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dc.contributor.authorPlummer, James E.
dc.contributor.authorDeForest, Craig
dc.contributor.authorMartinez-Galarce, Dennis S.
dc.contributor.authorKankelborg, Charles
dc.contributor.authorGore, David B.
dc.contributor.authorO'Neal, Ray H.
dc.contributor.authorWalker, Arthur B.C. II
dc.contributor.authorPowell, Forbes R.
dc.contributor.authorHoover, Richard B.
dc.contributor.authorBarbee, Troy W. Jr.
dc.contributor.authorWeed, J.W.
dc.date.accessioned2016-03-31T15:25:36Z
dc.date.available2016-03-31T15:25:36Z
dc.date.issued1995-06-20
dc.identifier.citationPlummer, James E., Craig E. DeForest, Dennis S. Martinez-Galarce, Charles C. Kankelborg, David B. Gore, et al. "Design and performance of thin foil XUV filters for the Multi-Spectral Solar Telescope Array II", Proceedings of the SPIE 2515, X-Ray and Extreme Ultraviolet Optics, 565 (June 20, 1995); doi:10.1117/12.212623en_US
dc.identifier.issn0277-786X
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/9663
dc.description.abstractThe redesigned payload of the Multi-Spectral Solar Telescope Array (MSSTA), the MSSTA II, was successfully flown on November 3, 1994. The multilayer mirrors used in the normal incidence optical systems of the MSSTA II are efficient reflectors for soft x-ray/extreme ultraviolet (EUV) radiation at wavelengths that satisfy the Bragg condition, thus allowing a narrow band of the soft x-ray/EUV spectrum to be isolated. When applied to solar observations the temperature response of an optical system is quite sensitive to telescope bandpass because of the high density of lines in the coronal spectrum. We have designed a set of thin foil filters in conjunction with our multilayer optics to eliminate contaminant lines and specular reflectivity, thus enhancing the temperature diagnostic capabilities of our instruments. Extensive measurements have recently been carried out on the thin foil filters at the Stanford Synchrotron Radiation Laboratory. We describe here the design and performance of thin foil filters developed for the MSSTA II.en_US
dc.description.sponsorshipThe MSSTA project at Stanford University is supported by NASA Grant NSG-5131. Richard B. Hoover is supported in part by a grant from the MSFC Center Director's Discretionary Fund and by NASA Grant NSG-5131. Troy W. Barbee, Jr., is supported by the U.S. Department of Energy through Lawrence Livermore National Laboratory under contract W-7405-Eng-48.en_US
dc.titleDesign and performance of thin foil XUV filters for the Multi‐Spectral Solar Telescope Array IIen_US
dc.typeArticleen_US
mus.citation.conferenceX-Ray and Extreme Ultraviolet Optics; Richard B. Hoover, Arthur B. C. Walker, Jr.; San Diego, CA, United States; July 09, 1995en_US
mus.citation.extentfirstpage565en_US
mus.citation.extentlastpage575en_US
mus.citation.journaltitleProceedings of the SPIE 2515, X-Ray and Extreme Ultraviolet Opticsen_US
mus.citation.volume2515en_US
mus.identifier.categoryPhysics & Mathematicsen_US
mus.identifier.doi10.1117/12.212623en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US
mus.data.thumbpage6en_US


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