Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission.
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| Title: | Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission. |
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| Authors: | Gershman, Daniel J.1 daniel.j.gershman@nasa.gov, Dorelli, John C.1, Avanov, Levon A.1,2, Gliese, Ulrik1,3, Barrie, Alexander1,4, Schiff, Conrad1, Da Silva, Daniel E.1,5, Paterson, William R.1, Giles, Barbara L.1, Pollock, Craig J.6 |
| Source: | Journal of Geophysical Research. Space Physics. Dec2019, Vol. 124 Issue 12, p10345-10359. 15p. |
| Subject Terms: | Magnetosphere, Charged particle accelerators, Phase space, High-density plasmas |
| Company/Entity: | United States. National Aeronautics & Space Administration |
| Abstract: | Systematic 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. Key Points: The flat‐field correction factors for the Fast Plasma Investigation suite on MMS are typically accurate to within a few percentBackground errors can be corrected for at the moment level if appropriate models are availableImperfect flat‐field correction factors result in systematic biases in plasma moments [ABSTRACT FROM AUTHOR] |
| Copyright of Journal of Geophysical Research. Space Physics is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.) | |
| Database: | GreenFILE |
| FullText | Text: Availability: 0 |
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| Header | DbId: 8gh DbLabel: GreenFILE An: 141383321 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Gershman%2C+Daniel+J%2E%22">Gershman, Daniel J.</searchLink><relatesTo>1</relatesTo><i> daniel.j.gershman@nasa.gov</i><br /><searchLink fieldCode="AR" term="%22Dorelli%2C+John+C%2E%22">Dorelli, John C.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Avanov%2C+Levon+A%2E%22">Avanov, Levon A.</searchLink><relatesTo>1,2</relatesTo><br /><searchLink fieldCode="AR" term="%22Gliese%2C+Ulrik%22">Gliese, Ulrik</searchLink><relatesTo>1,3</relatesTo><br /><searchLink fieldCode="AR" term="%22Barrie%2C+Alexander%22">Barrie, Alexander</searchLink><relatesTo>1,4</relatesTo><br /><searchLink fieldCode="AR" term="%22Schiff%2C+Conrad%22">Schiff, Conrad</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Da+Silva%2C+Daniel+E%2E%22">Da Silva, Daniel E.</searchLink><relatesTo>1,5</relatesTo><br /><searchLink fieldCode="AR" term="%22Paterson%2C+William+R%2E%22">Paterson, William R.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Giles%2C+Barbara+L%2E%22">Giles, Barbara L.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Pollock%2C+Craig+J%2E%22">Pollock, Craig J.</searchLink><relatesTo>6</relatesTo> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Journal+of+Geophysical+Research%2E+Space+Physics%22">Journal of Geophysical Research. Space Physics</searchLink>. Dec2019, Vol. 124 Issue 12, p10345-10359. 15p. – Name: Subject Label: Subject Terms Group: Su Data: <searchLink fieldCode="DE" term="%22Magnetosphere%22">Magnetosphere</searchLink><br /><searchLink fieldCode="DE" term="%22Charged+particle+accelerators%22">Charged particle accelerators</searchLink><br /><searchLink fieldCode="DE" term="%22Phase+space%22">Phase space</searchLink><br /><searchLink fieldCode="DE" term="%22High-density+plasmas%22">High-density plasmas</searchLink> – Name: SubjectCompany Label: Company/Entity Group: Su Data: <searchLink fieldCode="DE" term="%22United+States%2E+National+Aeronautics+%26+Space+Administration%22">United States. National Aeronautics & Space Administration</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Systematic 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. Key Points: The flat‐field correction factors for the Fast Plasma Investigation suite on MMS are typically accurate to within a few percentBackground errors can be corrected for at the moment level if appropriate models are availableImperfect flat‐field correction factors result in systematic biases in plasma moments [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Journal of Geophysical Research. Space Physics is the property of Wiley-Blackwell and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.) |
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| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1029/2019JA026980 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 15 StartPage: 10345 Subjects: – SubjectFull: Magnetosphere Type: general – SubjectFull: Charged particle accelerators Type: general – SubjectFull: Phase space Type: general – SubjectFull: High-density plasmas Type: general – SubjectFull: United States. National Aeronautics & Space Administration Type: general Titles: – TitleFull: Systematic Uncertainties in Plasma Parameters Reported by the Fast Plasma Investigation on NASA's Magnetospheric Multiscale Mission. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Gershman, Daniel J. – PersonEntity: Name: NameFull: Dorelli, John C. – PersonEntity: Name: NameFull: Avanov, Levon A. – PersonEntity: Name: NameFull: Gliese, Ulrik – PersonEntity: Name: NameFull: Barrie, Alexander – PersonEntity: Name: NameFull: Schiff, Conrad – PersonEntity: Name: NameFull: Da Silva, Daniel E. – PersonEntity: Name: NameFull: Paterson, William R. – PersonEntity: Name: NameFull: Giles, Barbara L. – PersonEntity: Name: NameFull: Pollock, Craig J. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 12 Text: Dec2019 Type: published Y: 2019 Identifiers: – Type: issn-print Value: 21699380 Numbering: – Type: volume Value: 124 – Type: issue Value: 12 Titles: – TitleFull: Journal of Geophysical Research. Space Physics Type: main |
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