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1. Tilt-to-length coupling in LISA Pathfinder: long-term stability

Author

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, A M, Danzmann, K, Silva, M de Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, E D, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Hartig, M-S, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Johann, U, Johlander, B, Karnesis, N, Kaune, B, Killow, C J, Korsakova, N, Lobo, J A, López-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Martín, V, Martin-Polo, L, Martin-Porqueras, F, Martino, J, McNamara, P W, Mendes, J, Mendes, L, Meshksar, N, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Plagnol, E, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, D I, Russano, G, Sanjuan, J, Slutsky, J, Sopuerta, C F, Sumner, T, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P J, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The tilt-to-length coupling during the LISA Pathfinder mission has been numerically and analytically modeled for particular timespans. In this work, we investigate the long-term stability of the coupling coefficients of this noise. We show that they drifted slowly (by 1\,$\mu$m/rad and 6$\times10^{-6}$ in 100 days) and strongly correlated to temperature changes within the satellite (8\,$\mu$m/rad/K and 30$\times10^{-6}$/K). Based on analytical TTL coupling models, we attribute the temperature-driven coupling changes to rotations of the test masses and small distortions in the optical setup. Particularly, we show that LISA Pathfinder's optical baseplate was bent during the cooldown experiment, which started in late 2016 and lasted several months.

Published
2024
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2. Precision measurements of the magnetic parameters of LISA Pathfinder test masses

Author

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, A M, Danzmann, K, Silva, M De Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, E D, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Hartig, M S, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Karnesis, N, Kaune, B, Korsakova, N, Killow, C J, Liu, L, Lobo, J A, López-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Martín, V, Martino, J, Martin-Polo, L, Martin-Porqueras, F, McNamara, P W, Mendes, J, Mendes, L, Meshksar, N, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Pivato, P, Plagnol, E, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, D I, Russano, G, Sala, L, Serrano, D, Slutsky, J, Sopuerta, C F, Sumner, T, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology
Abstract

A precise characterization of the magnetic properties of LISA Pathfinder free falling test-masses is of special interest for future gravitational wave observatory in space. Magnetic forces have an important impact on the instrument sensitivity in the low frequency regime below the millihertz. In this paper we report on the magnetic injection experiments performed throughout LISA Pathfinder operations. We show how these experiments allowed a high precision estimate of the instrument magnetic parameters. The remanent magnetic moment was found to have a modulus of $(0.245\pm0.081)\,\rm{nAm}^2$, the x-component of the background magnetic field within the test masses position was measured to be $(414 \pm 74)$ nT and its gradient had a value of $(-7.4\pm 2.1)\,\mu$T/m. Finally, we also measured the test mass magnetic susceptibility to be $(-3.35\pm0.15)\times$10$^{-5}$ in the low frequency regime. All results are in agreement with on-ground estimates.

Published
2024

3. Magnetic-induced force noise in LISA Pathfinder free-falling test masses

Author

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, A M, Danzmann, K, Silva, M De Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, E D, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Hartig, M S, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Karnesis, N, Kaune, B, Korsakova, N, Killow, C J, Liu, L, Lobo, J A, López-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Martín, V, Martino, J, Martin-Polo, L, Martin-Porqueras, F, McNamara, P W, Mendes, J, Mendes, L, Meshksar, N, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Pivato, P, Plagnol, E, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, D I, Russano, G, Sala, L, Serrano, D, Slutsky, J, Sopuerta, C F, Sumner, T, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology
Abstract

LISA Pathfinder was a mission designed to test key technologies required for gravitational wave detection in space. Magnetically driven forces play a key role in the instrument sensitivity in the low-frequency regime, which corresponds to the measurement band of interest for future space-borne gravitational wave observatories. Magnetic-induced forces couple to the test mass motion, introducing a contribution to the relative acceleration noise between the free falling test masses. In this Letter we present the first complete estimate of this term of the instrument performance model. Our results set the magnetic-induced acceleration noise during the February 2017 noise run of $\rm 0.25_{-0.08}^{+0.15}\,fm\,s^{-2}/\sqrt{Hz}$ at 1 mHz and $\rm 1.01_{-0.24}^{+0.73}\, fm\,s^{-2}/\sqrt{Hz}$ at 0.1 mHz. We also discuss how the non-stationarities of the interplanetary magnetic field can affect these values during extreme space weather conditions.

Published
2024

4. In-depth analysis of LISA Pathfinder performance results: Time evolution, noise projection, physical models, and implications for LISA

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Chiavegato, V., Cruise, A. M., Bosco, D. Dal, Danzmann, K., Silva, M. De Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M. S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Johlander, B., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Lobo, J. A., Lopez-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martın, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D. I., Russano, G., Sala, L., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W. J., Wissel, L., Wittchen, A., Zanoni, C., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
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.

Published
2024
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5. NanoNewton electrostatic force actuators for femtoNewton-sensitive measurements: system performance test in the LISA Pathfinder mission

Author

Armano, M, Audley, H, Baird, J, Bassan, M, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Chiavegato, V, Cruise, A M, Bosco, D Dal, Danzmann, K, Silva, M De Deus, De Rosa, R, Di Fiore, L, Diepholz, I, Dixon, G, Dolesi, R, Ferroni, L Ferraioli V, Fitzsimons, E D, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grado, A, Grimani, C, Grzymisch, J, Harrison, I, Hartig, M S, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Johlander, B, Karnesis, N, Kaune, B, Korsakova, N, Killow, C J, Liu, L, Lobo, J A, López-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Martín, V, Martin-Polo, L, Martin-Porqueras, F, Martino, J, McNamara, P W, Mendes, J, Mendes, L, Meshksar, N, Moerschell, J, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Plagnol, E, Praplan, C, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, D I, Russano, G, Sala, L, Sarra, P, Schule-Walewski, S L, Slutsky, J, Sopuerta, C F, Stanga, R, Sumner, T, Pierick, J ten, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P, Weber, W J, Wissel, L, Wittchen, A, Zanoni, C, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology
Abstract

Electrostatic force actuation is a key component of the system of geodesic reference test masses (TM) for the LISA orbiting gravitational wave observatory and in particular for performance at low frequencies, below 1 mHz, where the observatory sensitivity is limited by stray force noise. The system needs to apply forces of order 10$^{-9}$ N while limiting fluctuations in the measurement band to levels approaching 10$^{-15}$ N/Hz$^{1/2}$. We present here the LISA actuation system design, based on audio-frequency voltage carrier signals, and results of its in-flight performance test with the LISA Pathfinder test mission. In LISA, TM force actuation is used to align the otherwise free-falling TM to the spacecraft-mounted optical metrology system, without any forcing along the critical gravitational wave-sensitive interferometry axes. In LISA Pathfinder, on the other hand, the actuation was used also to stabilize the TM along the critical $x$ axis joining the two TM, with the commanded actuation force entering directly into the mission's main differential acceleration science observable. The mission allowed demonstration of the full compatibility of the electrostatic actuation system with the LISA observatory requirements, including dedicated measurement campaigns to amplify, isolate, and quantify the two main force noise contributions from the actuation system, from actuator gain noise and from low frequency ``in band'' voltage fluctuations. These campaigns have shown actuation force noise to be a relevant, but not dominant, noise source in LISA Pathfinder and have allowed performance projections for the conditions expected in the LISA mission.

Published
2023

6. Tilt-to-length coupling in LISA Pathfinder: a data analysis

Author

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, A M, Danzmann, K, Silva, M de Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, E D, Freschi, M, Gesa, L, Giardini, D, Gibert, F, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Hartig, M-S, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspé, H, Jennrich, O, Jetzer, P, Johann, U, Johlander, B, Karnesis, N, Kaune, B, Killow, C J, Korsakova, N, Lobo, J A, López-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Martín, V, Martin-Polo, L, Martin-Porqueras, F, Martino, J, McNamara, P W, Mendes, J, Mendes, L, Meshksar, N, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Plagnol, E, Ramos-Castro, J, Reiche, J, Rivas, F, Robertson, D I, Russano, G, Sanjuan, J, Slutsky, J, Sopuerta, C F, Sumner, T, Tevlin, L, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P J, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present a study of the tilt-to-length coupling noise during the LISA Pathfinder mission and how it depended on the system's alignment. Tilt-to-length coupling noise is the unwanted coupling of angular and lateral spacecraft or test mass motion into the primary interferometric displacement readout. It was one of the major noise sources in the LISA Pathfinder mission and is likewise expected to be a primary noise source in LISA. We demonstrate here that a recently derived and published analytical model describes the dependency of the LISA Pathfinder tilt-to-length coupling noise on the alignment of the two freely falling test masses. This was verified with the data taken before and after the realignments performed in March (engineering days) and June 2016, and during a two-day experiment in February 2017 (long cross-talk experiment). The latter was performed with the explicit goal of testing the tilt-to-length coupling noise dependency on the test mass alignment. Using the analytical model, we show that all realignments performed during the mission were only partially successful and explain the reasons why. In addition to the analytical model, we computed another physical tilt-to-length coupling model via a minimising routine making use of the long cross-talk experiment data. A similar approach could prove useful for the LISA mission.

