Observation based climatology Martian atmospheric waves perturbation Datasets
Abstract The Martian atmospheric waves perturbation Datasets (MAWPD) version 2.0 is the first observation-based climatology dataset of Martian atmospheric waves. It contains climatology-gridded temperature, gravity waves, and tides spanning the whole Martian year. MAWPD uses the Data INterpolating E...
| Main Authors: | , , , , , , , , |
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| Format: | Article |
| Language: | English |
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Nature Portfolio
2023-01-01
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| Series: | Scientific Data |
| Online Access: | https://doi.org/10.1038/s41597-022-01909-y |
| _version_ | 1797958815227838464 |
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| author | Jie Zhang Qianqian Ji Zheng Sheng Mingyuan He Yang He Xinjie Zuo Zefeng He Zilin Qin Gangyao Wu |
| author_facet | Jie Zhang Qianqian Ji Zheng Sheng Mingyuan He Yang He Xinjie Zuo Zefeng He Zilin Qin Gangyao Wu |
| author_sort | Jie Zhang |
| collection | DOAJ |
| description | Abstract The Martian atmospheric waves perturbation Datasets (MAWPD) version 2.0 is the first observation-based climatology dataset of Martian atmospheric waves. It contains climatology-gridded temperature, gravity waves, and tides spanning the whole Martian year. MAWPD uses the Data INterpolating Empirical Orthogonal Functions method (DINEOF) reconstruction method for data assimilation with the observational data from the Mars Global Surveyor (MGS), Mars Reconnaissance Orbiter (MRO), Mars Atmosphere and Volatile EvolutioN (MAVEN), Mars Pathfinder (MP), Mars Phoenix Lander (MPL), Mars Exploration Rover (MER) and Mars Express (MEX) temperature retrievals. The dataset includes gridded fields of temperature (Level 1 data) as well as the physical quantities of GWs (Level 2 data, amplitude, and potential energies), SPWs and tides (Level 2 data, amplitude, and phase). The MAWPD, based entirely on multiple reliable observations, provides climatological background atmospheric information of temperature and wave disturbances on Mars. The dataset is not only useful for observation-based scientific studies concerning Martian atmospheric waves, e.g., circulation, dust storms, and wave excitation mechanism, but also for cross-validating with model-based datasets or model results. |
| first_indexed | 2024-04-11T00:25:13Z |
| format | Article |
| id | doaj.art-85d666d4f1834815a098b710d77f57e4 |
| institution | Directory Open Access Journal |
| issn | 2052-4463 |
| language | English |
| last_indexed | 2024-04-11T00:25:13Z |
| publishDate | 2023-01-01 |
| publisher | Nature Portfolio |
| record_format | Article |
| series | Scientific Data |
| spelling | doaj.art-85d666d4f1834815a098b710d77f57e42023-01-08T12:04:26ZengNature PortfolioScientific Data2052-44632023-01-0110111310.1038/s41597-022-01909-yObservation based climatology Martian atmospheric waves perturbation DatasetsJie Zhang0Qianqian Ji1Zheng Sheng2Mingyuan He3Yang He4Xinjie Zuo5Zefeng He6Zilin Qin7Gangyao Wu8College of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyHigh-tech InstituteCollege of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyCollege of Meteorology and Oceanography, National University of Defense TechnologyAbstract The Martian atmospheric waves perturbation Datasets (MAWPD) version 2.0 is the first observation-based climatology dataset of Martian atmospheric waves. It contains climatology-gridded temperature, gravity waves, and tides spanning the whole Martian year. MAWPD uses the Data INterpolating Empirical Orthogonal Functions method (DINEOF) reconstruction method for data assimilation with the observational data from the Mars Global Surveyor (MGS), Mars Reconnaissance Orbiter (MRO), Mars Atmosphere and Volatile EvolutioN (MAVEN), Mars Pathfinder (MP), Mars Phoenix Lander (MPL), Mars Exploration Rover (MER) and Mars Express (MEX) temperature retrievals. The dataset includes gridded fields of temperature (Level 1 data) as well as the physical quantities of GWs (Level 2 data, amplitude, and potential energies), SPWs and tides (Level 2 data, amplitude, and phase). The MAWPD, based entirely on multiple reliable observations, provides climatological background atmospheric information of temperature and wave disturbances on Mars. The dataset is not only useful for observation-based scientific studies concerning Martian atmospheric waves, e.g., circulation, dust storms, and wave excitation mechanism, but also for cross-validating with model-based datasets or model results.https://doi.org/10.1038/s41597-022-01909-y |
| spellingShingle | Jie Zhang Qianqian Ji Zheng Sheng Mingyuan He Yang He Xinjie Zuo Zefeng He Zilin Qin Gangyao Wu Observation based climatology Martian atmospheric waves perturbation Datasets Scientific Data |
| title | Observation based climatology Martian atmospheric waves perturbation Datasets |
| title_full | Observation based climatology Martian atmospheric waves perturbation Datasets |
| title_fullStr | Observation based climatology Martian atmospheric waves perturbation Datasets |
| title_full_unstemmed | Observation based climatology Martian atmospheric waves perturbation Datasets |
| title_short | Observation based climatology Martian atmospheric waves perturbation Datasets |
| title_sort | observation based climatology martian atmospheric waves perturbation datasets |
| url | https://doi.org/10.1038/s41597-022-01909-y |
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