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https://iiif.si.eduView ManifestView in Mirador ViewerUsage Conditions May ApplyUsage Conditions ApplyThere are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page.
IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections.
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https://iiif.si.eduView ManifestView in Mirador ViewerUsage Conditions May ApplyUsage Conditions ApplyThere are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page.
IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections.
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https://iiif.si.eduView ManifestView in Mirador ViewerUsage Conditions May ApplyUsage Conditions ApplyThere are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page.
IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections.
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https://iiif.si.eduView ManifestView in Mirador ViewerUsage Conditions May ApplyUsage Conditions ApplyThere are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page.
IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections.
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IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections.
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https://iiif.si.eduView ManifestView in Mirador ViewerUsage Conditions May ApplyUsage Conditions ApplyThere are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page.
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This amplifier is a key electronic component (unflown but flight ready, with a non-flight plug) in the WMAP (Wilkinson Microwave Anisotropy Probe) satellite allowing for low noise amplification of the front end detectors of the Probe without need for sustained active deep cryogenic working environment. It would work to specification when cooled to -90K utilizing passive thermal radiators, which greatly extended the potential lifetime of the mission. Some 80 amplifiers of this basic design were employed on the Probe. These devices were designed, fabricated and rated for flight at the National Radio Astronomy Observatory's Central Development Laboratory in Charlottesville, VA. This microwave technology has also been applied to the NRAO ALMA array.
Display Status
This object is not on display at the National Air and Space Museum. It is either on loan or in storage.
Object Details
Country of Origin
United States of America
Type
MODELS-Uncrewed Spacecraft & Parts
Manufacturer
NASA, Goddard Space Flight Center Dimensions
3-D: 5.1 × 4 × 1.6cm, 0.5kg (2 × 1 9/16 × 5/8 in., 1lb.) Materials
Mixed metals and solid state electronics Inventory Number
A20060634002
Credit Line
Transferred from the NASA Goddard Space Flight Center.
Data Source
National Air and Space Museum
Restrictions & Rights
Usage conditions apply
For more information, visit the Smithsonians Terms of Use.