Published
2023
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7. Charging of free-falling test masses in orbit due to cosmic rays: results from LISA Pathfinder

Author

LISA Pathfinder Collaboration, Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cesarini, A. Cavalleri A., Cruise, A. M, Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M. -S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Killow, C. J., Korsakova, N., Lobo, J. A., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martino, J., Martin-Polo, L., Martin-Porqueras, F., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D. I., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T. J., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

A comprehensive summary of the measurements made to characterize test mass charging due to the space environment during the LISA Pathfinder mission is presented. Measurements of the residual charge of the test mass after release by the grabbing and positioning mechanism, show that the initial charge of the test masses was negative after all releases, leaving the test mass with a potential in the range $-12$ mV to $-512$ mV. Variations in the neutral test mass charging rate between $21.7$ e s$^{-1}$ and $30.7$ e s$^{-1}$ were observed over the course of the 17-month science operations produced by cosmic ray flux changes including a Forbush decrease associated with a small solar energetic particle event. A dependence of the cosmic ray charging rate on the test mass potential between $-30.2$ e s$^{-1}$ V$^{-1}$ and $-40.3$ e s$^{-1}$ V$^{-1}$ was observed and this is attributed to a contribution to charging from low-energy electrons emitted from the gold surfaces of the gravitational reference sensor. Data from the on-board particle detector show a reliable correlation with the charging rate and with other environmental monitors of the cosmic ray flux. This correlation is exploited to extrapolate test mass charging rates to a 20-year period giving useful insight into the expected range of charging rate that may be observed in the LISA mission., Comment: 17 pages, 10 figures

Published
2022
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8. Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Lobo, J. A., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D. I., Roma-Dollase, D., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T., Telloni, D., Texier, D., Thorpe, J. I., Trenkel, C., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Wealthy, D., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

LISA Pathfinder (LPF) has been a space-based mission designed to test new technologies that will be required for a gravitational wave observatory in space. Magnetically driven forces play a key role in the instrument sensitivity in the low-frequency regime (mHz and below), the measurement band of interest for a space-based observatory. The magnetic field can couple to the magnetic susceptibility and remanent magnetic moment from the test masses and disturb them from their geodesic movement. LISA Pathfinder carried on-board a dedicated magnetic measurement subsystem with noise levels of 10 $ \rm nT \ Hz^{-1/2}$ from 1 Hz down to 1 mHz. In this paper we report on the magnetic measurements throughout LISA Pathfinder operations. We characterise the magnetic environment within the spacecraft, study the time evolution of the magnetic field and its stability down to 20 $\mu$Hz, where we measure values around 200 $ \rm nT \ Hz^{-1/2}$ and identify two different frequency regimes, one related to the interplanetary magnetic field and the other to the magnetic field originating inside the spacecraft. Finally, we characterise the non-stationary component of the fluctuations of the magnetic field below the mHz and relate them to the dynamics of the solar wind., Comment: 16 pages, 17 figures. MNRAS LaTeX style file version 3.0

Published
2020
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9. LISA Pathfinder Performance Confirmed in an Open-Loop Configuration: Results from the Free-Fall Actuation Mode

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Lobo, J. A., Liu, L., Llopez-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Meshksar, N., Martìn, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Physics - Space Physics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We report on the results of the LISA Pathfinder (LPF) free-fall mode experiment, in which the control force needed to compensate the quasistatic differential force acting on two test masses is applied intermittently as a series of "impulse" forces lasting a few seconds and separated by roughly 350 s periods of true free fall. This represents an alternative to the normal LPF mode of operation in which this balancing force is applied continuously, with the advantage that the acceleration noise during free fall is measured in the absence of the actuation force, thus eliminating associated noise and force calibration errors. The differential acceleration noise measurement presented here with the free-fall mode agrees with noise measured with the continuous actuation scheme, representing an important and independent confirmation of the LPF result. An additional measurement with larger actuation forces also shows that the technique can be used to eliminate actuation noise when this is a dominant factor.

Published
2019
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10. Temperature stability in the sub-milliHertz band with LISA Pathfinder

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Lobo, J. A., Lloro, I., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Mansanet, C., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Sanjuán, J., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J. I., Trenkel, C., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Wealthy, D., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, General Relativity and Quantum Cosmology
Abstract

LISA Pathfinder (LPF) was a technology pioneering mission designed to test key technologies required for gravitational wave detection in space. In the low frequency regime (milli-Hertz and below), where space-based gravitational wave observatories will operate, temperature fluctuations play a crucial role since they can couple into the interferometric measurement and the test masses' free-fall accuracy in many ways. A dedicated temperature measurement subsystem, with noise levels in 10$\,\mu$K$\,$Hz$^{-1/2}$ down to $1\,$mHz was part of the diagnostics unit on board LPF. In this paper we report on the temperature measurements throughout mission operations, characterize the thermal environment, estimate transfer functions between different locations and report temperature stability (and its time evolution) at frequencies as low as 10$\,\mu$Hz, where typically values around $1\,$K$\,$Hz$^{-1/2}$ were measured., Comment: 13 pages, 16 figures. MNRAS LaTeX style file version 3.0

Published
2019
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11. Micrometeoroid Events in LISA Pathfinder

Author

Thorpe, James Ira, Slutsky, Jacob, Baker, John, Littenberg, Tyson, Hourihane, Sophie, Pagane, Nicole, Pokorny, Petr, Janches, Diego, Armano, Michele, Audley, Heather, Auger, G., Baird, Jonathan, Bassan, Massimo, Binetruy, Pierre, Born, Michael, Bortoluzzi, D., Brandt, N., Caleno, M., Cavalleri, A, Cesarini, A, Cruise, A. M., Danzmann, K., Silva, M. de Deus, De Rosa, R., Di Fiore, L., Diepholz, I., Dixon, G., Dolesi, R., Dunbar, N., Ferraioli, L., Ferroni, V., Fitzsimons, E., Flatscher, R., Freschi, M., Marirrodriga, C. Garcia, Gerndt, R., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grado, A., Grimani, C., Gryzmisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspe, H., Jennrich, O., Jetzer, P., Johlander, B., Karnesis, N., Kaune, B., Korsakova, N., Killow, C., Lobo, J. A., Lloro, I., Liu, L., Lopez-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martin, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Madden, S., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Prat, P., Ragnit, U., Ramos-Castro, J., Reiche, J., Robertson, D., Rozemeijer, H., Rivas, F., Russano, G., Sarra, P., Schleicher, A., Shaul, D., Soperta, C., Stanga, R., Sumner, T., Texier, D., Trobs, M., Vetrungno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Wealthy, D., Weber, W. J., Wissel, L., Wittchen, A., Zambotti, A., Zanoni, C., Ziegler, T., and Zweifel, P.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

The zodiacal dust complex, a population of dust and small particles that pervades the Solar System, provides important insight into the formation and dynamics of planets, comets, asteroids, and other bodies. Here we present a new set of data obtained using a novel technique: direct measurements of momentum transfer to a spacecraft from individual particle impacts. This technique is made possible by the extreme precision of the instruments flown on the LISA Pathfinder spacecraft, a technology demonstrator for a future space-based gravitational wave observatory that operated near the first Sun-Earth Lagrange point from early 2016 through Summer of 2017. Using a simple model of the impacts and knowledge of the control system, we show that it is possible to detect impacts and measure properties such as the transferred momentum (related to the particle's mass and velocity), direction of travel, and location of impact on the spacecraft. In this paper, we present the results of a systematic search for impacts during 4348 hours of Pathfinder data. We report a total of 54 candidates with momenta ranging from 0.2$\,\mu\textrm{Ns}$ to 230$\,\mu\textrm{Ns}$. We furthermore make a comparison of these candidates with models of micrometeoroid populations in the inner solar system including those resulting from Jupiter-family comets, Oort-cloud comets, Hailey-type comets, and Asteroids. We find that our measured population is consistent with a population dominated by Jupiter-family comets with some evidence for a smaller contribution from Hailey-type comets. This is in agreement with consensus models of the zodiacal dust complex in the momentum range sampled by LISA Pathfinder., Comment: 22 pages, 14 figures, accepted in ApJ

Published
2019
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12. Forbush decreases and $<$ 2-day GCR flux non-recurrent variations studied with LISA Pathfinder

Author

Grimani, C., Armano, M., Audley, H., Baird, J., Benella, S., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Fabi, M., Ferraioli, L., Ferroni, V., Finetti, N., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Kudela, K., Laurenza, M., Lobo, J. A., Lloro, I., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Meshksar, N., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T., Telloni, D., Texier, D., Thorpe, J. I., Vetrugno, D., Villani, M., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Physics - Space Physics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

Non-recurrent short term variations of the galactic cosmic-ray (GCR) flux above 70 MeV n$^{-1}$ were observed between 2016 February 18 and 2017 July 3 aboard the European Space Agency LISA Pathfinder (LPF) mission orbiting around the Lagrange point L1 at 1.5$\times$10$^6$ km from Earth. The energy dependence of three Forbush decreases (FDs) is studied and reported here. A comparison of these observations with others carried out in space down to the energy of a few tens of MeV n$^{-1}$ shows that the same GCR flux parameterization applies to events of different intensity during the main phase. FD observations in L1 with LPF and geomagnetic storm occurrence is also presented. Finally, the characteristics of GCR flux non-recurrent variations (peaks and depressions) of duration $<$ 2 days and their association with interplanetary structures are investigated. It is found that, most likely, plasma compression regions between subsequent corotating high-speed streams cause peaks, while heliospheric current sheet crossing cause the majority of the depressions.

