Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars

Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Platten...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Becker, Gesa Karen [verfasserIn] Knapmeyer-Endrun, Brigitte [akademischer betreuerIn] Christensen, Ulrich [gutachterIn] Gizon, Laurent [gutachterIn]
Hochschulschrift:	Dissertation ; Georg-August-Universität Göttingen ; 2018

Format:	E-Book
Sprache:	Englisch

Erschienen:	Göttingen: 2018

Schlagwörter:	Mars, Planet / Kruste / Reflexionsseismik
Formangabe:	Hochschulschrift

Umfang:	1 Online-Ressource ; Illustrationen, Diagramme

Weitere Ausgabe:	Erscheint auch als Druck-Ausgabe Becker, Gesa Karen: Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars - Göttingen, 2018

Links:	Link aufrufen Volltext Volltext Volltext Volltext

DOI / URN:	urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8

Katalog-ID:	1030406650

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title_full	Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker
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title_sort	crustal thickness from seismic noise correlations in preparation for the insight mission to mars
title_auth	Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars
abstract	Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro...
abstractGer	Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro...
abstract_unstemmed	Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro...
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allfields	18,O10 dnb 1166399753 DE-101 urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 urn (DE-627)1030406650 (DE-599)GBV1030406650 (OCoLC)1057312465 DE-627 ger DE-627 rda eng XA-DE-NI 530 22 550 DE-101 39.53 bkl Becker, Gesa Karen verfasserin aut Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker Göttingen 2018 1 Online-Ressource Illustrationen, Diagramme Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Dissertation Georg-August-Universität Göttingen 2018 Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro... Archivierung/Langzeitarchivierung gewährleistet pdager DE-101 Hochschulschrift (DE-588)4113937-9 (DE-627)105825778 (DE-576)209480580 gnd-content g (DE-588)4037687-4 (DE-627)106235990 (DE-576)209025999 Mars Planet gnd s (DE-588)4165817-6 (DE-627)105437352 (DE-576)209898097 Kruste gnd s (DE-588)4177335-4 (DE-627)104346272 (DE-576)209976926 Reflexionsseismik gnd DE-101 Knapmeyer-Endrun, Brigitte akademischer betreuerin dgs Christensen, Ulrich gutachterin oth Gizon, Laurent gutachterin oth Erscheint auch als Druck-Ausgabe Becker, Gesa Karen Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars Göttingen, 2018 109 Seiten (DE-627)1030406669 http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2018-10-05 Resolving-System Volltext http://d-nb.info/1166399753/34 2018-10-05 Langzeitarchivierung Nationalbibliothek Volltext GBV-ODiss GBV_ILN_20 ISIL_DE-84 SYSFLAG_1 GBV_KXP SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_21 ISIL_DE-46 GBV_ILN_22 ISIL_DE-18 GBV_ILN_23 ISIL_DE-830 GBV_ILN_30 ISIL_DE-104 GBV_ILN_40 ISIL_DE-7 GBV_ILN_60 ISIL_DE-705 GBV_ILN_63 ISIL_DE-Wim2 GBV_ILN_70 ISIL_DE-89 GBV_ILN_105 ISIL_DE-841 GBV_ILN_110 ISIL_DE-Luen4 GBV_ILN_132 ISIL_DE-959 GBV_ILN_151 ISIL_DE-546 GBV_ILN_161 ISIL_DE-960 GBV_ILN_213 ISIL_DE-551 GBV_ILN_293 ISIL_DE-960-3 GBV_ILN_370 ISIL_DE-1373 GBV_ILN_2403 ISIL_DE-LFER 39.53 Planeten (DE-627)106407635 BO 045F 530 20 01 0084 181050550X x 05-10-18 21 01 0046 1810515378 z 05-10-18 22 01 0018 181052542X SUBolrd xu 05-10-18 23 01 0830 1810534445 olr-d x 05-10-18 30 01 0104 1810541611 z 05-10-18 40 01 0007 1802610200 ediss xsn 07-09-18 60 01 0705 1810558514 OLRD z 05-10-18 63 01 3401 1810567459 ORD x 05-10-18 70 01 0089 1810573173 zdt 05-10-18 105 01 0841 1810637430 z 05-10-18 110 01 3110 1810581427 x 05-10-18 132 01 0959 1810591554 OLR-DISS x 05-10-18 151 01 0546 4159404189 OLR-ODISS z 30-06-22 161 01 0960 1810601657 ORD z 05-10-18 213 01 0551 1810611709 ORD x 05-10-18 293 01 3293 1810626412 ORD z 05-10-18 370 01 4370 1810634202 x 05-10-18 2403 01 DE-LFER 3480362737 00 --%%-- --%%-- n --%%-- l01 31-05-19 20 01 0084 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 