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Vibration Isolation Design for the Micro-X Rocket PayloadMicro-X is a NASA-funded, sounding rocket-borne X-ray imaging spectrometer that will allow high precision measurements of velocity structure, ionization state and elemental composition of extended astrophysical systems. One of the biggest challenges in payload design is to maintain the temperature of the detectors during launch. There are several vibration damping stages to prevent energy transmission from the rocket skin to the detector stage, which causes heating during launch. Each stage should be more rigid than the outer stages to achieve vibrational isolation. We describe a major design effort to tune the resonance frequencies of these vibration isolation stages to reduce heating problems prior to the projected launch in the summer of 2014.
Document ID
20140017810
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Heine, S. N. T.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Figueroa-Feliciano, E.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Rutherford, J. M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Wikus, P.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Oakley, P.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Porter, Frederick S.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
McCammon, D.
(Wisconsin Univ. Madison, WI, United States)
Date Acquired
December 30, 2014
Publication Date
January 1, 2014
Publication Information
Publisher: Journal of Low Temperture Physics
Subject Category
Astrophysics
Report/Patent Number
GSFC-E-DAA-TN16047
Report Number: GSFC-E-DAA-TN16047
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
Transition-edge sensors
Vibration isolation
X-ray spectrometers
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