LISA Pathfinder: mission and status

Finally, as the only detector in JUNO that is sensitive to certain fast neutron events produced by the rock muons or the corner clipping muons, we have estimated that the TT can

The main challenges when developing an optical simulator for LISA are : - simulate the propagation delays (16 s!) from one satellite to another - keep the phase noise of the

The measurement of this phase shift changes mainly relies on very good performance of the three stabilization stages: algorithms accuracy (TDI), precise feedback loops (arm-locking)

In the following is shown a procedure adopted to find possible scattered light sources and paths on an arbitrarily complex optical system (e.g. the ZIFO), and to calculate

An automated test bench has been developed for the ATLAS shapers and the analog memory integrated circuits. The measurement setup is based on a Labview application and the

MICROSCOPE is a French Space Agency mission that aims to test the Weak Equivalence Principle in space down to an accuracy of 10 − 15.. This is two orders of magnitude better than

a low frequency sinuso dal signal on the high voltage lines and to read the.. response from the signal layer by

With the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA), designed to characterize the coma of comet 67P/Churyumov-Gerasimenko, we were able to quantify the