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The Coronal Microscale ObservatoryIt has been a longstanding challenge to identify the mechanisms responsible for heating the solar corona, in part because heating, whether by waves or magnetic reconnection, is thought to be concentrated in thus far unresolved volumes with characteristic scales ≲100 km. The Coronal Microscale Observatory (CMO) is a mission concept designed to image these microscale heating events, identify the dominant physical mechanisms that control their initiation and evolution, and understand their effects on the formation of the solar wind. CMO positions three spacecraft and three instruments near the Sun-Earth L1 Lagrange point. One instrument is a cluster of 6 coaligned extreme ultraviolet (EUV) telescopes that image a common field of view with ultrahigh angular resolution (0.02−0.07 arcsec) in narrow wavelength bands, each sensitive to emission from plasma in a limited temperature range. The second instrument is a multi-band, full-disk, externally occulted coronagraph. Finally, a two-band fine scale EUV imager (resolution 0.3 arcsec) provides a larger field of view for context and additional science. The three CMO craft fly in precise formation to ensure that the EUV imagers point to a desired target on the Sun and the external occulter accurately blocks the solar disk. The novel mission architecture arises from the intrinsically long EUV focal length (≳100 m) of diffractive optics known as photon sieves, which achieve nearly diffraction-limited EUV imaging but require a distributed telescope, in which the optics and- the image sensors are on separate spacecraft. Two spacecraft are also needed to position an external occulter 200 m in front of the coronagraph, which enables visible-light imaging of the corona very close to the solar limb with undiminished angular resolution. Recent advances in fabricating ultraprecise and smooth reflective optics suggest that a conventional (single spacecraft)EUV “microscope” may now be feasible in an Explorer-class mission that could achieve a subset of the scientific objectives of CMO.
Document ID
20240002307
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Douglas Rabin
(Goddard Space Flight Center Greenbelt, United States)
Anne-marie D Novo-gradac
(Goddard Space Flight Center Greenbelt, United States)
Amy Renee Winebarger
(Marshall Space Flight Center Redstone Arsenal, United States)
Matthew John West
(Southwest Research Institute Boulder, CO, United States)
Nicholeen Mary Viall-kepko
(Goddard Space Flight Center Greenbelt, United States)
Daniel B Seaton
(Southwest Research Institute San Antonio, United States)
Nelson Leslie Reginald
(Catholic University of America Washington D.C., District of Columbia, United States)
Eliad Peretz
(Goddard Space Flight Center Greenbelt, United States)
Jacob D Parker
(Goddard Space Flight Center Greenbelt, United States)
Jeffrey S Newmark
(Goddard Space Flight Center Greenbelt, United States)
Emily Irene Mason
(Predictive Science (United States) San Diego, California, United States)
James Andrew Klimchuk
(Goddard Space Flight Center Greenbelt, United States)
Farzad Kamalabadi
(University of Illinois Urbana-Champaign Urbana, United States)
Leon Golub
(Center for Astrophysics Harvard & Smithsonian Cambridge, Massachusetts, United States)
Kevin Leon Denis
(Goddard Space Flight Center Greenbelt, United States)
Ineke De Moortel ORCID
(University of St Andrews St Andrews, United Kingdom)
Adrian Nigel Daw
(Goddard Space Flight Center Greenbelt, United States)
Steven D Christie
(Goddard Space Flight Center Greenbelt, United States)
Phillip C Chamberlin ORCID
(University of Colorado Boulder Boulder, United States)
Date Acquired
February 22, 2024
Subject Category
Solar Physics
Meeting Information
Meeting: Triennial Earth-Sun Summit (TESS)
Location: Dallas, TX
Country: US
Start Date: April 7, 2024
End Date: April 12, 2024
Sponsors: American Geophysical Union
Funding Number(s)
WBS: 981698.01.04.51.01.60.12
CONTRACT_GRANT: 80JSC023DA008
CONTRACT_GRANT: 80NSSC23K1323
CONTRACT_GRANT: 80NSSC21M0180
CONTRACT_GRANT: MOU- NOAA
CONTRACT_GRANT: HQ-NASA-HPAC
CONTRACT_GRANT: 80GSFC21CA007
CONTRACT_GRANT: NNM07AB07C
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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