Show simple item record

dc.contributor.authorCarroll, Benjamin
dc.date.accessioned2017-06-02T18:42:27Z
dc.date.available2017-06-02T18:42:27Z
dc.date.issued2017-04
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/12905
dc.description.abstractThe Extreme Ultra-Violet Snapshot Imaging Spectrograph (ESIS) is a solar camera scheduled to launch on board a sounding rocket in August 2018. ESIS images the sun over a large field of view in multiple spectral orders, allowing it to simultaneously collect spatial and spectral data. Since images are collected in specific wavelengths, any direct illumination of the CCD cameras from the sun would defeat the purpose of the experiment. Optical baffles are used to eliminate the potential for this to occur, as well as limit potential stray light reflecting onto the CCDs. Due to compact system design, variations in optical geometry, and numerous optical path crossings, designing an effective baffle system for ESIS presented several unique challenges. Using Z-Max ray-tracing and CREO Parametric modeling software we created an effective design using six flat baffles along the experiment’s length.en_US
dc.language.isoen_USen_US
dc.publisherMontana State Universityen_US
dc.titleEUV Snapshot Imaging Spectrograph (ESIS) Baffle Designen_US
dc.typePresentationen_US
mus.citation.conferenceStudent Research Celebrationen_US
mus.citation.extentfirstpage1en_US
mus.citation.extentlastpage1en_US
mus.relation.collegeCollege of Engineeringen_US
mus.relation.departmentMechanical & Industrial Engineering.en_US
mus.relation.universityMontana State University - Bozemanen_US
mus.data.thumbpage1en_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record