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On orbit performance of the GRACE Follow-On Laser Ranging Interferometer
The Laser Ranging Interferometer (LRI) instrument on the Gravity Recovery and Climate Experiment (GRACE) Follow-On mission has provided the first laser interferometric range measurements between remote spacecraft, separated by approximately 220 km. Autonomous controls that lock the laser frequency t...
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creator | Abich, Klaus Braxmaier, Claus Gohlke, Martin Sanjuan, Josep Abramovici, Alexander Brian Bachman Okihiro Barr, David C Bize, Maxime P Burke, Michael J Clark, Ken C de Vine, Glenn Dickson, Jeffrey A Dubovitsky, Serge Folkner, William M Francis, Samuel Gilbert, Martin S Katsumura, Mark Klipstein, William Larsen, Kameron Liebe, Carl Christian Liu, Jehhal McKenzie, Kirk Morton, Phillip R Murray, Alexander T Nguyen, Don J Ravich, Joshua A Shaddock, Daniel Spero, Robert Spiers, Gary Sutton, Andrew Trinh, Joseph Wang, Duo Wang, Rabi T Ware, Brent Woodruff, Christopher Amparan, Bengie Davis, Mike A Howell, James Kruger, Micah Lobmeyer, Lynette Pierce, Robert Reavis, Gretchen Sileo, Michael Stephens, Michelle Baatzsch, Andreas Dahl, Christian Dahl, Katrin Gilles, Frank Hager, Philipp Herding, Mark Kaufer, Marina Nicklaus, Kolja Voss, Kai Bogan, Christina Danzmann, Karsten Germán Fernández Barranco Heinzel, Gerhard Koch, Alexander Mahrdt, Christoph Misfeldt, Malte Müller, Vitali Reiche, Jens Schütze, Daniel Sheard, Benjamin Stede, Gunnar Wegener, Henry Eckardt, Andreas Burghardt Guenther Mangoldt, Thomas Zender, Bernd Thomas, Ester Heine, Frank Seiter, Christoph Windisch, Steve Flatscher, Reinhold Flechtner, Frank Grossard, Nicolas Hauden, Jerome Hinz, Martin Leikert, Thomas Zimmermann, Marcus Lebeda, Anton Arnold Lebeda |
description | The Laser Ranging Interferometer (LRI) instrument on the Gravity Recovery and Climate Experiment (GRACE) Follow-On mission has provided the first laser interferometric range measurements between remote spacecraft, separated by approximately 220 km. Autonomous controls that lock the laser frequency to a cavity reference and establish the 5 degree of freedom two-way laser link between remote spacecraft succeeded on the first attempt. Active beam pointing based on differential wavefront sensing compensates spacecraft attitude fluctuations. The LRI has operated continuously without breaks in phase tracking for more than 50 days, and has shown biased range measurements similar to the primary ranging instrument based on microwaves, but with much less noise at a level of \(1\,{\rm nm}/\sqrt{\rm Hz}\) at Fourier frequencies above 100 mHz. |
doi_str_mv | 10.48550/arxiv.1907.00104 |
format | article |
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Autonomous controls that lock the laser frequency to a cavity reference and establish the 5 degree of freedom two-way laser link between remote spacecraft succeeded on the first attempt. Active beam pointing based on differential wavefront sensing compensates spacecraft attitude fluctuations. The LRI has operated continuously without breaks in phase tracking for more than 50 days, and has shown biased range measurements similar to the primary ranging instrument based on microwaves, but with much less noise at a level of \(1\,{\rm nm}/\sqrt{\rm Hz}\) at Fourier frequencies above 100 mHz.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1907.00104</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>GRACE (experiment) ; Laser beams ; Laser ranging ; Lasers ; Microwaves ; Variation ; Wave fronts</subject><ispartof>arXiv.org, 2019-06</ispartof><rights>2019. 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Autonomous controls that lock the laser frequency to a cavity reference and establish the 5 degree of freedom two-way laser link between remote spacecraft succeeded on the first attempt. Active beam pointing based on differential wavefront sensing compensates spacecraft attitude fluctuations. The LRI has operated continuously without breaks in phase tracking for more than 50 days, and has shown biased range measurements similar to the primary ranging instrument based on microwaves, but with much less noise at a level of \(1\,{\rm nm}/\sqrt{\rm Hz}\) at Fourier frequencies above 100 mHz.