Published
2019
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13. Experimental results from the ST7 mission on LISA Pathfinder

Author

Anderson, G, Anderson, J, Anderson, M, Aveni, G, Bame, D, Barela, P, Blackman, K, Carmain, A, Chen, L, Cherng, M, Clark, S, Connally, M, Connolly, W, Conroy, D, Cooper, M, Cutler, C, D'Agostino, J, Demmons, N, Dorantes, E, Dunn, C, Duran, M, Ehrbar, E, Evans, J, Fernandez, J, Franklin, G, Girard, M, Gorelik, J, Hruby, V, Hsu, O, Jackson, D, Javidnia, S, Kern, D, Knopp, M, Kolasinski, R, Kuo, C, Le, T, Li, I, Liepack, O, Littlefield, A, Maghami, P, Malik, S, Markley, L, Martin, R, Marrese-Reading, C, Mehta, J, Mennela, J, Miller, D, Nguyen, D, O'Donnell, J, Parikh, R, Plett, G, Ramsey, T, Randolph, T, Rhodes, S, Romero-Wolf, A, Roy, T, Ruiz, A, Shaw, H, Slutsky, J, Spence, D, Stocky, J, Tallon, J, Thorpe, I, Tolman, W, Umfress, H, Valencia, R, Valerio, C, Warner, W, Wellman, J, Willis, P, Ziemer, J, Zwahlen, J, Armano, M, Audley, H, Baird, J, Binetruy, P, Born, a M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, A M, Danzmann, K, Silva, M de Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Fitzsimons, E D, Freschi, M, Gesa, L, Gibert, F, Giardini, D, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspe, H, Jennrich, O, Jetzer, P, Karnesis, N, Kaune, B, Korsakova, N, Killow, C J, Lobo, J A, Lloro, I, Liu, L, Lopez-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Meshksar, N, Martin, V, Martin-Polo, L, Martino, J, Martin-Porqueras, F, Mateos, I, McNamara, P W, Mendes, J, Mendes, L, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Pivato, P, Plagnol, E, Ramos-Castro, J, Reiche, J, Robertson, D I, Rivas, F, Russano, G, Sopuerta, C F, Sumner, T, Texier, D, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P J, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Space Technology 7 Disturbance Reduction System (ST7-DRS) is a NASA technology demonstration payload that operated from January 2016 through July of 2017 on the European Space Agency's LISA Pathfinder spacecraft. The joint goal of the NASA and ESA missions was to validate key technologies for a future space-based gravitational wave observatory targeting the source-rich milliHertz band. The two primary components of ST7-DRS are a micropropulsion system based on colloidal micro-Newton thrusters (CMNTs) and a control system that simultaneously controls the attitude and position of the spacecraft and the two free-flying test masses (TMs). This paper presents our main experimental results and summarizes the overall the performance of the CMNTs and control laws. We find that the CMNT performance to be consistent with pre-flight predictions, with a measured system thrust noise on the order of $100\,\textrm{nN}/\sqrt{\textrm{Hz}}$ in the $1\,\textrm{mHz}\leq f \leq 30\,\textrm{mHz}$ band. The control system maintained the TM-spacecraft separation with an RMS error of less than 2$\,$nm and a noise spectral density of less than $3\,\textrm{nm}/\sqrt{\textrm{Hz}}$ in the same band. Thruster calibration measurements yield thrust values consistent with the performance model and ground-based thrust-stand measurements, to within a few percent. We also report a differential acceleration noise between the two test masses with a spectral density of roughly $3\,\textrm{fm}/\textrm{s}^2/\sqrt{\textrm{Hz}}$ in the $1\,\textrm{mHz}\leq f \leq 30\,\textrm{mHz}$ band, slightly less than twice as large as the best performance reported with the baseline LISA Pathfinder configuration and below the current requirements for the Laser Interferometer Space Antenna (LISA) mission.

Published
2018
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14. Precision Charge Control for Isolated Free-Falling Test Masses: LISA Pathfinder Results

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Liu, L., Lloro, I., Lobo, J. A., López-Zaragoza, J. P., Maarschalkerweerd, R., Mailland, F., Mance, D., Martín, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Meshskar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pfeil, M., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Santoruvo, G., Sarra, P., Shaul, D., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J. I., Trenkel, C., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Waschke, S., Wass, P. J., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Physics - Instrumentation and Detectors
Abstract

The LISA Pathfinder charge management device was responsible for neutralising the cosmic ray induced electric charge that inevitably accumulated on the free-falling test masses at the heart of the experiment. We present measurements made on ground and in-flight that quantify the performance of this contactless discharge system which was based on photo-emission under UV illumination. In addition, a two-part simulation is described that was developed alongside the hardware. Modelling of the absorbed UV light within the Pathfinder sensor was carried out with the GEANT4 software toolkit and a separate MATLAB charge transfer model calculated the net photocurrent between the test masses and surrounding housing in the presence of AC and DC electric fields. We confront the results of these models with observations and draw conclusions for the design of discharge systems for future experiments like LISA that will also employ free-falling test masses.

Published
2018
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15. Calibrating the system dynamics of LISA Pathfinder

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Lobo, J. A., Lloro, I., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Meshksar, N., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

LISA Pathfinder (LPF) was a European Space Agency mission with the aim to test key technologies for future space-borne gravitational-wave observatories like LISA. The main scientific goal of LPF was to demonstrate measurements of differential acceleration between free-falling test masses at the sub-femto-g level, and to understand the residual acceleration in terms of a physical model of stray forces, and displacement readout noise. A key step toward reaching the LPF goals was the correct calibration of the dynamics of LPF, which was a three-body system composed by two test-masses enclosed in a single spacecraft, and subject to control laws for system stability. In this work, we report on the calibration procedures adopted to calculate the residual differential stray force per unit mass acting on the two test-masses in their nominal positions. The physical parameters of the adopted dynamical model are presented, together with their role on LPF performance. The analysis and results of these experiments show that the dynamics of the system was accurately modeled and the dynamical parameters were stationary throughout the mission. Finally, the impact and importance of calibrating system dynamics for future space-based gravitational wave observatories is discussed.

Published
2018
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16. Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a Forbush decrease with LISA Pathfinder

Author

Armano, M., Audley, H., Baird, J., Bassan, M., Benella, S., Binetruy, P., Born, M., Bortoluzzi, D., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dixon, G., Dolesi, R., Fabi, M., Ferraioli, L., Ferroni, V., Finetti, N., Fitzsimons, E. D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C. J., Laurenza, M., Lobo, J. A., Lloro, I., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D. I., Rivas, F., Russano, G., Sabbatini, F., Slutsky, J., Sopuerta, C. F., Sumner, T., Telloni, D., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W. J., Wissel, L., Wittchen, A., Zambotti, A., Zanoni, C., and Zweifel, P.

Subjects
Physics - Space Physics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract

Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high counting rate particle detector (PD) aboard LISA Pathfinder (LPF), meant for subsystems diagnostics, was devoted to the measurement of galactic cosmic-ray and solar energetic particle integral fluxes above 70 MeV n$^{-1}$ up to 6500 counts s$^{-1}$. PD data were gathered with a sampling time of 15 s. Characteristics and energy-dependence of GCR flux recurrent depressions and of a Forbush decrease dated August 2, 2016 are reported here. The capability of interplanetary missions, carrying PDs for instrument performance purposes, in monitoring the passage of interplanetary coronal mass ejections (ICMEs) is also discussed.

Published
2018
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17. Measuring the Galactic Cosmic Ray Flux with the LISA Pathfinder Radiation Monitor

Author

Armano, M, Audley, H, Baird, J, Binetruy, P, Born, M, Bortoluzzi, D, Castelli, E, Cavalleri, A, Cesarini, A, Cruise, M, Danzmann, K, Silva, M de Deus, Diepholz, I, Dixon, G, Dolesi, R, Ferraioli, L, Ferroni, V, Finetti, N, Fitzsimons, E D, Freschi, M, Gesa, L, Gibert, F, Giardini, D, Giusteri, R, Grimani, C, Grzymisch, J, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Inchauspe, H, Jennrich, O, Jetzer, P, Karnesis, N, Kaune, B, Korsakova, N, Killow, C J, Lobo, J A, Lloro, I, Liu, L, Lopez-Zaragoza, J P, Maarschalkerweerd, R, Mance, D, Meshskar, N, Martin, V, Martin-Polo, L, Martino, J, Martin-Porqueras, F, Mateos, I, McNamara, P W, Mendes, J, Mendes, L, Nofrarias, M, Paczkowski, S, Perreur-Lloyd, M, Petiteau, A, Pivato, P, Plagnol, E, Ramos-Castro, J, Reiche, J, Robertson, D I, Rivas, F, Russano, G, Slutsky, J, Sopuerta, C F, Sumner, T, Texier, D, Thorpe, J I, Vetrugno, D, Vitale, S, Wanner, G, Ward, H, Wass, P, Weber, W J, Wissel, L, Wittchen, A, and Zweifel, P

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

Test mass charging caused by cosmic rays will be a significant source of acceleration noise for space-based gravitational wave detectors like LISA. Operating between December 2015 and July 2017, the technology demonstration mission LISA Pathfinder included a bespoke monitor to help characterise the relationship between test mass charging and the local radiation environment. The radiation monitor made in situ measurements of the cosmic ray flux while also providing information about its energy spectrum. We describe the monitor and present measurements which show a gradual 40% increase in count rate coinciding with the declining phase of the solar cycle. Modulations of up to 10% were also observed with periods of 13 and 26 days that are associated with co-rotating interaction regions and heliospheric current sheet crossings. These variations in the flux above the monitor detection threshold (approximately 70 MeV) are shown to be coherent with measurements made by the IREM monitor on-board the Earth orbiting INTEGRAL spacecraft. Finally we use the measured deposited energy spectra, in combination with a GEANT4 model, to estimate the galactic cosmic ray differential energy spectrum over the course of the mission.

