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Orbiting Artificial Star for High-Resolution Coronal Imaging from the GroundThis paper establishes the scientific motivation of the Orbiting Artificial Star for High-resolution Coronal Imaging from the Ground (ORCAS-Helio), and presents the Preliminary Science Traceability Matrix (STM), defining the scientific objectives, the expected significance, and the impact of the mission. Furthermore, the paper describes the payload, mission configuration, and spacecraft architecture and shows it could meet its scientific and engineering requirements. By doing so, a viable mission configuration for the ORCAS-Helio mission is established.
Document ID
20220012071
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Eliad Peretz
(Goddard Space Flight Center Greenbelt, Maryland, United States)
John C Mather
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Doug Rabin
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Thomas Rimmele
(National Science Foundation Arlington, Virginia, United States)
Jeff Kuhn
(University of Hawaii at Manoa Honolulu, Hawaii, United States)
Dirk Schmidt
(National Solar Observatory Boulder, Colorado, United States)
Andrew Lewis
(GSFC Intern)
Kayla Carmical
(GSFC Intern)
Luis Leon
(GSFC Intern)
Date Acquired
August 5, 2022
Publication Date
July 18, 2022
Publication Information
Publication: SPIE Astronomical Telescopes and Instrumentation
Publisher: SPIE
Subject Category
Solar Physics
Meeting Information
Meeting: SPIE Astronomical Telescopes + Instrumentation 2022
Location: Montreal
Country: CA
Start Date: July 17, 2022
End Date: July 22, 2022
Sponsors: SPIE
Funding Number(s)
WBS: 432938.09.01.04.40.10
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
External Peer Committee
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