The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance

The Ganymede Laser Altimeter (GALA) is one of the ten scientific instruments selected for the Jupiter Icy Moons Explorer (JUICE) mission currently implemented under responsibility of the European Space Agency (ESA). JUICE is scheduled for launch in mid 2022; arrival at Jupiter will be by end of 2029...

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Autores: Hussmann, Hauke, Lingenauber, Kay, Kallenbach, Reinald, Enya, Keigo, Thomas, Nicolas, Lara, Luisa María, Althaus, Christian L., Araki, Hiroshi, Behnke, Thomas, Castro Marín, J. M., Eisenmenger, Henri, Gerber, Thomas, Herranz, Miguel, Hüttig, Christian, Ishibashi, Ko, Jiménez Ortega, Jaime, Kimura, Jun, Kobayashi, Masanori, Lötzke, Horst-Georg, Lichopoj, Alexander, Lüdicke, Fabian, Martínez-Navajas, Ignacio, Michaelis, Harald, Namiki, Noriyuki, Noda, Hirotomo, Oberst, Jürgen, Oshigami, Shoko, Rodríguez García, Juan Pablo, Rodrigo, Julio, Rösner, Kerstin, Stark, Alexander, Steinbrügge, Gregor, Thabaut, Pascal, del Togno, Simone, Touhara, Kazuyuki, Villamil, Sebastian, Wendler, Belinda, Wickhusen, Kai, Willner, Konrad
Tipo de recurso: artículo
Estado:Versión aceptada para publicación
Fecha de publicación:2019
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/198157
Acceso en línea:http://hdl.handle.net/10261/198157
Access Level:acceso abierto
Palabra clave:Laser Altimetry
Solar System
Satellites of Jupiter
Ganymede
JUICE mission
GALA
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spelling The Ganymede laser altimeter (GALA): key objectives, instrument design, and performanceHussmann, HaukeLingenauber, KayKallenbach, ReinaldEnya, KeigoThomas, NicolasLara, Luisa MaríaAlthaus, Christian L.Araki, HiroshiBehnke, ThomasCastro Marín, J. M.Eisenmenger, HenriGerber, ThomasHerranz, MiguelHüttig, ChristianIshibashi, KoJiménez Ortega, JaimeKimura, JunKobayashi, MasanoriLötzke, Horst-GeorgLichopoj, AlexanderLüdicke, FabianMartínez-Navajas, IgnacioMichaelis, HaraldNamiki, NoriyukiNoda, HirotomoOberst, JürgenOshigami, ShokoRodríguez García, Juan PabloRodrigo, JulioRösner, KerstinStark, AlexanderSteinbrügge, GregorThabaut, Pascaldel Togno, SimoneTouhara, KazuyukiVillamil, SebastianWendler, BelindaWickhusen, KaiWillner, KonradLaser AltimetrySolar SystemSatellites of JupiterGanymedeJUICE missionGALAThe Ganymede Laser Altimeter (GALA) is one of the ten scientific instruments selected for the Jupiter Icy Moons Explorer (JUICE) mission currently implemented under responsibility of the European Space Agency (ESA). JUICE is scheduled for launch in mid 2022; arrival at Jupiter will be by end of 2029 with the nominal science mission—including close flybys at Ganymede, Europa, and Callisto and a Ganymede orbit phase—ending by mid 2033. GALA’s main objective is to obtain topographic data of the icy satellites of Jupiter: Europa, Ganymede, and Callisto. By measuring the diurnal tidal deformation of Ganymede, which crucially depends on the decoupling of the surface ice layer from the deep interior by a liquid water ocean, GALA will obtain evidence for (or against) a subsurface ocean in a 500 km orbit around the satellite and will provide constraints on Ganymede’s ice shell thickness. In combination with other instruments, it will characterize the morphology of surface units on Ganymede, Europa, and Callisto providing not only topography but also surface roughness and albedo (at 1064 nm) measurements. GALA is a single-beam laser altimeter operating with up to 50 Hz (nominal 30 Hz) shot frequency at a wavelength of 1064 nm and pulse lengths of 5.5 ± 2.5 ns using a Nd:YAG laser. The return pulse is detected by an Avalanche Photo Diode (APD) with 100 MHz bandwidth and is digitized at a sampling rate of 200 MHz providing range measurements with a subsample resolution of 0.1 m and surface roughness measurements from pulse-shape analysis on the scale of the footprint size of about 50 m at 500 km altitude. The instrument is developed in collaboration of institutes and industry from Germany, Japan, Switzerland, and Spain. © 2019, CEAS.Financial support was provided under grant 50 QJ 1401 on behalf of the DLR Space Administration by the German Bundesministerium fur Wirtschaft und Energie. This research has been supported by the Spanish Ministerio de Economia y Competitividad under Contract ESP 2016-76076-R.Peer reviewedSpringer NatureGerman Centre for Air and Space TravelMinisterio de Economía y Competitividad (España)European CommissionConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202020202019info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Postprintinfo:eu-repo/semantics/acceptedVersionhttp://hdl.handle.net/10261/198157reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Inglés#PLACEHOLDER_PARENT_METADATA_VALUE#info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2016-76076-Rhttp://dx.doi.org/10.1007/s12567-019-00282-8Síinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1981572026-05-22T06:33:51Z
dc.title.none.fl_str_mv The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
title The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
spellingShingle The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
Hussmann, Hauke
Laser Altimetry
Solar System
Satellites of Jupiter
Ganymede
JUICE mission
GALA