Published
2017
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18. Charge-induced force-noise on free-falling test masses: results from LISA Pathfinder

Author

Armano, M., Audley, H., Auger, G., Baird, J. T., Binetruy, P., Born, M., Bortoluzzi, D., Brandt, N., Bursi, A., Caleno, M., Cavalleri, A., Cesarini, A., Cruise, M., Danzmann, K., Silva, M. de Deus, Diepholz, I., Dolesi, R., Dunbar, N., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Flatscher, R., Freschi, M., Gallegos, J., Marirrodriga, C. García, Gerndt, R., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hueller, M., Huesler, J., Inchauspé, H., Jennrich, O., Jetzer, P., Johlander, B., Karnesis, N., Kaune, B., Killow, C. J., Korsakova, N., Lloro, I., Liu, L., Maarschalkerweerd, R., Madden, S., Mance, D., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P. W., Mendes, J., Mendes, L., Moroni, A., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Prat, P., Ragnit, U., Ramos-Castro, J., Reiche, J., Perez, J. A. Romera, Robertson, D. I., Rozemeijer, H., Rivas, F., Russano, G., Sarra, P., Schleicher, A., Slutsky, J., Sopuerta, C., Sumner, T. J., Texier, D., Thorpe, J. I., Trenkel, C., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Wealthy, D., Weber, W. J., Wittchen, A., Zanoni, C., Ziegler, T., and Zweifel, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We report on electrostatic measurements made on board the European Space Agency mission LISA Pathfinder. Detailed measurements of the charge-induced electrostatic forces exerted on free-falling test masses (TMs) inside the capacitive gravitational reference sensor are the first made in a relevant environment for a space-based gravitational wave detector. Employing a combination of charge control and electric-field compensation, we show that the level of charge-induced acceleration noise on a single TM can be maintained at a level close to 1.0 fm/s^2/sqrt(Hz) across the 0.1-100 mHz frequency band that is crucial to an observatory such as LISA. Using dedicated measurements that detect these effects in the differential acceleration between the two test masses, we resolve the stochastic nature of the TM charge build up due to interplanetary cosmic rays and the TM charge-to-force coupling through stray electric fields in the sensor. All our measurements are in good agreement with predictions based on a relatively simple electrostatic model of the LISA Pathfinder instrument., Comment: 9 Pages, 3 figures

Published
2017
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19. In-flight testing of the injection of the LISA Pathfinder test mass into a geodesic

Author

Bortoluzzi, D., Vignotto, D., Zambotti, A., Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A.M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E.D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M.-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C.J., Lobo, J.A., Liu, L., López-Zaragoza, J.P., Maarschalkerweerd, R., Mance, D., Meshksar, N., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., McNamara, P.W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D.I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C.F., Sumner, T., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P.J., Weber, W.J., Wissel, L., Wittchen, A., Zweifel, P., and Zanoni, Carlo

Published
2021
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20. Land use following deforestation for Africa

Author

Masolele, R.N., Marcos, Diego, de Sy, Niki, Abu, Itohan-Osa, Verbesselt, J., Reiche, J., Herold, M., Masolele, R.N., Marcos, Diego, de Sy, Niki, Abu, Itohan-Osa, Verbesselt, J., Reiche, J., and Herold, M.

Abstract

These datasets were generated from the research article "Mapping the diversity of land uses following deforestation across Africa". Here we publish the yearly time series maps showing land use following deforestation across Africa at 30 m resolution covering the year 2001 to 2020 (20 years). The maps are derived from Planet-NICFI images using U-Net deep neural network architecture enhanced with attention. The original landuse maps are derived from 5 m resolution Planet-NICFI imagery (research license with Planet Labs Inc) of 2022. The Planet-NICFI imagery are accessible upon sign up at https://www.planet.com/nicfi/ or https://developers.planet.com/docs/integrations/gee/nicfi/ The landuse dataset has fifteen classes with values ranging from 1 -15, where 1: Larger-scale cropland, 2: Pasture, 3: Mining, 4: Small-scale cropland, 5: Roads, 6: Other land with tree cover, 7: Plantation forest, 8: Coffee, 9: Settlement, 10: Tea plantation, 11: Water, 12: Oil palm, 13: Rubber, 14: Cashew, 15: Cacao, Data Description These datasets were generated from the research article "Mapping the diversity of land uses following deforestation across Africa". Here we publish the yearly time series maps showing land use following deforestation across Africa at 30 m resolution covering the year 2001 to 2020 (20 years). The maps are derived from Planet-NICFI images using U-Net deep neural network architecture enhanced with attention. The original landuse maps are derived from 5 m resolution Planet-NICFI imagery (research license with Planet Labs Inc) of 2022. The Planet-NICFI imagery are accessible upon sign up at https://www.planet.com/nicfi/ or https://developers.planet.com/docs/integrations/gee/nicfi/ The landuse dataset has fifteen classes with values ranging from 1 -15, where 1: Larger-scale cropland, 2: Pasture, 3: Mining, 4: Small-scale cropland, 5: Roads, 6: Other land with tree cover, 7: Plantation forest, 8: Coffee, 9: Settlement, 10: Tea plantation, 11: Water, 12: Oil palm, 13: Rubber, 14: Cashew, 15: Cacao The data is accompanied by the sld and qml file (Visualisation_layer_descriptor_sld_and_qml) to aid in visualisation or legend creation. Data Visualisation at 5 m resolution: https://robertnag82.users.earthengine.app/view/africalu File Naming: LandUseFollowingDeforestation_dl_30m_20010101_20201231_af_epsg.4326_v1.tif Generic variable name: LandUseFollowingDeforestation Method of data production: dl (Deep learning) Spatial support in m: 30m Time reference begin time (YYYYMMDD): i.e. 20010101 Time reference end time: 20201230 Bounding box (2 letters max): af (Refering to Africa) EPSG code: epsg.4326 Version code: v1 JSON field representing the legend. This is important for the visualization of the legend. [ { "Large-scale cropland": "1", "color": "#FFFF00" }, { "Pasture": "2", "color": "#808080" }, { "Mining": "3", "color": "#FFC0CB" }, { "Small-scale cropland": "4", "color": "#F39C12" }, { "Roads": "5", "color": "#800000" }, { "Other land with tree cover/Regrowth "

Published
2024

21. Mapping the diversity of land uses following deforestation across Africa

Author

Masolele, R.N., Marcos, Diego, de Sy, Niki, Abu, Itohan-Osa, Verbesselt, J., Reiche, J., Herold, M., Masolele, R.N., Marcos, Diego, de Sy, Niki, Abu, Itohan-Osa, Verbesselt, J., Reiche, J., and Herold, M.

Abstract

African forest are increasingly in decline as a result of land-use conversion due to human activities. However, a consistent and detailed characterization and mapping of land-use change that results in forest loss is not available at the spatial-temporal resolution and thematic levels suitable for decision-making at the local and regional scales; so far they have only been provided on coarser scales and restricted to humid forests. Here we present the first high-resolution (5 m) and continental-scale mapping of land use following deforestation in Africa, which covers an estimated 13.85% of the global forest area, including humid and dry forests. We use reference data for 15 different land-use types from 30 countries and implement an active learning framework to train a deep learning model for predicting land-use following deforestation with an F1-score of for the whole of Africa. Our results show that the causes of forest loss vary by region. In general, small-scale cropland is the dominant driver of forest loss in Africa, with hotspots in Madagascar and DRC. In addition, commodity crops such as cacao, oil palm, and rubber are the dominant drivers of forest loss in the humid forests of western and central Africa, forming an “arc of commodity crops” in that region. At the same time, the hotspots for cashew are found to increasingly dominate in the dry forests of both western and south-eastern Africa, while larger hotspots for large-scale croplands were found in Nigeria and Zambia. The increased expansion of cacao, cashew, oil palm, rubber, and large-scale croplands observed in humid and dry forests of western and south-eastern Africa suggests they are vulnerable to future land-use changes by commodity crops, thus creating challenges for achieving the zero deforestation supply chains, support REDD+ initiatives, and towards sustainable development goals.

Published
2024

22. Critical Assessment of Cocoa Classification with Limited Reference Data: A Study in Côte d’Ivoire and Ghana Using Sentinel-2 and Random Forest Model

Author

Moraiti, N., Mullissa, A.G., Rahn, Eric, Sassen, M., Reiche, J., Moraiti, N., Mullissa, A.G., Rahn, Eric, Sassen, M., and Reiche, J.

Abstract

Cocoa is the economic backbone of Côte d’Ivoire and Ghana, making them the leading cocoa-producing countries in the world. However, cocoa farming has been a major driver of deforestation and landscape degradation in West Africa. Various stakeholders are striving for a zero-deforestation cocoa sector by implementing sustainable farming strategies and a more transparent supply chain. In the context of tracking cocoa sources and contributing to cocoa-driven deforestation monitoring, the demand for accurate and up-to-date maps of cocoa plantations is increasing. Yet, access to limited reference data and imperfect data quality can impose challenges in producing reliable maps. This study classified full-sun-cocoa-growing areas using limited reference data relative to the large and heterogeneous study areas in Côte d’Ivoire and Ghana. A Sentinel-2 composite image of 2021 was generated to train a random forest model. We undertook reference data refinement, selection of the most important handcrafted features and data sampling to ensure spatial independence. After refining the quality of the reference data and despite their size reduction, the random forest performance was improved, achieving an overall accuracy of 85.1 ± 2.0% and an F1 score of 84.6 ± 2.4% (mean ± one standard deviation from ten bootstrapping iterations). Emphasis was given to the qualitative visual assessment of the map using very high-resolution images, which revealed cases of strong and weak generalisation capacity of the random forest. Further insight was gained from the comparative analysis of our map with two previous cocoa classification studies. Implications of the use of cocoa maps for reporting were discussed.

