Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission

dc.contributor.authorGershman, Daniel J.
dc.contributor.authorDorelli, John C.
dc.contributor.authorAvanov, Levon A.
dc.contributor.authorGliese, Ulrik
dc.contributor.authorBarrie, Alexander
dc.contributor.authorSchiff, Conrad
dc.contributor.authorda Silva, Daniel
dc.contributor.authorPaterson, William R.
dc.contributor.authorGiles, Barbara L.
dc.contributor.authorPollock, Craig J.
dc.date.accessioned2024-10-28T14:30:54Z
dc.date.available2024-10-28T14:30:54Z
dc.date.issued2019-11-23
dc.description.abstractSystematic uncertainties in the conversion of measured counts to phase space density by charged particle instrumentation result in errors in reported plasma moments (e.g., density, velocity, and temperature). Unlike previous particle instrumentation that relied on a spacecraft spin to sample all look-directions, the Fast Plasma Investigation (FPI) suite on NASA's Magnetospheric Multiscale mission nearly simultaneously images the full sky. This configuration results in unprecedented time resolution but also introduces the possibility of spin tones in plasma moments, in particular electron bulk velocity. Here we characterize the effect of systematic linear errors of corrected FPI phase space densities on its reported plasma moments. We find that the flat-fielding correction factors (i.e., scale factor errors) of FPI are typically accurate to within a few percent but can nonetheless result in significant spin tones in magnetospheric plasmas.
dc.description.sponsorshipThis research was supported by theNASA Magnetospheric MultiscaleMission in association with NASAcontract NNG04EB99C. IRAPcontributions to MMS FPI weresupported by CNES and CNRS. Wethank the entire MMS team andinstrument leads for data access andsupport. The data presented in thispaper are the L2 data of MMS and canbe accessed from MMS Science DataCenter.
dc.description.urihttps://onlinelibrary.wiley.com/doi/abs/10.1029/2019JA026980
dc.format.extent15 pages
dc.genrejournal articles
dc.identifierdoi:10.13016/m2qkzb-rsjo
dc.identifier.citationGershman, Daniel J., John C. Dorelli, Levon A. Avanov, Ulrik Gliese, Alexander Barrie, Conrad Schiff, Daniel E. Da Silva, William R. Paterson, Barbara L. Giles, and Craig J. Pollock. “Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA’s Magnetospheric Multiscale Mission.” Journal of Geophysical Research: Space Physics 124, no. 12 (2019): 10345–59. https://doi.org/10.1029/2019JA026980.
dc.identifier.urihttps://doi.org/10.1029/2019JA026980
dc.identifier.urihttp://hdl.handle.net/11603/36781
dc.language.isoen_US
dc.publisherAGU
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis 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.rightsPublic Domain
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.subjectphase space density
dc.subjectpenetrating radiation
dc.subjectplasma moment
dc.subjectspin tone
dc.subjectflat-fielding
dc.subjectparticle instrument
dc.titleSystematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-7537-3539

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