The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations
Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and...
Ausführliche Beschreibung
Autor*in: |
Pla-Garcia, Jorge [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2016 |
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Rechteinformationen: |
Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. |
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Schlagwörter: |
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Übergeordnetes Werk: |
Enthalten in: Icarus - Amsterdam [u.a.] : Elsevier, 1962, 280(2016), Seite 103-113 |
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volume:280 ; year:2016 ; pages:103-113 |
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DOI / URN: |
10.1016/j.icarus.2016.03.013 |
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10.1016/j.icarus.2016.03.013 doi PQ20170501 (DE-627)OLC1986946185 (DE-599)GBVOLC1986946185 (PRQ)c1867-7b9fa56b8cc10c7447aa6a0e9b785f619122fecb117266a23742fb86ace071900 (KEY)0009293220160000280000000103meteorologyofgalecraterasdeterminedfromroverenviro DE-627 ger DE-627 rakwb eng 520 530 DNB Pla-Garcia, Jorge verfasserin aut The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. Environmental monitoring Comparative analysis Mars (Planet) Research institutes Models Rafkin, Scot C.R oth Kahre, Melinda oth Gomez-Elvira, Javier oth Hamilton, Victoria E oth Navarro, Sara oth Torres, Josefina oth Marín, Mercedes oth R. Vasavada, Ashwin oth Enthalten in Icarus Amsterdam [u.a.] : Elsevier, 1962 280(2016), Seite 103-113 (DE-627)129321966 (DE-600)131023-9 (DE-576)014554259 0019-1035 nnns volume:280 year:2016 pages:103-113 http://dx.doi.org/10.1016/j.icarus.2016.03.013 Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_2279 GBV_ILN_2286 AR 280 2016 103-113 |
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10.1016/j.icarus.2016.03.013 doi PQ20170501 (DE-627)OLC1986946185 (DE-599)GBVOLC1986946185 (PRQ)c1867-7b9fa56b8cc10c7447aa6a0e9b785f619122fecb117266a23742fb86ace071900 (KEY)0009293220160000280000000103meteorologyofgalecraterasdeterminedfromroverenviro DE-627 ger DE-627 rakwb eng 520 530 DNB Pla-Garcia, Jorge verfasserin aut The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. Environmental monitoring Comparative analysis Mars (Planet) Research institutes Models Rafkin, Scot C.R oth Kahre, Melinda oth Gomez-Elvira, Javier oth Hamilton, Victoria E oth Navarro, Sara oth Torres, Josefina oth Marín, Mercedes oth R. Vasavada, Ashwin oth Enthalten in Icarus Amsterdam [u.a.] : Elsevier, 1962 280(2016), Seite 103-113 (DE-627)129321966 (DE-600)131023-9 (DE-576)014554259 0019-1035 nnns volume:280 year:2016 pages:103-113 http://dx.doi.org/10.1016/j.icarus.2016.03.013 Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_2279 GBV_ILN_2286 AR 280 2016 103-113 |
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10.1016/j.icarus.2016.03.013 doi PQ20170501 (DE-627)OLC1986946185 (DE-599)GBVOLC1986946185 (PRQ)c1867-7b9fa56b8cc10c7447aa6a0e9b785f619122fecb117266a23742fb86ace071900 (KEY)0009293220160000280000000103meteorologyofgalecraterasdeterminedfromroverenviro DE-627 ger DE-627 rakwb eng 520 530 DNB Pla-Garcia, Jorge verfasserin aut The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. Environmental monitoring Comparative analysis Mars (Planet) Research institutes Models Rafkin, Scot C.R oth Kahre, Melinda oth Gomez-Elvira, Javier oth Hamilton, Victoria E oth Navarro, Sara oth Torres, Josefina oth Marín, Mercedes oth R. Vasavada, Ashwin oth Enthalten in Icarus Amsterdam [u.a.] : Elsevier, 1962 280(2016), Seite 103-113 (DE-627)129321966 (DE-600)131023-9 (DE-576)014554259 0019-1035 nnns volume:280 year:2016 pages:103-113 http://dx.doi.org/10.1016/j.icarus.2016.03.013 Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_2279 GBV_ILN_2286 AR 280 2016 103-113 |
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10.1016/j.icarus.2016.03.013 doi PQ20170501 (DE-627)OLC1986946185 (DE-599)GBVOLC1986946185 (PRQ)c1867-7b9fa56b8cc10c7447aa6a0e9b785f619122fecb117266a23742fb86ace071900 (KEY)0009293220160000280000000103meteorologyofgalecraterasdeterminedfromroverenviro DE-627 ger DE-627 rakwb eng 520 530 DNB Pla-Garcia, Jorge verfasserin aut The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. Nutzungsrecht: © COPYRIGHT 2016 Elsevier B.V. Environmental monitoring Comparative analysis Mars (Planet) Research institutes Models Rafkin, Scot C.R oth Kahre, Melinda oth Gomez-Elvira, Javier oth Hamilton, Victoria E oth Navarro, Sara oth Torres, Josefina oth Marín, Mercedes oth R. Vasavada, Ashwin oth Enthalten in Icarus Amsterdam [u.a.] : Elsevier, 1962 280(2016), Seite 103-113 (DE-627)129321966 (DE-600)131023-9 (DE-576)014554259 0019-1035 nnns volume:280 year:2016 pages:103-113 http://dx.doi.org/10.1016/j.icarus.2016.03.013 Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 GBV_ILN_70 GBV_ILN_2012 GBV_ILN_2279 GBV_ILN_2286 AR 280 2016 103-113 |
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The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations |
abstract |
Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. |
abstractGer |
Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. |
abstract_unstemmed |
Simulations of the meteorology of Gale crater with the Mars regional atmospheric modeling system compare favorably to the data recorded by the rover environmental monitoring station aboard the Mars Science Laboratory Curiosity Rover. * Simulations are conducted for periods covering Ls 0, 90, 180 and 270. * The model may be used to provide context for the observations and to elucidate the physics behind the variations of the observed meteorological parameters. |
collection_details |
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title_short |
The meteorology of Gale crater as determined from rover environmental monitoring station observations and numerical modeling. Part I: Comparison of model simulations with observations |
url |
http://dx.doi.org/10.1016/j.icarus.2016.03.013 |
remote_bool |
false |
author2 |
Rafkin, Scot C.R Kahre, Melinda Gomez-Elvira, Javier Hamilton, Victoria E Navarro, Sara Torres, Josefina Marín, Mercedes R. Vasavada, Ashwin |
author2Str |
Rafkin, Scot C.R Kahre, Melinda Gomez-Elvira, Javier Hamilton, Victoria E Navarro, Sara Torres, Josefina Marín, Mercedes R. Vasavada, Ashwin |
ppnlink |
129321966 |
mediatype_str_mv |
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hochschulschrift_bool |
false |
author2_role |
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doi_str |
10.1016/j.icarus.2016.03.013 |
up_date |
2024-07-04T05:23:24.630Z |
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1803624754314215424 |
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