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one of the most challenging aspects of the development of future generations of ligo detectors is the fabrication of ultra-precise laser mirrors, optimized for the extreme stability required to withstand seismic and thermal loading for months at a time. a key result of the initial phase of this effort was the successful construction and operability of a vacuum cryostat that enabled the first generation of test-bed seismometers, detectors that were designed to measure minute shifts in the overall length of one of the test masses, which enabled the characterization of seismic noise down to levels of a few to tens of nano-meters.


the intent of this paper is to provide a background for the simulation of the mechanics of the jwst mechanism and the theoretical source of orbital error, as well as some background on how the jwst mechanisms are constructed from the ground up in an effort to understand how to better plan future jwst projects.


prevention of primary contamination of other tapes is important in today’s world of ever-increasing complexity and operational demands on field data systems. unfortunately, it is also extremely difficult, and costly, to ensure that there is zero risk of contamination. the most important technique to address this risk is to use an accepted and tested product, such as the fbs-101. however, for some special uses where extreme contamination is not a concern, we can think of some applications where it is better to use a product that can be easily cleaned. 84d34552a1