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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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 |
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1724824995297755136 |