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How X-rays Pass Through the Mirrors
(Curtis-mirror-beam.mov and curtis_web.mov)

Movie
Hi-res Movie
(235 MB)
Movie
Low-res Movie
(377 KB)
Run Time: 26 sec

VIDEOAUDIO
The animation shows light rays passing through two sets of the reflectors (seen in cross-section). The rays focus onto the detector. The cross-section of the precollimator appears, with light rays that are outside of the main beam not passing through the pre-collimator. This animation ends with an overlay of the Astro-E2 satellite over the mirror and detector.

CURTIS: The X-ray beam hits the primary reflector, then hits the secondary reflector and then moves on to the detector about four and a half meters away. We add a pre-collimator, before the primary reflection, to block off-axis X-rays.


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The Suzaku Learning Center is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC), within the Astrophysics Scicence Division (ASD) at NASA's Goddard Space Flight Center.

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Curator: Meredith Gibb
Responsible NASA Official: Phil Newman

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