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Dataset Persistent ID
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doi:10.18715/IPGP.2024.lri0fn8r |
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Publication Date
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2024-01-18 |
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Title
| Swarm Bravo ASM-V data version 050X |
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Author
| Hulot, Gauthier (Université Paris Cité, Institut de physique du globe de Paris, CNRS, France) - ORCID: 0000-0001-8011-3096
Chauvet, Louis (Institut de Physique du Globe de Paris) - ORCID: 0000-0002-1467-9136
Vigneron, Pierre (Université Paris Cité, Institut de physique du globe de Paris, CNRS, France) |
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Contact
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Use email button above to contact.
Hulot, Gauthier (Université Paris Cité, Institut de physique du globe de Paris, CNRS, France) |
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Description
| This dataset consists of version 050X 1 Hz (bandwidth 0-0.4 Hz) self-calibrated experimental vector data acquired by the ASM magnetometer on board satellite Bravo of the ESA Swarm mission. These data are produced by IPGP when the ASM instrument is set in its “vector mode”, which is the mode in which this instrument has been operated for the most part of the mission, except at times (typically during one week sessions) when the instruments are set in their alternative "scalar burst mode". The dataset is organized in annual zipped folders (one per year since 2013), each folder containing all available daily files for the year of interest. The dataset also comes with a SW-ASMV-DD-IPGP-0007_ASMV_Experimental_L1B_Product_Definition Revision 1 file, providing details of the data definition and format of the daily files. |
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Subject
| Astronomy and Astrophysics; Earth and Environmental Sciences; Physics |
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Keyword
| Magnetometry
Scientific Satellites
Geomagnetism |
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Topic Classification
| Geomagnetism |
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Related Publication
| Vigneron, P., Hulot, G., Léger, J.M., Jager, T., Using improved Swarm’s experimental absolute vector mode data to produce a candidate Definitive Geomagnetic Reference Field (DGRF) 2015.0 model, Earth Planets and Space, 73 : 197, 2021. doi: 10.1186/s40623-021-01529-7 https://doi.org/10.1186/s40623-021-01529-7 |
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Notes
| If you use these data, please read the 00_README file and make sure to give proper credit, as invited, by citing both this dataset and the above Vigneron et al (2021) related publication, as well as acknowledging that "The ASM instrument was developed by CEA-Léti and provided by CNES to ESA as a Customer Furnished Instrument". |
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Language
| English |
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Producer
| Hulot, Gauthier (Space Magnetism Project, IPGP) (Université Paris Cité, Institut de physique du globe de Paris, CNRS, France) |
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Production Place
| Institut de physique du globe de Paris |
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Contributor
| Project Leader : Hulot, Gauthier
Project Member : Chauvet, Louis
Project Member : Bonnot, Olivier |
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Grant Information
| CNES: This work was supported by CNES, focused on ASM magnetometers of the Swarm mission |
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Distributor
| Space Magnetism Project, IPGP (Université Paris Cité, Institut de physique du globe de Paris, CNRS, France) |
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Depositor
| Chauvet, Louis |
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Deposit Date
| 2024-01-17 |
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Time Period Covered
| Start: 2013-11-27 ; End: 2022-09-23 |
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Date of Collection
| Start: 2013-11-27 ; End: 2022-09-23 |
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Kind of Data
| Satellite calibrated vector magnetic data acquired at 1 Hz rate (bandwidth 0-0.4 Hz) |
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Software
| driver_asmv_production.m with (MATLAB 9.7.0.1190202 (R2019b)), Version: 8
L1A ASM, Version: 7 |
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Related Datasets
| These data are constructed and provided in a format that allows direct use and comparison with versions 050X of the official ESA Swarm MAGx_LR 1B data available at https://swarm-diss.eo.esa.int/#swarm/Level1b. |
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Other References
| More details about how this ASM vector mode operates and is being calibrated can be found in Gravrand et al. (2001, https://doi.org/10.1186/BF03351692), Léger et al. (2015, https://doi.org/10.1186/s40623-015-0231-1), Fratter et al. (2016, https://doi.org/10.1016/j.actaastro.2015.12.025) and references therein. |