21 01 0046 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 22 01 0018 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 23 01 0830 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 30 01 0104 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 01 0007 Volltext http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 LF 60 01 0705 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 63 01 3401 E-Book http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 LF 70 01 0089 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 105 01 0841 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 110 01 3110 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 132 01 0959 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 151 01 0546 Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 161 01 0960 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 213 01 0551 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 293 01 3293 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 370 01 4370 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2403 01 DE-LFER http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 00 DE-7 00 (DE-627)623602830 TGG 548 Geologie des Mars {Astronomie} 60 01 0705 10 ho 20 01 0084 OLRD 110 01 3110 OLRD 370 01 4370 OLRD 22 01 0018 SUBolrd 23 01 0830 olr-d 40 01 0007 ediss 60 01 0705 OLRD 63 01 3401 ORD 132 01 0959 OLR-DISS 151 01 0546 OLR-ODISS 161 01 0960 ORD 213 01 0551 ORD 293 01 3293 ORD 23 01 0830 2018-10-05:10:05:51
spelling	18,O10 dnb 1166399753 DE-101 urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 urn (DE-627)1030406650 (DE-599)GBV1030406650 (OCoLC)1057312465 DE-627 ger DE-627 rda eng XA-DE-NI 530 22 550 DE-101 39.53 bkl Becker, Gesa Karen verfasserin aut Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker Göttingen 2018 1 Online-Ressource Illustrationen, Diagramme Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Dissertation Georg-August-Universität Göttingen 2018 Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro... Archivierung/Langzeitarchivierung gewährleistet pdager DE-101 Hochschulschrift (DE-588)4113937-9 (DE-627)105825778 (DE-576)209480580 gnd-content g (DE-588)4037687-4 (DE-627)106235990 (DE-576)209025999 Mars Planet gnd s (DE-588)4165817-6 (DE-627)105437352 (DE-576)209898097 Kruste gnd s (DE-588)4177335-4 (DE-627)104346272 (DE-576)209976926 Reflexionsseismik gnd DE-101 Knapmeyer-Endrun, Brigitte akademischer betreuerin dgs Christensen, Ulrich gutachterin oth Gizon, Laurent gutachterin oth Erscheint auch als Druck-Ausgabe Becker, Gesa Karen Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars Göttingen, 2018 109 Seiten (DE-627)1030406669 http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2018-10-05 Resolving-System Volltext http://d-nb.info/1166399753/34 2018-10-05 Langzeitarchivierung Nationalbibliothek Volltext GBV-ODiss GBV_ILN_20 ISIL_DE-84 SYSFLAG_1 GBV_KXP SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_21 ISIL_DE-46 GBV_ILN_22 ISIL_DE-18 GBV_ILN_23 ISIL_DE-830 GBV_ILN_30 ISIL_DE-104 GBV_ILN_40 ISIL_DE-7 GBV_ILN_60 ISIL_DE-705 GBV_ILN_63 ISIL_DE-Wim2 GBV_ILN_70 ISIL_DE-89 GBV_ILN_105 ISIL_DE-841 GBV_ILN_110 ISIL_DE-Luen4 GBV_ILN_132 ISIL_DE-959 GBV_ILN_151 ISIL_DE-546 GBV_ILN_161 ISIL_DE-960 GBV_ILN_213 ISIL_DE-551 GBV_ILN_293 ISIL_DE-960-3 GBV_ILN_370 ISIL_DE-1373 GBV_ILN_2403 ISIL_DE-LFER 39.53 Planeten (DE-627)106407635 BO 045F 530 20 01 0084 181050550X x 05-10-18 21 01 0046 1810515378 z 05-10-18 22 01 0018 181052542X SUBolrd xu 05-10-18 23 01 0830 1810534445 olr-d x 05-10-18 30 01 0104 1810541611 z 05-10-18 40 01 0007 1802610200 ediss xsn 07-09-18 60 01 0705 1810558514 OLRD z 05-10-18 63 01 3401 1810567459 ORD x 05-10-18 70 01 0089 1810573173 zdt 05-10-18 105 01 0841 1810637430 z 05-10-18 110 01 3110 1810581427 x 05-10-18 132 01 0959 1810591554 OLR-DISS x 05-10-18 151 01 0546 4159404189 OLR-ODISS z 30-06-22 161 01 0960 1810601657 ORD z 05-10-18 213 01 0551 1810611709 ORD x 05-10-18 293 01 3293 1810626412 ORD z 05-10-18 370 01 4370 1810634202 x 05-10-18 2403 01 DE-LFER 3480362737 00 --%%-- --%%-- n --%%-- l01 31-05-19 20 01 0084 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 