Fabricating Sub-Collimating Grids for an X-Ray Solar Imaging Spectrometer Using LIGA Techniques

Brennen, R.A.; Hecht, M.H.; Wiberg, D.V.; Bonivert, W.D.; Hruby, J.M.; Scholz, M.L.; Stowe, T.D.; Kenny, T.W.; Jackson, K.H.; Malek, C.K.

dc.contributor.author	Brennen, R.A.	en_US
dc.contributor.author	Hecht, M.H.	en_US
dc.contributor.author	Wiberg, D.V.	en_US
dc.contributor.author	Bonivert, W.D.	en_US
dc.contributor.author	Hruby, J.M.	en_US
dc.contributor.author	Scholz, M.L.	en_US
dc.contributor.author	Stowe, T.D.	en_US
dc.contributor.author	Kenny, T.W.	en_US
dc.contributor.author	Jackson, K.H.	en_US
dc.contributor.author	Malek, C.K.	en_US
dc.date.accessioned	2004-10-03T03:40:53Z
dc.date.available	2004-10-03T03:40:53Z
dc.date.issued	1995-06	en_US
dc.identifier.citation	Stockholm, Sweden	en_US
dc.identifier.clearanceno	95-0756	en_US
dc.identifier.uri	http://hdl.handle.net/2014/30889
dc.description.abstract	A proposed NASA mission uses a High Energy Solar Spectroscopic Imager (HESSI) to image solar X-rays. The HESSI instrument consists of twelve rotating pairs of high aspect ratio, high Z grids, each pair of which is separated by 1.7 meters and backed by a single Ge detector. Discussed are the fabrication of these proof-of-concept sub-collimating X-ray grids which are to be used in HESSI.	en_US
dc.format.extent	81647 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	solar spectroscopic imager HESSI sub-collimating grid fabrication	en_US
dc.title	Fabricating Sub-Collimating Grids for an X-Ray Solar Imaging Spectrometer Using LIGA Techniques	en_US