-ray Spectrometer (MaGIXS) sounding rocket experiment launched on 2021 July 30 from the White Sands Missile Range in New Mexico. MaGIXS is a unique solar observing telescope developed to capture X-ray spectral images of coronal active regions in the 6–24 Å wavelength range. Its novel design takes advantage of recent technological advances related to fabricating and optimizing X-ray optical systems, as well as breakthroughs in inversion methodologies necessary to create spectrally pure maps from overlapping spectral images. MaGIXS is the first instrument of its kind to provide spatially resolved soft X-ray spectra across a wide field of view. The plasma diagnostics available in this spectral regime make this instrument a powerful tool for probing solar coronal heating. This paper presents details from the first MaGIXS flight, the captured observations, the data processing and inversion techniques, and the first science results.

Funder

NASA ∣ SMD ∣ Heliophysics Division

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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