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| attachment:itmx1.jpg attachment:itmx2.jpg attachment:itmx3.jpg | [[MugIce|{{attachment:itmx1.jpg||height=700}}]] [[MugIce|{{attachment:itmx2.jpg||height=700}}]] [[MugIce|{{attachment:itmx3.jpg||height=700}}]] |
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| http://www.ligo.caltech.edu/LIGO_web/icons/ligo_logo.gif [[BR]] | {{http://www.ligo.caltech.edu/LIGO_web/icons/ligo_logo.gif}} <<BR>> |
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| * TMC [[http://www.techmfg.com/Products/Advanced/STACIS2000.htm|STACIS 2000]] web site and [[http://www.techmfg.com/TechBkgd.pdf|Technical Background (pdf)]][[BR]]http://www.ligo.caltech.edu/~ajw/stacis2000.jpg http://www.ligo.caltech.edu/~ajw/stacis_block.gif | * TMC [[[http://www.techmfg.com/Products/Advanced/STACIS2000.htm|STACIS|2000]]] web site and [[[http://www.techmfg.com/TechBkgd.pdf|Technical|Background (pdf)]]]<<BR>>{{http://www.ligo.caltech.edu/~ajw/stacis2000.jpg}} {{http://www.ligo.caltech.edu/~ajw/stacis_block.gif}} |
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| * Between 11/27-12/6/00, Stave Vass and Larry Jones mounted the STACIS seismic isolation systems on the four 40m test mass chambers.[[BR]]http://www.ligo.caltech.edu/~ajw/stacisinst1.jpg http://www.ligo.caltech.edu/~ajw/stacisinst2.jpg | * Between 11/27-12/6/00, Stave Vass and Larry Jones mounted the STACIS seismic isolation systems on the four 40m test mass chambers.<<BR>>{{http://www.ligo.caltech.edu/~ajw/stacisinst1.jpg}} {{http://www.ligo.caltech.edu/~ajw/stacisinst2.jpg}} |
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| * Preliminary results, in [[http://www.ligo.caltech.edu/~ajw/stacis.ps|Postscript]] and [[http://www.ligo.caltech.edu/~ajw/stacis.pdf|pdf]]. * We are limited by our ability to measure motion below a few Hz and above some 10's of Hz, by our geophones. More about geophones: [[http://www.treefort.org/~ghost/geo.shtml| GEOPHONE FAQ[[|, [[http://micromachine.stanford.edu/smssl/projects/Geophones/|Geophone research at Stanford]], [[http://www.i-o.com/htmlweb/framesetland.htm|Geophones from i-o.com]]. |
* Preliminary results, in [[[http://www.ligo.caltech.edu/~ajw/stacis.ps|Postscript]]] and [[[http://www.ligo.caltech.edu/~ajw/stacis.pdf|pdf]]]. * We are limited by our ability to measure motion below a few Hz and above some 10's of Hz, by our geophones. More about geophones: [[[http://www.treefort.org/~ghost/geo.shtml||GEOPHONE FAQ[[|, [[http://micromachine.stanford.edu/smssl/projects/Geophones/|Geophone research at Stanford]]], [[[http://www.i-o.com/htmlweb/framesetland.htm|Geophones|from i-o.com]]]. |
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| URL: http://www.ligo.caltech.edu/~ajw/40m_stacis.html [[BR]] Questions? Contact [[mailto:ajw@ligo.caltech.edu|Alan Weinstein]]. ]]]] | URL: http://www.ligo.caltech.edu/~ajw/40m_stacis.html <<BR>> Questions? Contact [[[mailto:ajw@ligo.caltech.edu|Alan|Weinstein]]]. ]]]] |
Old Web PAge Below
Laser Interferometer Gravitational-Wave Observatory
STACIS seismic isolation at LIGO's 40 meter prototype Laboratory
Between 11/27-12/6/00, Stave Vass and Larry Jones mounted the STACIS seismic isolation systems on the four 40m test mass chambers.
Preliminary results, in Postscript] and pdf].
We are limited by our ability to measure motion below a few Hz and above some 10's of Hz, by our geophones. More about geophones: [[[http://www.treefort.org/~ghost/geo.shtml||GEOPHONE FAQ[[|, Geophone research at Stanford], Geophones].
URL: http://www.ligo.caltech.edu/~ajw/40m_stacis.html
Questions? Contact Alan]. ]]]]