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 |