Published
2024

23. Free-flight experiments in LISA Pathfinder

Author

Armano, M., Audley, H., Auger, G., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Brandt, N., Bursi, A., Caleno, M., Cavalleri, A., Cesarini, A., Cruise, M., Cutler, C., Danzmann, K., Diepholz, I., Dolesi, R., Dunbar, N., Ferraioli, L., Ferroni, V., Fitzsimons, E., Freschi, M., Gallegos, J., Marirrodriga, C. Garcia., Gerndt, R., Gesa, LI., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hueller, M., Huesler, J., Inchauspe, H., Jennrich, O., Jetzer, P., Johlander, B., Karnesis, N., Kaune, B., Korsakova, N., Killow, C., Lloro, I., Maarschalkerweerd, R., Madden, S., Maghami, P., Mance, D., Martin, V., Martin-Porqueras, F., Mateos, I., McNamara, P., Mendes, J., Mendes, L., Moroni, A., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Prat, P., Ragnit, U., Ramos-Castro, J., Reiche, J., Perez, J. A. Romera., Robertson, D., Rozemeijer, H., Russano, G., Sarra, P., Schleicher, A., Slutsky, J., Sopuerta, C. F., Sumner, T., Texier, D., Thorpe, J., Trenkel, C., Tu, H. B., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Waschke, S., Wass, P., Wealthy, D., Wen, S., Weber, W., Wittchen, A., Zanoni, C., Ziegler, T., and Zweifel, P.

Subjects
General Relativity and Quantum Cosmology, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The LISA Pathfinder mission will demonstrate the technology of drag-free test masses for use as inertial references in future space-based gravitational wave detectors. To accomplish this, the Pathfinder spacecraft will perform drag-free flight about a test mass while measuring the acceleration of this primary test mass relative to a second reference test mass. Because the reference test mass is contained within the same spacecraft, it is necessary to apply forces on it to maintain its position and attitude relative to the spacecraft. These forces are a potential source of acceleration noise in the LISA Pathfinder system that are not present in the full LISA configuration. While LISA Pathfinder has been designed to meet it's primary mission requirements in the presence of this noise, recent estimates suggest that the on-orbit performance may be limited by this `suspension noise'. The drift-mode or free-flight experiments provide an opportunity to mitigate this noise source and further characterize the underlying disturbances that are of interest to the designers of LISA-like instruments. This article provides a high-level overview of these experiments and the methods under development to analyze the resulting data., Comment: 13 pages, 5 figures. Accepted to Journal Of Physics, Conference Series. Presented at 10th International LISA Symposium, May 2014, Gainesville, FL, USA

Published
2014
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24. Sensor noise in LISA Pathfinder : Laser frequency noise and its coupling to the optical test mass readout

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Brandt, N., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Flatscher, R., additional, Freschi, M., additional, García, A., additional, Gerndt, R., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Guzman, F., additional, Harrison, I., additional, Hartig, M.-S., additional, Hechenblaikner, G., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Johann, U., additional, Johlander, B., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, Lobo, J. A., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martin-Polo, L., additional, Martin-Porqueras, F., additional, Martino, J., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Monsky, A., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Sanjuan, J., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Steier, F., additional, Sumner, T., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wand, V., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2024
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25. State space modelling and data analysis exercises in LISA Pathfinder

Author

Nofrarias, M, Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Bogenstahl, J, Bortoluzzi, D, Brandt, N, Caleno, M, Cavalleri, A, Congedo, G, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, Dolesi, R, Dunbar, N, Fauste, J, Ferraioli, L, Fichter, V Ferroni W, Fitzsimons, E, Freschi, M, Marirrodriga, C García, Gerndt, R, Gesa, L, Gibert, F, Giardini, D, Grimani, C, Grynagier, A, Guzmán, F, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hoyland, D, Hueller, M, Huesler, J, Jennrich, O, Jetzer, P, Johlander, B, Karnesis, N, Korsakova, N, Killow, C, Llamas, X, Lloro, I, Lobo, A, Maarschalkerweerd, R, Madden, S, Mance, D, Mateos, I, McNamara, P W, Mendes, J, Mitchell, E, Nicolini, D, Nicolodi, D, Perreur-Lloyd, M, Plagnol, E, Prat, P, Ramos-Castro, J, Reiche, J, Perez, J A Romera, Robertson, D, Rozemeijer, H, Russano, G, Schleicher, A, Shaul, D, Sopuerta, CF, Sumner, T J, Taylor, A, Texier, D, Trenkel, C, Tu, H-B, Vitale, S, Wanner, G, Ward, H, Waschke, S, Wass, P, Wealthy, D, Wen, S, Weber, W J, Ziegler, T, and Zweifel, P

Subjects
General Relativity and Quantum Cosmology, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Data Analysis, Statistics and Probability, Physics - Instrumentation and Detectors
Abstract

LISA Pathfinder is a mission planned by the European Space Agency to test the key technologies that will allow the detection of gravitational waves in space. The instrument on-board, the LISA Technology package, will undergo an exhaustive campaign of calibrations and noise characterisation campaigns in order to fully describe the noise model. Data analysis plays an important role in the mission and for that reason the data analysis team has been developing a toolbox which contains all the functionalities required during operations. In this contribution we give an overview of recent activities, focusing on the improvements in the modelling of the instrument and in the data analysis campaigns performed both with real and simulated data., Comment: Plenary talk presented at the 9th International LISA Symposium, 21-25 May 2012, Paris

Published
2013

26. The Gravitational Universe

Author

Consortium, The eLISA, Seoane, P. Amaro, Aoudia, S., Audley, H., Auger, G., Babak, S., Baker, J., Barausse, E., Barke, S., Bassan, M., Beckmann, V., Benacquista, M., Bender, P. L., Berti, E., Binétruy, P., Bogenstahl, J., Bonvin, C., Bortoluzzi, D., Brause, N. C., Brossard, J., Buchman, S., Bykov, I., Camp, J., Caprini, C., Cavalleri, A., Cerdonio, M., Ciani, G., Colpi, M., Congedo, G., Conklin, J., Cornish, N., Danzmann, K., de Vine, G., DeBra, D., Freitag, M. Dewi, Di Fiore, L., Aguilo, M. Diaz, Diepholz, I., Dolesi, R., Dotti, M., Barranco, G. Fernández, Ferraioli, L., Ferroni, V., Finetti, N., Fitzsimons, E., Gair, J., Galeazzi, F., Garcia, A., Gerberding, O., Gesa, L., Giardini, D., Gibert, F., Grimani, C., Groot, P., Cervantes, F. Guzman, Haiman, Z., Halloin, H., Heinzel, G., Hewitson, M., Hogan, C., Holz, D., Hornstrup, A., Hoyland, D., Hoyle, C. D., Hueller, M., Hughes, S., Jetzer, P., Kalogera, V., Karnesis, N., Kilic, M., Killow, C., Klipstein, W., Kochkina, E., Korsakova, N., Krolak, A., Larson, S., Lieser, M., Littenberg, T., Livas, J., Lloro, I., Mance, D., Madau, P., Maghami, P., Mahrdt, C., Marsh, T., Mateos, I., Mayer, L., McClelland, D., McKenzie, K., McWilliams, S., Merkowitz, S., Miller, C., Mitryk, S., Moerschell, J., Mohanty, S., Monsky, A., Mueller, G., Müller, V., Nelemans, G., Nicolodi, D., Nissanke, S., Nofrarias, M., Numata, K., Ohme, F., Otto, M., Perreur-Lloyd, M., Petiteau, A., Phinney, E. S., Plagnol, E., Pollack, S., Porter, E., Prat, P., Preston, A., Prince, T., Reiche, J., Richstone, D., Robertson, D., Rossi, E. M., Rosswog, S., Rubbo, L., Ruiter, A., Sanjuan, J., Sathyaprakash, B. S., Schlamminger, S., Schutz, B., Schütze, D., Sesana, A., Shaddock, D., Shah, S., Sheard, B., Sopuerta, C. F., Spector, A., Spero, R., Stanga, R., Stebbins, R., Stede, G., Steier, F., Sumner, T., Sun, K. -X., Sutton, A., Tanaka, T., Tanner, D., Thorpe, I., Tröbs, M., Tinto, M., Tu, H. -B., Vallisneri, M., Vetrugno, D., Vitale, S., Volonteri, M., Wand, V., Wang, Y., Wanner, G., Ward, H., Ware, B., Wass, P., Weber, W. J., Yu, Y., Yunes, N., and Zweifel, P.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology
Abstract

The last century has seen enormous progress in our understanding of the Universe. We know the life cycles of stars, the structure of galaxies, the remnants of the big bang, and have a general understanding of how the Universe evolved. We have come remarkably far using electromagnetic radiation as our tool for observing the Universe. However, gravity is the engine behind many of the processes in the Universe, and much of its action is dark. Opening a gravitational window on the Universe will let us go further than any alternative. Gravity has its own messenger: Gravitational waves, ripples in the fabric of spacetime. They travel essentially undisturbed and let us peer deep into the formation of the first seed black holes, exploring redshifts as large as z ~ 20, prior to the epoch of cosmic re-ionisation. Exquisite and unprecedented measurements of black hole masses and spins will make it possible to trace the history of black holes across all stages of galaxy evolution, and at the same time constrain any deviation from the Kerr metric of General Relativity. eLISA will be the first ever mission to study the entire Universe with gravitational waves. eLISA is an all-sky monitor and will offer a wide view of a dynamic cosmos using gravitational waves as new and unique messengers to unveil The Gravitational Universe. It provides the closest ever view of the early processes at TeV energies, has guaranteed sources in the form of verification binaries in the Milky Way, and can probe the entire Universe, from its smallest scales around singularities and black holes, all the way to cosmological dimensions., Comment: 20 pages; submitted to the European Space Agency on May 24th, 2013 for the L2/L3 selection of ESA's Cosmic Vision program

