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The Apollo Telescope Mount on SkylabThe Apollo Telescope Mount (ATM) containing eight telescopes that cover wavelengths ranging from 2 to 6563 A is described. These are a white light coronograph, an XUV coronal spectroheliograph, and XUV spectrograph, an X-ray spectrographic telescope, a UV scanning polychromator/spectroheliometer, an X-ray telescope, and two H-alpha telescopes. The purpose, performance, and characteristic features of each of these instruments are discussed. The extremely high quality of the transmitted data is noted, and solar photographs are presented.
Document ID
19740030145
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ise, R.
Cagle, E. H.
(NASA Marshall Space Flight Center Huntsville, Ala., United States)
Date Acquired
August 7, 2013
Publication Date
October 1, 1973
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: International Astronautical Congress
Location: Baku
Country: Azerbaidzhan SSR
Start Date: October 7, 1973
End Date: October 13, 1973
Sponsors: International Astronautical Federation
Accession Number
74A12895
Distribution Limits
Public
Copyright
Other

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