</description><subject>GRACE (experiment)</subject><subject>Laser beams</subject><subject>Laser ranging</subject><subject>Lasers</subject><subject>Microwaves</subject><subject>Variation</subject><subject>Wave 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Marcus</creatorcontrib><creatorcontrib>Lebeda, Anton</creatorcontrib><creatorcontrib>Arnold Lebeda</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content (ProQuest)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abich, Klaus</au><au>Braxmaier, Claus</au><au>Gohlke, Martin</au><au>Sanjuan, Josep</au><au>Abramovici, Alexander</au><au>Brian Bachman Okihiro</au><au>Barr, David C</au><au>Bize, Maxime P</au><au>Burke, Michael J</au><au>Clark, Ken C</au><au>de Vine, Glenn</au><au>Dickson, Jeffrey A</au><au>Dubovitsky, Serge</au><au>Folkner, William M</au><au>Francis, Samuel</au><au>Gilbert, Martin S</au><au>Katsumura, Mark</au><au>Klipstein, William</au><au>Larsen, Kameron</au><au>Liebe, Carl Christian</au><au>Liu, Jehhal</au><au>McKenzie, Kirk</au><au>Morton, Phillip R</au><au>Murray, Alexander T</au><au>Nguyen, Don J</au><au>Ravich, Joshua A</au><au>Shaddock, Daniel</au><au>Spero, Robert</au><au>Spiers, Gary</au><au>Sutton, Andrew</au><au>Trinh, Joseph</au><au>Wang, Duo</au><au>Wang, Rabi T</au><au>Ware, Brent</au><au>Woodruff, Christopher</au><au>Amparan, Bengie</au><au>Davis, Mike A</au><au>Howell, James</au><au>Kruger, Micah</au><au>Lobmeyer, Lynette</au><au>Pierce, Robert</au><au>Reavis, Gretchen</au><au>Sileo, Michael</au><au>Stephens, Michelle</au><au>Baatzsch, Andreas</au><au>Dahl, Christian</au><au>Dahl, Katrin</au><au>Gilles, Frank</au><au>Hager, Philipp</au><au>Herding, Mark</au><au>Kaufer, Marina</au><au>Nicklaus, Kolja</au><au>Voss, Kai</au><au>Bogan, Christina</au><au>Danzmann, Karsten</au><au>Germán Fernández Barranco</au><au>Heinzel, Gerhard</au><au>Koch, Alexander</au><au>Mahrdt, Christoph</au><au>Misfeldt, Malte</au><au>Müller, Vitali</au><au>Reiche, Jens</au><au>Schütze, Daniel</au><au>Sheard, Benjamin</au><au>Stede, Gunnar</au><au>Wegener, Henry</au><au>Eckardt, Andreas</au><au>Burghardt Guenther</au><au>Mangoldt, Thomas</au><au>Zender, Bernd</au><au>Thomas, Ester</au><au>Heine, Frank</au><au>Seiter, Christoph</au><au>Windisch, Steve</au><au>Flatscher, Reinhold</au><au>Flechtner, Frank</au><au>Grossard, Nicolas</au><au>Hauden, Jerome</au><au>Hinz, Martin</au><au>Leikert, Thomas</au><au>Zimmermann, Marcus</au><au>Lebeda, Anton</au><au>Arnold Lebeda</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On orbit performance of the GRACE Follow-On Laser Ranging Interferometer</atitle><jtitle>arXiv.org</jtitle><date>2019-06-28</date><risdate>2019</risdate><eissn>2331-8422</eissn><abstract>The Laser Ranging Interferometer (LRI) instrument on the Gravity Recovery and Climate Experiment (GRACE) Follow-On mission has provided the first laser interferometric range measurements between remote spacecraft, separated by approximately 220 km. Autonomous controls that lock the laser frequency to a cavity reference and establish the 5 degree of freedom two-way laser link between remote spacecraft succeeded on the first attempt. Active beam pointing based on differential wavefront sensing compensates spacecraft attitude fluctuations. The LRI has operated continuously without breaks in phase tracking for more than 50 days, and has shown biased range measurements similar to the primary ranging instrument based on microwaves, but with much less noise at a level of \(1\,{\rm nm}/\sqrt{\rm Hz}\) at Fourier frequencies above 100 mHz.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1907.00104</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2019-06 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2250840992 |
source | Publicly Available Content (ProQuest) |
subjects | GRACE (experiment) Laser beams Laser ranging Lasers Microwaves Variation Wave fronts |
title | On orbit performance of the GRACE Follow-On Laser Ranging Interferometer |
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