Noise Analysis of a Passive Resonant Laser Gyroscope

Large-scale laser gyroscopes have found important applications in Earth sciences due to their self-sufficient property of measurement of the Earth’s rotation without any external references. In order to extend the relative rotation measurement accuracy to a better level so that it can be used for th...

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Main Authors: Kui Liu, Fenglei Zhang, Zongyang Li, Xiaohua Feng, Ke Li, Yuanbo Du, Karl Ulrich Schreiber, Zehuang Lu, Jie Zhang
Format: Article
Language:English
Published: MDPI AG 2020-09-01
Series:Sensors
Subjects:
Online Access:https://www.mdpi.com/1424-8220/20/18/5369
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spelling doaj-9cf926c587c64426b1c61ae4bdcd36552020-11-25T02:31:23ZengMDPI AGSensors1424-82202020-09-01205369536910.3390/s20185369Noise Analysis of a Passive Resonant Laser GyroscopeKui Liu0Fenglei Zhang1Zongyang Li2Xiaohua Feng3Ke Li4Yuanbo Du5Karl Ulrich Schreiber6Zehuang Lu7Jie Zhang8MOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaTechnical University of Munich, Forschungseinrichtung Satellitengeodäsie, Geodetic Observatory Wettzell, 93444 Bad Kötzting, GermanyMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaMOE Key Laboratory of Fundamental Physical Quantities Measurements & Hubei Key Laboratory of Gravitation and Quantum Physics, PGMF and School of Physics, Huazhong University of Science and Technology, Wuhan 430074, ChinaLarge-scale laser gyroscopes have found important applications in Earth sciences due to their self-sufficient property of measurement of the Earth’s rotation without any external references. In order to extend the relative rotation measurement accuracy to a better level so that it can be used for the determination of the Earth orientation parameters (EOP), we investigate the limitations in a passive resonant laser gyroscope (PRG) developed at Huazhong University of Science and Technology (HUST) to pave the way for future development. We identify the noise sources from the derived noise transfer function of the PRG. In the frequency range below <inline-formula><math display="inline"><semantics><mrow><msup><mn>10</mn><mrow><mo>−</mo><mn>2</mn></mrow></msup><mspace width="3.33333pt"></mspace><mi>Hz</mi></mrow></semantics></math></inline-formula>, the contribution of free-spectral-range (FSR) variation is the dominant limitation, which comes from the drift of the ring cavity length. In the <inline-formula><math display="inline"><semantics><msup><mn>10</mn><mrow><mo>−</mo><mn>2</mn></mrow></msup></semantics></math></inline-formula> to <inline-formula><math display="inline"><semantics><mrow><msup><mn>10</mn><mn>3</mn></msup><mspace width="3.33333pt"></mspace><mi>Hz</mi></mrow></semantics></math></inline-formula> frequency range, the limitation is due to the noises of the frequency discrimination system, which mainly comes from the residual amplitude modulation (RAM) in the frequency range below 2 Hz. In addition, the noise contributed by the Mach–Zehnder-type beam combiner is also noticeable in the 0.01 to 2 Hz frequency range. Finally, possible schemes for future improvement are also discussed.https://www.mdpi.com/1424-8220/20/18/5369passive resonant laser gyroscopeEarth rotationSagnac effectnoise analysis
collection DOAJ
language English
format Article
sources DOAJ
author Kui Liu
Fenglei Zhang
Zongyang Li
Xiaohua Feng
Ke Li
Yuanbo Du
Karl Ulrich Schreiber
Zehuang Lu
Jie Zhang
spellingShingle Kui Liu
Fenglei Zhang
Zongyang Li
Xiaohua Feng
Ke Li
Yuanbo Du
Karl Ulrich Schreiber
Zehuang Lu
Jie Zhang
Noise Analysis of a Passive Resonant Laser Gyroscope
Sensors
passive resonant laser gyroscope
Earth rotation
Sagnac effect
noise analysis
author_facet Kui Liu
Fenglei Zhang
Zongyang Li
Xiaohua Feng
Ke Li
Yuanbo Du
Karl Ulrich Schreiber
Zehuang Lu
Jie Zhang
author_sort Kui Liu
title Noise Analysis of a Passive Resonant Laser Gyroscope
title_short Noise Analysis of a Passive Resonant Laser Gyroscope
title_full Noise Analysis of a Passive Resonant Laser Gyroscope
title_fullStr Noise Analysis of a Passive Resonant Laser Gyroscope
title_full_unstemmed Noise Analysis of a Passive Resonant Laser Gyroscope
title_sort noise analysis of a passive resonant laser gyroscope
publisher MDPI AG
series Sensors
issn 1424-8220
publishDate 2020-09-01
description Large-scale laser gyroscopes have found important applications in Earth sciences due to their self-sufficient property of measurement of the Earth’s rotation without any external references. In order to extend the relative rotation measurement accuracy to a better level so that it can be used for the determination of the Earth orientation parameters (EOP), we investigate the limitations in a passive resonant laser gyroscope (PRG) developed at Huazhong University of Science and Technology (HUST) to pave the way for future development. We identify the noise sources from the derived noise transfer function of the PRG. In the frequency range below <inline-formula><math display="inline"><semantics><mrow><msup><mn>10</mn><mrow><mo>−</mo><mn>2</mn></mrow></msup><mspace width="3.33333pt"></mspace><mi>Hz</mi></mrow></semantics></math></inline-formula>, the contribution of free-spectral-range (FSR) variation is the dominant limitation, which comes from the drift of the ring cavity length. In the <inline-formula><math display="inline"><semantics><msup><mn>10</mn><mrow><mo>−</mo><mn>2</mn></mrow></msup></semantics></math></inline-formula> to <inline-formula><math display="inline"><semantics><mrow><msup><mn>10</mn><mn>3</mn></msup><mspace width="3.33333pt"></mspace><mi>Hz</mi></mrow></semantics></math></inline-formula> frequency range, the limitation is due to the noises of the frequency discrimination system, which mainly comes from the residual amplitude modulation (RAM) in the frequency range below 2 Hz. In addition, the noise contributed by the Mach–Zehnder-type beam combiner is also noticeable in the 0.01 to 2 Hz frequency range. Finally, possible schemes for future improvement are also discussed.
topic passive resonant laser gyroscope
Earth rotation
Sagnac effect
noise analysis
url https://www.mdpi.com/1424-8220/20/18/5369
work_keys_str_mv AT kuiliu noiseanalysisofapassiveresonantlasergyroscope
AT fengleizhang noiseanalysisofapassiveresonantlasergyroscope
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AT keli noiseanalysisofapassiveresonantlasergyroscope
AT yuanbodu noiseanalysisofapassiveresonantlasergyroscope
AT karlulrichschreiber noiseanalysisofapassiveresonantlasergyroscope
AT zehuanglu noiseanalysisofapassiveresonantlasergyroscope
AT jiezhang noiseanalysisofapassiveresonantlasergyroscope
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