Published
2013

27. From laboratory experiments to LISA Pathfinder: achieving LISA geodesic motion

Author

Antonucci, F, Armano, M, Audley, H, Auger, G, Benedetti, M, Binetruy, P, Boatella, C, Bogenstahl, J, Bortoluzzi, D, Bosetti, P, Brandt, N, Caleno, M, Cavalleri, A, Cesa, M, Chmeissani, M, Ciani, G, Conchillo, A, Congedo, G, Cristofolini, I, Cruise, M, Danzmann, K, De Marchi, F, Diaz-Aguilo, M, Diepholz, I, Dixon, G, Dolesi, R, Dunbar, N, Fauste, J, Ferraioli, L, Fertin, D, Fichter, W, Fitzsimons, E, Freschi, M, Marin, A García, Marirrodriga, C García, Gerndt, R, Gesa, L, Giardini, D, Gibert, F, Grimani, C, Grynagier, A, Guillaume, B, Guzmán, F, Harrison, I, Heinzel, G, Hewitson, M, Hollington, D, Hough, J, Hoyland, D, Hueller, M, Huesler, J, Jeannin, O, Jennrich, O, Jetzer, P, Johlander, B, Killow, C, Llamas, X, Lloro, I, Lobo, A, Maarschalkerweerd, R, Madden, S, Mance, D, Mateos, I, McNamara, P W, Mendestì, J, Mitchell, E, Monsky, A, Nicolini, D, Nicolodi, D, Nofrarias, M, Pedersen, F, Perreur-Lloyd, M, Perreca, A, Plagnol, E, Prat, P, Racca, G D, Rais, B, Ramos-Castro, J, Reiche, J, Perez, J A Romera, Robertson, D, Rozemeijer, H, Sanjuan, J, Schleicher, A, Schulte, M, Shaul, D, Stagnaro, L, Strandmoe, S, Steier, F, Sumner, T J, Taylor, A, Texier, D, Trenkel, C, Tombolato, D, Vitale, S, Wanner, G, Ward, H, Waschke, S, Wass, P, Weber, W J, and Zweifel, P

Subjects
General Relativity and Quantum Cosmology, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

This paper presents a quantitative assessment of the performance of the upcoming LISA Pathfinder geodesic explorer mission. The findings are based on the results of extensive ground testing and simulation campaigns using flight hardware and flight control and operations algorithms. The results show that, for the central experiment of measuring the stray differential acceleration between the LISA test masses, LISA Pathfinder will be able to verify the overall acceleration noise to within a factor two of the LISA requirement at 1 mHz and within a factor 6 at 0.1 mHz. We also discuss the key elements of the physical model of disturbances, coming from LISA Pathfinder and ground measurement, that will guarantee the LISA performance., Comment: Proceedings of the 8th LISA Symposium. To appear Class. Quantum Grav. 28 (2011)

Published
2010
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28. Tilt-to-length coupling in LISA Pathfinder: A data analysis

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Freschi, M., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Harrison, I., additional, Hartig, M-S., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Johann, U., additional, Johlander, B., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, Lobo, J. A., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martin-Polo, L., additional, Martin-Porqueras, F., additional, Martino, J., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Sanjuan, J., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Sumner, T., additional, Tevlin, L., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2023
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29. Measuring the Galactic Cosmic Ray flux with the LISA Pathfinder radiation monitor

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A.M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Finetti, N., Fitzsimons, E.D., Freschi, M., Gesa, L., Gibert, F., Giardini, D., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Korsakova, N., Killow, C.J., Lobo, J.A., Lloro, I., Liu, L., Lopez-Zaragoza, J.P., Maarschalkerweerd, R., Mance, D., Meshskar, N., Martín, V., Martin-Polo, L., Martino, J., Martin-Porqueras, F., Mateos, I., McNamara, P.W., Mendes, J., Mendes, L., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Robertson, D.I., Rivas, F., Russano, G., Slutsky, J., Sopuerta, C.F., Sumner, T., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P., Weber, W.J., Wissel, L., Wittchen, A., and Zweifel, P.

Published
2018
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30. ARE-Wochenbericht KW 22

Author

Buda, S, Dürrwald, R, Biere, B, Reiche, J, Buchholz, U, Tolksdorf, K, Schilling, J, Goerlitz, L, Streib, V, Preuß, U, Prahm, K, Krupka, S, Lehfeld, AS, Haas, W, and AGI-Studiengruppe

Subjects
ddc:610, 610 Medizin und Gesundheit
Abstract

Die Aktivität akuter Atemwegserkrankungen (ARE-Rate) in der Bevölkerung (GrippeWeb) ist in der 22. KW 2023 im Vergleich zur Vorwoche stabil geblieben. Die aktuelle ARE-Rate liegt im oberen Wertebereich der vorpandemischen Jahre zu dieser Zeit. Im ambulanten Bereich (Arbeitsgemeinschaft Influenza) ist die Zahl der Arztbesuche wegen ARE im Vergleich zur Vorwoche deutlich gesunken. Sie liegt ebenfalls im oberen Wertebereich der vorpandemischen Jahre zu dieser Zeit. Im NRZ für Influenzaviren wurden in der 22. KW 2023 in insgesamt 15 (38 %) der 40 eingesandten Sentinelproben respiratorische Viren identifiziert, darunter 14 (35 %) Proben mit Rhinoviren sowie jeweils eine (3 %) Probe mit Parainfluenzaviren (PIV), Influenzaviren bzw. humanen saisonalen Coronaviren (hCoV). Weitere Viren des Erregerpanels wurden in der 22. KW nicht nachgewiesen. Im Rahmen der ICD-10-Code basierten Krankenhaussurveillance (ICOSARI) ist die Zahl schwerer akuter respiratorischer Infektionen (SARI) in den letzten Wochen gesunken und lag in der 22. KW 2023 auf Sommerniveau. Unter den in der 22. KW 2023 wegen einer schweren Atemwegserkrankung hospitalisierten Patientinnen und Patienten erhielten 5 % eine COVID-19-Diagnose, 1 % eine Influenza-Diagnose und weniger als 1 % eine RSV-Diagnose. Die ARE-Aktivität in der Bevölkerung ist für die Jahreszeit in der 22. KW 2023 immer noch vergleichsweise hoch. Sie ist hauptsächlich auf die Zirkulation von Rhinoviren zurückzuführen. Die Zahl schwer verlaufen der Atemwegsinfektionen bleibt weiterhin auf einem niedrigen Niveau.

Published
2023

31. Charging of free-falling test masses in orbit due to cosmic rays: Results from LISA Pathfinder

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Freschi, M., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Harrison, I., additional, Hartig, M.-S., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, Lobo, J. A., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martino, J., additional, Martin-Polo, L., additional, Martin-Porqueras, F., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Sumner, T. J., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2023
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32. Tilt-to-length coupling in LISA Pathfinder: A data analysis

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Johann, U., Johlander, B., Karnesis, N., Kaune, B., Killow, C. J., Korsakova, N., Lobo, J. A., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D. I., Russano, G., Sanjuan, J., Slutsky, J., Sopuerta, C. F., Sumner, T., Tevlin, L., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Weber, W. J., Wissel, L., Wittchen, A., Zweifel, P., Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E. D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Johann, U., Johlander, B., Karnesis, N., Kaune, B., Killow, C. J., Korsakova, N., Lobo, J. A., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., McNamara, P. W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D. I., Russano, G., Sanjuan, J., Slutsky, J., Sopuerta, C. F., Sumner, T., Tevlin, L., Texier, D., Thorpe, J. I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P. J., Weber, W. J., Wissel, L., Wittchen, A., and Zweifel, P.

Abstract

We present a study of the tilt-to-length coupling noise during the LISA Pathfinder mission and how it depended on the system's alignment. Tilt-to-length coupling noise is the unwanted coupling of angular and lateral spacecraft or test mass motion into the primary interferometric displacement readout. It was one of the major noise sources in the LISA Pathfinder mission and is likewise expected to be a primary noise source in LISA. We demonstrate here that a recently derived and published analytical model describes the dependency of the LISA Pathfinder tilt-to-length coupling noise on the alignment of the two freely falling test masses. This was verified with the data taken before and after the realignments performed in March (engineering days) and June 2016, and during a two-day experiment in February 2017 (long cross-talk experiment). The latter was performed with the explicit goal of testing the tilt-to-length coupling noise dependency on the test mass alignment. Using the analytical model, we show that all realignments performed during the mission were only partially successful and explain the reasons why. In addition to the analytical model, we computed another physical tilt-to-length coupling model via a minimizing routine making use of the long cross-talk experiment data. A similar approach could prove useful for the LISA mission.

Published
2023

33. Charging of free-falling test masses in orbit due to cosmic rays: Results from LISA Pathfinder

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A.M., Danzmann, K., De Deus, Silva M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E.D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M.-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Killow, C.J., Korsakova, N., Lobo, J.A., López-Zaragoza, J.P., Maarschalkerweerd, R., Mance, D., Martín, V., Martino, J., Martin-Polo, L., Martin-Porqueras, F., McNamara, P.W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D.I., Russano, G., Slutsky, J., Sopuerta, C.F., Sumner, T.J., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P.J., Weber, W.J., Wissel, L., Wittchen, A., Zweifel, P., Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A.M., Danzmann, K., De Deus, Silva M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E.D., Freschi, M., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Harrison, I., Hartig, M.-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Karnesis, N., Kaune, B., Killow, C.J., Korsakova, N., Lobo, J.A., López-Zaragoza, J.P., Maarschalkerweerd, R., Mance, D., Martín, V., Martino, J., Martin-Polo, L., Martin-Porqueras, F., McNamara, P.W., Mendes, J., Mendes, L., Meshksar, N., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D.I., Russano, G., Slutsky, J., Sopuerta, C.F., Sumner, T.J., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wanner, G., Ward, H., Wass, P.J., Weber, W.J., Wissel, L., Wittchen, A., and Zweifel, P.

