Scattered light noise at LIGO Livingston Observatory during O4
Debasmita Nandi, Anamaria Effler, Siddharth Soni, Tabata Aira Ferreira, Robert Schofield, Huyen Pham, Timothy O'Hanlon, V. V. Frolov, Gabriela Gonz\'alez

TL;DR
This paper investigates scattered light noise in LIGO Livingston during O4, identifying two glitch populations linked to ground motion and demonstrating mitigation through baffles and seismic isolation.
Contribution
It models coupling mechanisms of scattered light glitches and shows effective noise reduction strategies implemented during O4.
Findings
High-SNR glitches correlated with microseismic ground motion along X direction.
Installation of baffles reduced high-SNR glitch rate and SNR.
Seismic isolation platform eliminated low-SNR glitches caused by vertical ground motion.
Abstract
Scattered light is one of the most common sources of noise in the LIGO gravitational wave detectors. Light scattering is a highly non-linear process through which motion at low frequencies gets up-converted and creates noise in a higher frequency band in the detector data. From the beginning of the fourth observation run, many glitches appeared in the data of LIGO Livingston detector in the frequency range 10-40 Hz, and the morphology of these glitches suggested that they were produced by scattered light. From our analysis, we identified two different populations of scattered light glitches, one group having higher SNR than the other. The glitches of the high- SNR group were solely modulated by microseismic ground motion (ground motion in 0.1-1.0 Hz) and in this paper, we present models of possible coupling mechanisms for these glitches. We also present results of a statistical…
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