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  • SOLAR PHYSICS  (1)
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    Publication Date: 2019-06-28
    Description: Scientific objectives and requirements are discussed for solar X-ray observations, coronagraph observations, studies of coronal particle acceleration, and cosmic X-ray observations. Improved sensitivity and resolution can be provided for these studies using the pinhole/occulter facility which consists of a self-deployed boom of 50 m length separating an occulter plane from a detector plane. The X-ray detectors and coronagraphic optics mounted on the detector plane are analogous to the focal plane instrumentation of an ordinary telescope except that they use the occulter only for providing a shadow pattern. The occulter plane is passive and has no electrical interface with the rest of the facility.
    Keywords: SOLAR PHYSICS
    Type: NASA-TP-2168 , NAS 1.60:2168
    Format: application/pdf
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