Physically Accurate Large Dynamic Range Pseudo Moments for the MMS Fast Plasma Investigation
| dc.contributor.author | Barrie, A. C. | |
| dc.contributor.author | da Silva, Daniel | |
| dc.contributor.author | Elkington, S. | |
| dc.contributor.author | Sternovsky, Z. | |
| dc.contributor.author | Rager, A. C. | |
| dc.contributor.author | Gershman, D. J. | |
| dc.contributor.author | Paterson, W. R. | |
| dc.contributor.author | Dorelli, J. C. | |
| dc.contributor.author | Giles, B. | |
| dc.date.accessioned | 2024-10-28T14:30:55Z | |
| dc.date.available | 2024-10-28T14:30:55Z | |
| dc.date.issued | 2018-08-02 | |
| dc.description.abstract | The Fast Plasma Investigation onboard the Magnetospheric Multiscale (MMS) mission captures full-sky particle data over a range of 10 eV to 30 keV every 30 ms for electrons and 150 ms for ions. Only about 5% of the count data at this time resolution are sent to the ground due to telemetry limitations; however, a complete set of onboard trigger terms are sent due to their small data volume. These trigger terms are composed of simplified integrals that scale proportionally to plasma moments. They were initially conceived as a mechanism to rank scientific data for priority downlink; however, they can be adapted to represent pseudo moment quantities that are accurate to within several percent of fully corrected plasma moments. Tuning the dynamic range per plasma region and correcting via a trained neural network allow for far greater accuracy than previous missions. Corrections are performed based on statistical sampling of data from the first MMS day side pass. The corrections are validated by comparing pseudo moments to a published event showcasing detection of kinetic Alfvén waves. Physically accurate pseudo plasma moment quantities are available for the entirety of the MMS prime science regions, and can be a valuable asset for future scientific analysis of the MMS data repository. | |
| dc.description.sponsorship | This work was funded by NASA and theMMS mission. All source data areavailable from the MMS ScienceData Center. | |
| dc.description.uri | https://onlinelibrary.wiley.com/doi/abs/10.1029/2018EA000407 | |
| dc.format.extent | 13 pages | |
| dc.genre | journal articles | |
| dc.identifier | doi:10.13016/m29x8h-kyve | |
| dc.identifier.citation | Barrie, A. C., D. da Silva, S. Elkington, Z. Sternovsky, A. C. Rager, D. J. Gershman, W. R. Paterson, J. C. Dorelli, and B. Giles. “Physically Accurate Large Dynamic Range Pseudo Moments for the MMS Fast Plasma Investigation.” Earth and Space Science 5, no. 9 (2018): 503–15. https://doi.org/10.1029/2018EA000407. | |
| dc.identifier.uri | https://doi.org/10.1029/2018EA000407 | |
| dc.identifier.uri | http://hdl.handle.net/11603/36784 | |
| dc.language.iso | en_US | |
| dc.publisher | AGU | |
| dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
| dc.relation.ispartof | UMBC Goddard Planetary Heliophysics Institute (GPHI) | |
| dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
| dc.rights | Public Domain | |
| dc.rights.uri | https://creativecommons.org/publicdomain/mark/1.0/ | |
| dc.subject | data correction | |
| dc.subject | onboard moments | |
| dc.subject | plasma | |
| dc.subject | FPI | |
| dc.subject | MMS | |
| dc.subject | neural network | |
| dc.title | Physically Accurate Large Dynamic Range Pseudo Moments for the MMS Fast Plasma Investigation | |
| dc.type | Text | |
| dcterms.creator | https://orcid.org/0000-0001-7537-3539 |
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