21 01 0046 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 22 01 0018 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 23 01 0830 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 30 01 0104 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 01 0007 Volltext http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 LF 60 01 0705 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 63 01 3401 E-Book http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 LF 70 01 0089 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 105 01 0841 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 110 01 3110 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 132 01 0959 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 151 01 0546 Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 161 01 0960 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 213 01 0551 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 293 01 3293 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 370 01 4370 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2403 01 DE-LFER http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 00 DE-7 00 (DE-627)623602830 TGG 548 Geologie des Mars {Astronomie} 60 01 0705 10 ho 20 01 0084 OLRD 110 01 3110 OLRD 370 01 4370 OLRD 22 01 0018 SUBolrd 23 01 0830 olr-d 40 01 0007 ediss 60 01 0705 OLRD 63 01 3401 ORD 132 01 0959 OLR-DISS 151 01 0546 OLR-ODISS 161 01 0960 ORD 213 01 0551 ORD 293 01 3293 ORD 23 01 0830 2018-10-05:10:05:51
allfields_unstemmed	18,O10 dnb 1166399753 DE-101 urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 urn (DE-627)1030406650 (DE-599)GBV1030406650 (OCoLC)1057312465 DE-627 ger DE-627 rda eng XA-DE-NI 530 22 550 DE-101 39.53 bkl Becker, Gesa Karen verfasserin aut Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker Göttingen 2018 1 Online-Ressource Illustrationen, Diagramme Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Dissertation Georg-August-Universität Göttingen 2018 Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro... Archivierung/Langzeitarchivierung gewährleistet pdager DE-101 Hochschulschrift (DE-588)4113937-9 (DE-627)105825778 (DE-576)209480580 gnd-content g (DE-588)4037687-4 (DE-627)106235990 (DE-576)209025999 Mars Planet gnd s (DE-588)4165817-6 (DE-627)105437352 (DE-576)209898097 Kruste gnd s (DE-588)4177335-4 (DE-627)104346272 (DE-576)209976926 Reflexionsseismik gnd DE-101 Knapmeyer-Endrun, Brigitte akademischer betreuerin dgs Christensen, Ulrich gutachterin oth Gizon, Laurent gutachterin oth Erscheint auch als Druck-Ausgabe Becker, Gesa Karen Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars Göttingen, 2018 109 Seiten (DE-627)1030406669 http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2018-10-05 Resolving-System Volltext http://d-nb.info/1166399753/34 2018-10-05 Langzeitarchivierung Nationalbibliothek Volltext GBV-ODiss GBV_ILN_20 ISIL_DE-84 SYSFLAG_1 GBV_KXP SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_21 ISIL_DE-46 GBV_ILN_22 ISIL_DE-18 GBV_ILN_23 ISIL_DE-830 GBV_ILN_30 ISIL_DE-104 GBV_ILN_40 ISIL_DE-7 GBV_ILN_60 ISIL_DE-705 GBV_ILN_63 ISIL_DE-Wim2 GBV_ILN_70 ISIL_DE-89 GBV_ILN_105 ISIL_DE-841 GBV_ILN_110 ISIL_DE-Luen4 GBV_ILN_132 ISIL_DE-959 GBV_ILN_151 ISIL_DE-546 GBV_ILN_161 ISIL_DE-960 GBV_ILN_213 ISIL_DE-551 GBV_ILN_293 ISIL_DE-960-3 GBV_ILN_370 ISIL_DE-1373 GBV_ILN_2403 ISIL_DE-LFER 39.53 Planeten (DE-627)106407635 BO 045F 530 20 01 0084 181050550X x 05-10-18 21 01 0046 1810515378 z 05-10-18 22 01 0018 181052542X SUBolrd xu 05-10-18 23 01 0830 1810534445 olr-d x 05-10-18 30 01 0104 1810541611 z 05-10-18 40 01 0007 1802610200 ediss xsn 07-09-18 60 01 0705 1810558514 OLRD z 05-10-18 63 01 3401 1810567459 ORD x 05-10-18 70 01 0089 1810573173 zdt 05-10-18 105 01 0841 1810637430 z 05-10-18 110 01 3110 1810581427 x 05-10-18 132 01 0959 1810591554 OLR-DISS x 05-10-18 151 01 0546 4159404189 OLR-ODISS z 30-06-22 161 01 0960 1810601657 ORD z 05-10-18 213 01 0551 1810611709 ORD x 05-10-18 293 01 3293 1810626412 ORD z 05-10-18 370 01 4370 1810634202 x 05-10-18 2403 01 DE-LFER 3480362737 00 --%%-- --%%-- n --%%-- l01 31-05-19 20 01 0084 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 