Abstract

A comprehensive summary of the measurements made to characterize test-mass charging due to the space environment during the LISA Pathfinder mission is presented. Measurements of the residual charge of the test mass after release by the grabbing and positioning mechanism show that the initial charge of the test masses was negative after all releases, leaving the test mass with a potential in the range from -12 to -512. Variations in the neutral test-mass charging rate between 21.7 and 30.7 e s-1 were observed over the course of the 17-month science operations produced by cosmic ray flux changes including a Forbush decrease associated with a small solar energetic particle event. A dependence of the cosmic ray charging rate on the test-mass potential between -30.2 and -40.3 e s-1 V-1 was observed resulting in an equilibrium test-mass potential between 670 and 960 mV, and this is attributed to a contribution to charging from low-energy electrons emitted from the gold surfaces of the gravitational reference sensor. Data from the onboard particle detector show a reliable correlation with the charging rate and with other environmental monitors of the cosmic ray flux. This correlation is exploited to extrapolate test-mass charging rates to a 20-year period giving useful insight into the expected range of charging rate that may be observed in the LISA mission.

Published
2023

34. Seasonal Forest Disturbance Detection Using Sentinel-1 SAR & Sentinel-2 Optical Timeseries Data and Transformers

Author

Mullissa, A.G., Reiche, J., Saatchi, Sassan S., Mullissa, A.G., Reiche, J., and Saatchi, Sassan S.

Abstract

Tropical seasonal forests make up 40% of the globally available forest stock and play an essential role in regulating the variability in the global carbon cycle. Therefore, there is a strong need to persistently monitor seasonal forest changes to understand the forest carbon fluctuation and to better conserve biodiversity and enforce laws. In this regard, the advent of the European Space Agency (ESA) Copernicus program avails a dense time-series of both Synthetic Aperture Radar (SAR) and optical images, globally and free of charge, that enables the exploitation of these images for near real-time forest monitoring. Detecting seasonal forest changes in dense time-series, however, is complicated by fluctuation in the detected signal that is induced by forest phenology change. Therefore, forest disturbance detection methods should account for these seasonal fluctuations to make an accurate inference about forest disturbances. In this regard, deep learning approaches designed for sequential data such as Transformers can be used to implicitly learn the natural forest seasonality pattern in the signal to detect forest disturbances. This abstract demonstrates the efficacy of Transformers to detect seasonal forest disturbance in a seasonal dry-forest region in Bolivia.

Published
2023

35. ARE-Wochenbericht KW 19

Author

Buda, S, Dürrwald, R, Biere, B, Reiche, J, Buchholz, U, Tolksdorf, K, Schilling, J, Goerlitz, L, Streib, V, Preuß, U, Prahm, K, Krupka, S, and Haas, W

Subjects
ddc:610, 610 Medizin und Gesundheit
Abstract

Die Aktivität akuter Atemwegserkrankungen (ARE-Rate) in der Bevölkerung (GrippeWeb) ist in der 19. KW im Vergleich zur Vorwoche leicht gesunken. Die aktuelle ARE-Rate lag über den Werten der vorpandemi-schen Jahre zu dieser Zeit. Im ambulanten Bereich (Arbeitsgemeinschaft Influenza) ist die Zahl der Arztbesuche wegen ARE im Vergleich zur Vorwoche weiter gesunken. Auch die Zahl der Arztbesuche lag über dem Wertebereich der vorpandemischen Jahre zu dieser Zeit. Im NRZ für Influenzaviren wurden in der 19. KW 2023 in insgesamt 28 (47 %) der 60 eingesandten Sentinelproben respiratorische Viren identifiziert, darunter zehn (17 %) Proben mit humanen saisonalen Coronaviren (hCoV), acht (13 %) mit Rhinoviren, sechs (10 %) mit Influenzaviren, drei (5 %) mit Parainfluenzaviren (PIV) und drei (5 %) Proben mit SARS-CoV-2. Humane Metapneumoviren (hMPV) und Respiratorische Synzytialviren (RSV) wurden in der 19. KW nicht nachgewiesen. Im Rahmen der ICD-10-Code basierten Krankenhaussurveillance (ICOSARI) ist die Zahl schwerer akuter respiratorischer Infektionen (SARI) in den letzten Wochen gesunken und lag in der 19. KW 2023 weiterhin auf einem niedrigen Niveau. Insgesamt ist der Anteil der mit einer schweren Atemwegserkrankung hospitalisierten Patientinnen und Patienten mit einer COVID-19-Diagnose in der 19. KW 2023 erneut leicht gesunken und lag bei 9 %. Der Anteil an Influenza-Diagnosen bzw. an RSV-Diagnosen lag in der 19. KW 2023 jeweils bei 1 %. Die ARE-Aktivität in der Bevölkerung ist für die Jahreszeit in der 19. KW 2023 immer noch vergleichsweise hoch. Sie ist auf die Zirkulation unterschiedlicher Viren zurückzuführen, insbesondere auf hCoV, Rhinoviren und Influenzaviren. Die Zahl schwer verlaufender Atemwegsinfektionen liegt weiterhin auf einem niedrigen Niveau.

Published
2023

36. Monitoring direct drivers of small-scale tropical forest disturbance in near real-time with Sentinel-1 and -2 data

Author

Slagter, B., Reiche, J., Marcos, D., Mullissa, A., Lossou, E., Peña-Claros, M., and Herold, M.

Subjects
Near real-time monitoring, Forest degradation, Small-scale forest disturbance, Tropical forest, Deep learning, Deforestation, Smallholder agriculture, Driver attribution, Road development, Selective logging, Mining
Abstract

Advancements in satellite-based forest monitoring increasingly enable the near real-time detection of small-scale tropical forest disturbances. However, there is an urgent need to enhance such monitoring methods with automated direct driver attributions to detected disturbances. This would provide important additional information to make forest disturbance alerts more actionable and useful for uptake by different stakeholders. In this study, we demonstrate spatially explicit and near real-time methods to monitor direct drivers of small-scale tropical forest disturbance across a range of tropical forest conditions in Suriname, the Republic of the Congo and the Democratic Republic of the Congo. We trained a convolutional neural network with Sentinel-1 and Sentinel-2 data to continuously classify newly detected RAdar for Detecting Deforestation (RADD) alerts as smallholder agriculture, road development, selective logging, mining or other. Different monitoring scenarios were evaluated based on varying sensor combinations, post-disturbance time periods and confidence levels. In general, the use of Sentinel-2 data was found to be most accurate for driver classifications, especially with data composited over a period of 4 to 6 months after the disturbance detection. Sentinel-1 data showed to be valuable for more rapid classifications of specific drivers, especially in areas with persistent cloud cover. Throughout all monitoring scenarios, smallholder agriculture was classified most accurately, while road development, selective logging and mining were more challenging to distinguish. An accuracy assessment throughout the full extent of our study regions revealed a Macro-F1 score of 0.861 and an Overall Accuracy of 0.897 for the best performing model, based on the use of 6-month post-disturbance Sentinel-2 composites. Finally, we addressed three specific monitoring use cases that relate to rapid law enforcement against illegal activities, ecological impact assessments and timely carbon emission reporting, by optimizing the trade-off in classification timeliness and confidence to reach required accuracies. Our findings demonstrate the strong capacities of high spatiotemporal resolution satellite data for monitoring direct drivers of small-scale forest disturbance, considering different user interests. The produced forest disturbance driver maps can be accessed via: https://bartslagter94.users.earthengine.app/view/forest-disturbance-drivers.

Published
2023

37. Sensor noise in LISA Pathfinder : An extensive in-flight review of the angular and longitudinal interferometric measurement system

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Brandt, N., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Flatscher, R., additional, Freschi, M., additional, García, A., additional, Gerndt, R., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Guzman, F., additional, Harrison, I., additional, Hartig, M-S, additional, Hechenblaikner, G., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Johann, U., additional, Johlander, B., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, Lobo, J. A., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martin-Polo, L., additional, Martin-Porqueras, F., additional, Martino, J., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Monsky, A., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Sanjuan, J., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Steier, F., additional, Sumner, T., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wand, V., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2022
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39. Space-based detectors

Author

Sesana, A., Weber, W. J., Killow, C. J., Perreur-Lloyd, M., Robertson, D. I., Ward, H., Fitzsimons, E. D., Bryant, J., Cruise, A. M., Dixon, G., Hoyland, D., Smith, D., Bogenstahl, J., McNamara, P. W., Gerndt, R., Flatscher, R., Hechenblaikner, G., Hewitson, M., Gerberding, O., Barke, S., Brause, N., Bykov, I., Danzmann, K., Enggaard, A., Gianolio, A., Vendt Hansen, T., Heinzel, G., Hornstrup, A., Jennrich, O., Kullmann, J., Møller-Pedersen, S., Rasmussen, T., Reiche, J., Sodnik, Z., Suess, M., Armano, M., Sumner, T., Bender, P. L., Akutsu, T., Sathyaprakash, B. S., and DECIGO working group

Published
2014
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41. Stray light in the LISA mission: perturbation of an interferometer due to back-scattered light

Author

Rohr, J. Max, Lintz, Michel, Ast, S., Gerberding, O., Reiche, J., Heinzel, G., Khodnevych, V., Nardello, M., Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), CNES, INFN, and LISA Laser Interferometer Space Antenna https://www.lisamission.org

Subjects
Ondes gravitationnelles, [SPI]Engineering Sciences [physics], interférométrie laser, [SDU]Sciences of the Universe [physics], Astrophysics::Instrumentation and Methods for Astrophysics, Physics::Optics, rétrodiffusion, lumière parasite, Interference & diffraction of light, Gravitational wave detectors
Abstract

International audience; LISA is a constellation of three spacecraft exchanging laser beams on a 2.5 Mkm triangle. The GW measurement exploits heterodyne interferometric phase measurements of the distance between distant optical benches, with additional interferometers measuring the test mass to optical bench movement, and the optical phase difference of the two lasers onboard the same spacecraft. Stray light (SL) can affect the operations in various ways, but the most obvious perturbation comes from coherent SL being recoupled into one of the interferometers.We present activities aiming at- characterizing the re-coupling of SL scattered from a mirror, back into a Michelson interferometer where a collimated beam hits the mirror under test. Back-scatter (BS) from the mirror is measured down to 10^-13 in power- providing a simple and approximate, yet analytic method to estimate the fraction of BS recoupled into an interferometer: when a complex optics, such as a telescope, is involved, considering only BS rays in the solid angle corresponding to an overlap with the beam waist provides a reasonably precise value of coupled SL- measuring Rayleigh BS from the "back-link" optical fibre. The back-link allows to prepare the beating of one laser with the other laser on the same spacecraft. We use a heterodyne Mach-Zehnder interferometer to measure BS power in the ppm-level. We also characterize the fibers' reaction to stress and ionizing radiation. Mitigation strategies are presented.