title_short The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
title_full The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
title_fullStr The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
title_full_unstemmed The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
title_sort The Ganymede laser altimeter (GALA): key objectives, instrument design, and performance
dc.creator.none.fl_str_mv Hussmann, Hauke
Lingenauber, Kay
Kallenbach, Reinald
Enya, Keigo
Thomas, Nicolas
Lara, Luisa María
Althaus, Christian L.
Araki, Hiroshi
Behnke, Thomas
Castro Marín, J. M.
Eisenmenger, Henri
Gerber, Thomas
Herranz, Miguel
Hüttig, Christian
Ishibashi, Ko
Jiménez Ortega, Jaime
Kimura, Jun
Kobayashi, Masanori
Lötzke, Horst-Georg
Lichopoj, Alexander
Lüdicke, Fabian
Martínez-Navajas, Ignacio
Michaelis, Harald
Namiki, Noriyuki
Noda, Hirotomo
Oberst, Jürgen
Oshigami, Shoko
Rodríguez García, Juan Pablo
Rodrigo, Julio
Rösner, Kerstin
Stark, Alexander
Steinbrügge, Gregor
Thabaut, Pascal
del Togno, Simone
Touhara, Kazuyuki
Villamil, Sebastian
Wendler, Belinda
Wickhusen, Kai
Willner, Konrad
author Hussmann, Hauke
author_facet Hussmann, Hauke
Lingenauber, Kay
Kallenbach, Reinald
Enya, Keigo
Thomas, Nicolas
Lara, Luisa María
Althaus, Christian L.
Araki, Hiroshi
Behnke, Thomas
Castro Marín, J. M.
Eisenmenger, Henri
Gerber, Thomas
Herranz, Miguel
Hüttig, Christian
Ishibashi, Ko
Jiménez Ortega, Jaime
Kimura, Jun
Kobayashi, Masanori
Lötzke, Horst-Georg
Lichopoj, Alexander
Lüdicke, Fabian
Martínez-Navajas, Ignacio
Michaelis, Harald
Namiki, Noriyuki
Noda, Hirotomo
Oberst, Jürgen
Oshigami, Shoko
Rodríguez García, Juan Pablo
Rodrigo, Julio
Rösner, Kerstin
Stark, Alexander
Steinbrügge, Gregor
Thabaut, Pascal
del Togno, Simone
Touhara, Kazuyuki
Villamil, Sebastian
Wendler, Belinda
Wickhusen, Kai
Willner, Konrad
author_role author
author2 Lingenauber, Kay
Kallenbach, Reinald
Enya, Keigo
Thomas, Nicolas
Lara, Luisa María
Althaus, Christian L.
Araki, Hiroshi
Behnke, Thomas
Castro Marín, J. M.
Eisenmenger, Henri
Gerber, Thomas
Herranz, Miguel
Hüttig, Christian
Ishibashi, Ko
Jiménez Ortega, Jaime
Kimura, Jun
Kobayashi, Masanori
Lötzke, Horst-Georg
Lichopoj, Alexander
Lüdicke, Fabian
Martínez-Navajas, Ignacio
Michaelis, Harald
Namiki, Noriyuki
Noda, Hirotomo
Oberst, Jürgen
Oshigami, Shoko
Rodríguez García, Juan Pablo
Rodrigo, Julio
Rösner, Kerstin
Stark, Alexander
Steinbrügge, Gregor
Thabaut, Pascal
del Togno, Simone
Touhara, Kazuyuki
Villamil, Sebastian
Wendler, Belinda
Wickhusen, Kai
Willner, Konrad
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv German Centre for Air and Space Travel
Ministerio de Economía y Competitividad (España)
European Commission
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Laser Altimetry
Solar System
Satellites of Jupiter
Ganymede
JUICE mission
GALA
topic Laser Altimetry
Solar System
Satellites of Jupiter
Ganymede
JUICE mission
GALA
description The Ganymede Laser Altimeter (GALA) is one of the ten scientific instruments selected for the Jupiter Icy Moons Explorer (JUICE) mission currently implemented under responsibility of the European Space Agency (ESA). JUICE is scheduled for launch in mid 2022; arrival at Jupiter will be by end of 2029 with the nominal science mission—including close flybys at Ganymede, Europa, and Callisto and a Ganymede orbit phase—ending by mid 2033. GALA’s main objective is to obtain topographic data of the icy satellites of Jupiter: Europa, Ganymede, and Callisto. By measuring the diurnal tidal deformation of Ganymede, which crucially depends on the decoupling of the surface ice layer from the deep interior by a liquid water ocean, GALA will obtain evidence for (or against) a subsurface ocean in a 500 km orbit around the satellite and will provide constraints on Ganymede’s ice shell thickness. In combination with other instruments, it will characterize the morphology of surface units on Ganymede, Europa, and Callisto providing not only topography but also surface roughness and albedo (at 1064 nm) measurements. GALA is a single-beam laser altimeter operating with up to 50 Hz (nominal 30 Hz) shot frequency at a wavelength of 1064 nm and pulse lengths of 5.5 ± 2.5 ns using a Nd:YAG laser. The return pulse is detected by an Avalanche Photo Diode (APD) with 100 MHz bandwidth and is digitized at a sampling rate of 200 MHz providing range measurements with a subsample resolution of 0.1 m and surface roughness measurements from pulse-shape analysis on the scale of the footprint size of about 50 m at 500 km altitude. The instrument is developed in collaboration of institutes and industry from Germany, Japan, Switzerland, and Spain. © 2019, CEAS.
publishDate 2019
dc.date.none.fl_str_mv 2019
2020
2020
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Postprint
info:eu-repo/semantics/acceptedVersion
format article
status_str acceptedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/198157
url http://hdl.handle.net/10261/198157
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv #PLACEHOLDER_PARENT_METADATA_VALUE#
info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2016-76076-R
http://dx.doi.org/10.1007/s12567-019-00282-8

dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Springer Nature
publisher.none.fl_str_mv Springer Nature
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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