Astrophysics > Instrumentation and Methods for Astrophysics
[Submitted on 8 May 2024 (v1), last revised 4 Sep 2024 (this version, v3)]
Title:In-depth analysis of LISA Pathfinder performance results: Time evolution, noise projection, physical models, and implications for LISA
View PDF HTML (experimental)Abstract:We present an in-depth analysis of the LISA Pathfinder differential acceleration performance over the entire course of its science operations, spanning approximately 500 days. We find that: 1) the evolution of the Brownian noise that dominates the acceleration amplitude spectral density (ASD), for frequencies $f\gtrsim 1\,\text{mHz}$, is consistent with the decaying pressure due to the outgassing of a single gaseous species. 2) between $f=36\,\mu\text{Hz}$ and $1\,\text{mHz}$, the acceleration ASD shows a $1/f$ tail in excess of the Brownian noise of almost constant amplitude, with $\simeq 20\%$ fluctuations over a period of a few days, with no particular time pattern over the course of the mission; 3) at the lowest considered frequency of $f=18\,\mu\text{Hz}$, the ASD significantly deviates from the $1/f$ behavior, because of temperature fluctuations that appear to modulate a quasi-static pressure gradient, sustained by the asymmetries of the outgassing pattern. We also present the results of a projection of the observed acceleration noise on the potential sources for which we had either a direct correlation measurement, or a quantitative estimate from dedicated experiments. These sources account for approximately $40\%$ of the noise power in the $1/f$ tail. Finally, we analyze the possible sources of the remaining unexplained fraction, and identify the possible measures that may be taken to keep those under control in LISA.
Submission history
From: Lorenzo Sala [view email][v1] Wed, 8 May 2024 16:47:04 UTC (5,164 KB)
[v2] Wed, 3 Jul 2024 08:17:42 UTC (5,165 KB)
[v3] Wed, 4 Sep 2024 08:33:55 UTC (5,165 KB)
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