Published
2021

42. Sensor Noise in LISA Pathfinder: In-Flight Performance of the Optical Test Mass Readout

Author

Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Brandt, N., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E.D., Flatscher, R., Freschi, M., García, A., Gerndt, R., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Guzman, F., Harrison, I., Hartig, M.-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Johann, U., Johlander, B., Karnesis, N., Kaune, B., Killow, C.J., Korsakova, N., Lobo, J.A., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., McNamara, P.W., Mendes, J., Mendes, L., Meshksar, N., Monsky, A., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D.I., Russano, G., Sanjuan, J., Slutsky, J., Sopuerta, C.F., Steier, F., Sumner, T., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wand, V., Wanner, G., Ward, H., Wass, P. J., Weber, W.J., Wissel, L., Wittchen, A., Zweifel, P., Armano, M., Audley, H., Baird, J., Binetruy, P., Born, M., Bortoluzzi, D., Brandt, N., Castelli, E., Cavalleri, A., Cesarini, A., Cruise, A. M., Danzmann, K., de Deus Silva, M., Diepholz, I., Dixon, G., Dolesi, R., Ferraioli, L., Ferroni, V., Fitzsimons, E.D., Flatscher, R., Freschi, M., García, A., Gerndt, R., Gesa, L., Giardini, D., Gibert, F., Giusteri, R., Grimani, C., Grzymisch, J., Guzman, F., Harrison, I., Hartig, M.-S., Heinzel, G., Hewitson, M., Hollington, D., Hoyland, D., Hueller, M., Inchauspé, H., Jennrich, O., Jetzer, P., Johann, U., Johlander, B., Karnesis, N., Kaune, B., Killow, C.J., Korsakova, N., Lobo, J.A., Liu, L., López-Zaragoza, J. P., Maarschalkerweerd, R., Mance, D., Martín, V., Martin-Polo, L., Martin-Porqueras, F., Martino, J., McNamara, P.W., Mendes, J., Mendes, L., Meshksar, N., Monsky, A., Nofrarias, M., Paczkowski, S., Perreur-Lloyd, M., Petiteau, A., Pivato, P., Plagnol, E., Ramos-Castro, J., Reiche, J., Rivas, F., Robertson, D.I., Russano, G., Sanjuan, J., Slutsky, J., Sopuerta, C.F., Steier, F., Sumner, T., Texier, D., Thorpe, J.I., Vetrugno, D., Vitale, S., Wand, V., Wanner, G., Ward, H., Wass, P. J., Weber, W.J., Wissel, L., Wittchen, A., and Zweifel, P.

Abstract

We report on the first subpicometer interferometer flown in space. It was part of ESA's Laser Interferometer Space Antenna (LISA) Pathfinder mission and performed the fundamental measurement of the positional and angular motion of two free-falling test masses. The interferometer worked immediately, stably, and reliably from switch on until the end of the mission with exceptionally low residual noise of 32.0-1.7+2.4 fm/Hz, significantly better than required. We present an upper limit for the sensor performance at millihertz frequencies and a model for the measured sensitivity above 200 mHz.

Published
2021

45. Sensor Noise in LISA Pathfinder : In-Flight Performance of the Optical Test Mass Readout

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Brandt, N., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Flatscher, R., additional, Freschi, M., additional, García, A., additional, Gerndt, R., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Guzman, F., additional, Harrison, I., additional, Hartig, M.-S., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Johann, U., additional, Johlander, B., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, Lobo, J. A., additional, Liu, L., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martin-Polo, L., additional, Martin-Porqueras, F., additional, Martino, J., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Monsky, A., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Pivato, P., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Sanjuan, J., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Steier, F., additional, Sumner, T., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wand, V., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2021
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48. Spacecraft and interplanetary contributions to the magnetic environment on-board LISA Pathfinder

Author

Armano, M, primary, Audley, H, additional, Baird, J, additional, Binetruy, P, additional, Born, M, additional, Bortoluzzi, D, additional, Castelli, E, additional, Cavalleri, A, additional, Cesarini, A, additional, Cruise, A M, additional, Danzmann, K, additional, de Deus Silva, M, additional, Diepholz, I, additional, Dixon, G, additional, Dolesi, R, additional, Ferraioli, L, additional, Ferroni, V, additional, Fitzsimons, E D, additional, Freschi, M, additional, Gesa, L, additional, Gibert, F, additional, Giardini, D, additional, Giusteri, R, additional, Grimani, C, additional, Grzymisch, J, additional, Harrison, I, additional, Hartig, M-S, additional, Heinzel, G, additional, Hewitson, M, additional, Hollington, D, additional, Hoyland, D, additional, Hueller, M, additional, Inchauspé, H, additional, Jennrich, O, additional, Jetzer, P, additional, Karnesis, N, additional, Kaune, B, additional, Korsakova, N, additional, Killow, C J, additional, Lobo, J A, additional, Liu, L, additional, López-Zaragoza, J P, additional, Maarschalkerweerd, R, additional, Mance, D, additional, Martín, V, additional, Martin-Polo, L, additional, Martino, J, additional, Martin-Porqueras, F, additional, Mateos, I, additional, McNamara, P W, additional, Mendes, J, additional, Mendes, L, additional, Meshksar, N, additional, Nofrarias, M, additional, Paczkowski, S, additional, Perreur-Lloyd, M, additional, Petiteau, A, additional, Pivato, P, additional, Plagnol, E, additional, Ramos-Castro, J, additional, Reiche, J, additional, Rivas, F, additional, Robertson, D I, additional, Roma-Dollase, D, additional, Russano, G, additional, Slutsky, J, additional, Sopuerta, C F, additional, Sumner, T, additional, Telloni, D, additional, Texier, D, additional, Thorpe, J I, additional, Trenkel, C, additional, Vetrugno, D, additional, Vitale, S, additional, Wanner, G, additional, Ward, H, additional, Wass, P J, additional, Wealthy, D, additional, Weber, W J, additional, Wissel, L, additional, Wittchen, A, additional, and Zweifel, P, additional

Published
2020
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49. Analysis of the accuracy of actuation electronics in the laser interferometer space antenna pathfinder

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Born, M., additional, Bortoluzzi, D., additional, Cardines, N., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Freschi, M., additional, Gesa, L., additional, Giardini, D., additional, Gibert, F., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Harrison, I., additional, Hartig, M.-S., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Karnesis, N., additional, Kaune, B., additional, Killow, C. J., additional, Korsakova, N., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Martín, V., additional, Martin-Polo, L., additional, Martino, J., additional, Martin-Porqueras, F., additional, Mateos, I., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Meshksar, N., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Pivato, P., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Rivas, F., additional, Robertson, D. I., additional, Russano, G., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Sumner, T., additional, Texier, D., additional, ten Pierick, J., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wanner, G., additional, Ward, H., additional, Wass, P. J., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2020
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50. LISA Pathfinder

Author

Armano, M., primary, Audley, H., additional, Baird, J., additional, Binetruy, P., additional, Born, M., additional, Bortoluzzi, D., additional, Castelli, E., additional, Cavalleri, A., additional, Cesarini, A., additional, Cruise, A. M., additional, Danzmann, K., additional, de Deus Silva, M., additional, Diepholz, I., additional, Dixon, G., additional, Dolesi, R., additional, Ferraioli, L., additional, Ferroni, V., additional, Fitzsimons, E. D., additional, Freschi, M., additional, Gesa, L., additional, Gibert, F., additional, Giardini, D., additional, Giusteri, R., additional, Grimani, C., additional, Grzymisch, J., additional, Harrison, I., additional, Heinzel, G., additional, Hewitson, M., additional, Hollington, D., additional, Hoyland, D., additional, Hueller, M., additional, Inchauspé, H., additional, Jennrich, O., additional, Jetzer, P., additional, Karnesis, N., additional, Kaune, B., additional, Korsakova, N., additional, Killow, C. J., additional, Lobo, J. A., additional, Lloro, I., additional, Liu, L., additional, López-Zaragoza, J. P., additional, Maarschalkerweerd, R., additional, Mance, D., additional, Meshskar, N., additional, Martín, V., additional, Martin-Polo, L., additional, Martino, J., additional, Martin-Porqueras, F., additional, Mateos, I., additional, McNamara, P. W., additional, Mendes, J., additional, Mendes, L., additional, Nofrarias, M., additional, Paczkowski, S., additional, Perreur-Lloyd, M., additional, Petiteau, A., additional, Pivato, P., additional, Plagnol, E., additional, Ramos-Castro, J., additional, Reiche, J., additional, Robertson, D. I., additional, Rivas, F., additional, Russano, G., additional, Slutsky, J., additional, Sopuerta, C. F., additional, Sumner, T., additional, Texier, D., additional, Thorpe, J. I., additional, Vetrugno, D., additional, Vitale, S., additional, Wanner, G., additional, Ward, H., additional, Wass, P., additional, Weber, W. J., additional, Wissel, L., additional, Wittchen, A., additional, and Zweifel, P., additional

Published
2020
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