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dc.contributor.authorHeine, Sarah Nicole Trowbridge
dc.contributor.authorFigueroa-Feliciano, Enectali
dc.contributor.authorRutherford, J. M.
dc.contributor.authorWikus, P.
dc.contributor.authorOakley, P. H. H.
dc.contributor.authorPorter, F. S.
dc.contributor.authorMcCammon, D.
dc.date.accessioned2014-07-25T16:56:49Z
dc.date.available2014-07-25T16:56:49Z
dc.date.issued2013-12
dc.date.submitted2013-07
dc.identifier.issn0022-2291
dc.identifier.issn1573-7357
dc.identifier.urihttp://hdl.handle.net/1721.1/88500
dc.description.abstractMicro-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.en_US
dc.language.isoen_US
dc.publisherSpringer Science+Business Mediaen_US
dc.relation.isversionofhttp://dx.doi.org/10.1007/s10909-013-1032-1en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleVibration Isolation Design for the Micro-X Rocket Payloaden_US
dc.typeArticleen_US
dc.identifier.citationHeine, S. N. T., E. Figueroa-Feliciano, J. M. Rutherford, P. Wikus, P. Oakley, F. S. Porter, and D. McCammon. “Vibration Isolation Design for the Micro-X Rocket Payload.” J Low Temp Phys (December 31, 2013).en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorHeine, Sarah Nicole Trowbridgeen_US
dc.contributor.mitauthorFigueroa-Feliciano, Enectalien_US
dc.contributor.mitauthorRutherford, J. M.en_US
dc.contributor.mitauthorWikus, P.en_US
dc.contributor.mitauthorOakley, P. H. H.en_US
dc.contributor.mitauthorPorter, F. S.en_US
dc.contributor.mitauthorMcCammon, D.en_US
dc.relation.journalJournal of Low Temperature Physicsen_US
dc.eprint.versionOriginal manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dspace.orderedauthorsHeine, S. N. T.; Figueroa-Feliciano, E.; Rutherford, J. M.; Wikus, P.; Oakley, P.; Porter, F. S.; McCammon, D.en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-4081-6322
dc.identifier.orcidhttps://orcid.org/0000-0001-9285-5556
dspace.mitauthor.errortrue
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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