21 01 0046 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 22 01 0018 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 23 01 0830 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 30 01 0104 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 01 0007 Volltext http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 LF 60 01 0705 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 63 01 3401 E-Book http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 LF 70 01 0089 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 105 01 0841 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 110 01 3110 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 132 01 0959 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 151 01 0546 Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 161 01 0960 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 213 01 0551 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 293 01 3293 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 370 01 4370 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2403 01 DE-LFER http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 00 DE-7 00 (DE-627)623602830 TGG 548 Geologie des Mars {Astronomie} 60 01 0705 10 ho 20 01 0084 OLRD 110 01 3110 OLRD 370 01 4370 OLRD 22 01 0018 SUBolrd 23 01 0830 olr-d 40 01 0007 ediss 60 01 0705 OLRD 63 01 3401 ORD 132 01 0959 OLR-DISS 151 01 0546 OLR-ODISS 161 01 0960 ORD 213 01 0551 ORD 293 01 3293 ORD 23 01 0830 2018-10-05:10:05:51
allfieldsGer	18,O10 dnb 1166399753 DE-101 urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 urn (DE-627)1030406650 (DE-599)GBV1030406650 (OCoLC)1057312465 DE-627 ger DE-627 rda eng XA-DE-NI 530 22 550 DE-101 39.53 bkl Becker, Gesa Karen verfasserin aut Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker Göttingen 2018 1 Online-Ressource Illustrationen, Diagramme Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Dissertation Georg-August-Universität Göttingen 2018 Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro... 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allfieldsSound	18,O10 dnb 1166399753 DE-101 urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 urn (DE-627)1030406650 (DE-599)GBV1030406650 (OCoLC)1057312465 DE-627 ger DE-627 rda eng XA-DE-NI 530 22 550 DE-101 39.53 bkl Becker, Gesa Karen verfasserin aut Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars vorgelegt von Gesa Karen Becker Göttingen 2018 1 Online-Ressource Illustrationen, Diagramme Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Dissertation Georg-August-Universität Göttingen 2018 Die Entstehung terrestrischer Planeten wirft noch viele Fragen auf. Die Untersuchung des Inneren des Planeten Mars mit Hilfe seismischer Wellen kann zur Beantwortung dieser Fragen beitragen. Große Teile der Marskruste sind aus der Frühzeit der Entwicklung des Planeten erhalten, da Mars keine Plattentektonik aufweist. Informationen über die Mächtigkeit und den Aufbau der Kruste können somit zu unserem Verständnis der Entstehung und Entwicklung terrestrischer Planeten beitragen. Die InSight Mission zum Mars wird ein Seismometer auf der Oberfläche des Planeten absetzen. Um die seismischen Date... The formation of terrestrial planets is still poorly understood. Studying the interior of Mars by analysing seismic waves can help to answer questions about that process. In the absence of plate tectonics, Mars has retained much of its crust from early stages of the planet’s evolution. Knowledge of its crustal thickness and structure can therefore contribute to the understanding of terrestrial planet formation and evolution. In preparation for the InSight seismometer installation on Mars, a method is developed to image the reflectivity of the subsurface and extract the crustal thickness fro... Archivierung/Langzeitarchivierung gewährleistet pdager DE-101 Hochschulschrift (DE-588)4113937-9 (DE-627)105825778 (DE-576)209480580 gnd-content g (DE-588)4037687-4 (DE-627)106235990 (DE-576)209025999 Mars Planet gnd s (DE-588)4165817-6 (DE-627)105437352 (DE-576)209898097 Kruste gnd s (DE-588)4177335-4 (DE-627)104346272 (DE-576)209976926 Reflexionsseismik gnd DE-101 