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Apollo Telescope Mount experiments technologyThe Skylab Apollo Telescope Mount (ATM) experiments, consisting of a white light coronagraph, four ultraviolet instruments, two X-ray telescopes and two hydrogen-alpha telescopes, observed the sun daily for nine solar rotations. The ATM instruments were individually larger, more complex, and provided better spatial resolution than previous solar satellite instruments. An additional major advantage of the telescope complex was its ability to simultaneously collect multispectral data of specific solar phenomena. To maximize the scientific benefits of the orbiting observatory, a coordinated observing program involving worldwide ground-based observatories was conducted. A description of the Skylab, the ATM, and the ATM experiments is given, and the daily process of flight planning and execution is described.
Document ID
19750029517
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Keathley, W. C.
(NASA Marshall Space Flight Center Huntsville, Ala., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Astronautics (General)
Meeting Information
Meeting: Technology today for tomorrow; Eleventh Space Congress
Location: Cocoa Beach, FL
Start Date: April 17, 1974
End Date: April 19, 1974
Accession Number
75A13589
Distribution Limits
Public
Copyright
Other

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