Knapmeyer-Endrun, Brigitte akademischer betreuerin dgs Christensen, Ulrich gutachterin oth Gizon, Laurent gutachterin oth Erscheint auch als Druck-Ausgabe Becker, Gesa Karen Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars Göttingen, 2018 109 Seiten (DE-627)1030406669 http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 Resolving-System Volltext kostenfrei Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2018-10-05 Resolving-System Volltext http://d-nb.info/1166399753/34 2018-10-05 Langzeitarchivierung Nationalbibliothek Volltext GBV-ODiss GBV_ILN_20 ISIL_DE-84 SYSFLAG_1 GBV_KXP SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_21 ISIL_DE-46 GBV_ILN_22 ISIL_DE-18 GBV_ILN_23 ISIL_DE-830 GBV_ILN_30 ISIL_DE-104 GBV_ILN_40 ISIL_DE-7 GBV_ILN_60 ISIL_DE-705 GBV_ILN_63 ISIL_DE-Wim2 GBV_ILN_70 ISIL_DE-89 GBV_ILN_105 ISIL_DE-841 GBV_ILN_110 ISIL_DE-Luen4 GBV_ILN_132 ISIL_DE-959 GBV_ILN_151 ISIL_DE-546 GBV_ILN_161 ISIL_DE-960 GBV_ILN_213 ISIL_DE-551 GBV_ILN_293 ISIL_DE-960-3 GBV_ILN_370 ISIL_DE-1373 GBV_ILN_2403 ISIL_DE-LFER 39.53 Planeten (DE-627)106407635 BO 045F 530 20 01 0084 181050550X x 05-10-18 21 01 0046 1810515378 z 05-10-18 22 01 0018 181052542X SUBolrd xu 05-10-18 23 01 0830 1810534445 olr-d x 05-10-18 30 01 0104 1810541611 z 05-10-18 40 01 0007 1802610200 ediss xsn 07-09-18 60 01 0705 1810558514 OLRD z 05-10-18 63 01 3401 1810567459 ORD x 05-10-18 70 01 0089 1810573173 zdt 05-10-18 105 01 0841 1810637430 z 05-10-18 110 01 3110 1810581427 x 05-10-18 132 01 0959 1810591554 OLR-DISS x 05-10-18 151 01 0546 4159404189 OLR-ODISS z 30-06-22 161 01 0960 1810601657 ORD z 05-10-18 213 01 0551 1810611709 ORD x 05-10-18 293 01 3293 1810626412 ORD z 05-10-18 370 01 4370 1810634202 x 05-10-18 2403 01 DE-LFER 3480362737 00 --%%-- --%%-- n --%%-- l01 31-05-19 20 01 0084 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 21 01 0046 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 22 01 0018 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 23 01 0830 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 30 01 0104 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 01 0007 Volltext http://hdl.handle.net/11858/00-1735-0000-002E-E495-4 LF 60 01 0705 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 63 01 3401 E-Book http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 LF 70 01 0089 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 105 01 0841 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 110 01 3110 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 132 01 0959 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 151 01 0546 Volltext http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 161 01 0960 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 213 01 0551 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 293 01 3293 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 370 01 4370 http://nbn-resolving.de/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 2403 01 DE-LFER http://nbn-resolving.org/urn:nbn:de:gbv:7-11858/00-1735-0000-002E-E495-4-8 40 00 DE-7 00 (DE-627)623602830 TGG 548 Geologie des Mars {Astronomie} 60 01 0705 10 ho 20 01 0084 OLRD 110 01 3110 OLRD 370 01 4370 OLRD 22 01 0018 SUBolrd 23 01 0830 olr-d 40 01 0007 ediss 60 01 0705 OLRD 63 01 3401 ORD 132 01 0959 OLR-DISS 151 01 0546 OLR-ODISS 161 01 0960 ORD 213 01 0551 ORD 293 01 3293 ORD 23 01 0830 2018-10-05:10:05:51
language	English
format_phy_str_mv	Book
bklname	Planeten
institution	findex.gbv.de
selectbib_iln_str_mv	20@ 21@ 22@u 23@ 30@ 40@sn 60@ 63@ 70@dt 105@ 110@ 132@ 151@ 161@ 213@ 293@ 370@ 2403@01
dewey-raw	530
authorswithroles_txt_mv	Becker, Gesa Karen @@aut@@ Knapmeyer-Endrun, Brigitte @@dgs@@ Christensen, Ulrich @@oth@@ Gizon, Laurent @@oth@@
genre_facet	Hochschulschrift
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title_short	Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars
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up_date	2024-07-04T10:25:30.902Z
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Crustal thickness from seismic noise correlations in preparation for the InSight mission to Mars

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