Production of Negative Hydrogen Ions Within the MMS Fast Plasma Investigation Due to Solar Wind Bombardment.
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| Title: | Production of Negative Hydrogen Ions Within the MMS Fast Plasma Investigation Due to Solar Wind Bombardment. |
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| Authors: | Gingell, Imogen1 i.gingell@imperial.ac.uk, Schwartz, Steven J.1,2, Gershman, Daniel J.3, Paterson, William R.3, Desai, Ravindra T.1, Giles, Barbara L.3, Pollock, Craig J.3, Avanov, Levon A.3 |
| Source: | Journal of Geophysical Research. Space Physics. Aug2018, Vol. 123 Issue 8, p6161-6170. 10p. |
| Subject Terms: | Solar wind, Space vehicles, Electron spectrometers, Hydrogen ions, Electron temperature |
| Abstract: | The particle data delivered by the Fast Plasma Investigation instrument aboard National Aeronautics and Space Administration's Magnetospheric Multiscale (MMS) mission allow for exceptionally high‐resolution examination of the electron and ion phase space in the near‐Earth plasma environment. It is necessary to identify populations which originate from instrumental effects. Using Fast Plasma Investigation's Dual Electron Spectrometers, we isolate a high‐energy (approximately kiloelectron volt) beam, present while the spacecraft are in the solar wind, which exhibits an azimuthal drift with period associated with the spacecraft spin. We show that this population is consistent with negative hydrogen ions H− generated by a double charge exchange interaction between the incident solar wind H+ ions and the metallic surfaces within the instrument. This interaction is likely to occur at the deflector plates close to the instrument aperture. The H− density is shown to be approximately 0.2–0.4% of the solar wind ion density, and the energy of the negative ion population is shown to be 70% of the incident solar wind energy. These negative ions may introduce errors in electron velocity moments on the order of 0.2–0.4% of the solar wind velocity and significantly higher errors in the electron temperature. Key Points: An anomalous population is observed by MMS's electron plasma instruments in the solar windThe population is consistent with negative ions generated by charge exchange within the instrumentThe errors in the calculation of the electron moments are estimated [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: 132308080 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Production of Negative Hydrogen Ions Within the MMS Fast Plasma Investigation Due to Solar Wind Bombardment. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Gingell%2C+Imogen%22">Gingell, Imogen</searchLink><relatesTo>1</relatesTo><i> i.gingell@imperial.ac.uk</i><br /><searchLink fieldCode="AR" term="%22Schwartz%2C+Steven+J%2E%22">Schwartz, Steven J.</searchLink><relatesTo>1,2</relatesTo><br /><searchLink fieldCode="AR" term="%22Gershman%2C+Daniel+J%2E%22">Gershman, Daniel J.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Paterson%2C+William+R%2E%22">Paterson, William R.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Desai%2C+Ravindra+T%2E%22">Desai, Ravindra T.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Giles%2C+Barbara+L%2E%22">Giles, Barbara L.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Pollock%2C+Craig+J%2E%22">Pollock, Craig J.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Avanov%2C+Levon+A%2E%22">Avanov, Levon A.</searchLink><relatesTo>3</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>. Aug2018, Vol. 123 Issue 8, p6161-6170. 10p. – Name: Subject Label: Subject Terms Group: Su Data: <searchLink fieldCode="DE" term="%22Solar+wind%22">Solar wind</searchLink><br /><searchLink fieldCode="DE" term="%22Space+vehicles%22">Space vehicles</searchLink><br /><searchLink fieldCode="DE" term="%22Electron+spectrometers%22">Electron spectrometers</searchLink><br /><searchLink fieldCode="DE" term="%22Hydrogen+ions%22">Hydrogen ions</searchLink><br /><searchLink fieldCode="DE" term="%22Electron+temperature%22">Electron temperature</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: The particle data delivered by the Fast Plasma Investigation instrument aboard National Aeronautics and Space Administration's Magnetospheric Multiscale (MMS) mission allow for exceptionally high‐resolution examination of the electron and ion phase space in the near‐Earth plasma environment. It is necessary to identify populations which originate from instrumental effects. Using Fast Plasma Investigation's Dual Electron Spectrometers, we isolate a high‐energy (approximately kiloelectron volt) beam, present while the spacecraft are in the solar wind, which exhibits an azimuthal drift with period associated with the spacecraft spin. We show that this population is consistent with negative hydrogen ions H− generated by a double charge exchange interaction between the incident solar wind H+ ions and the metallic surfaces within the instrument. This interaction is likely to occur at the deflector plates close to the instrument aperture. The H− density is shown to be approximately 0.2–0.4% of the solar wind ion density, and the energy of the negative ion population is shown to be 70% of the incident solar wind energy. These negative ions may introduce errors in electron velocity moments on the order of 0.2–0.4% of the solar wind velocity and significantly higher errors in the electron temperature. Key Points: An anomalous population is observed by MMS's electron plasma instruments in the solar windThe population is consistent with negative ions generated by charge exchange within the instrumentThe errors in the calculation of the electron moments are estimated [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: 10.1029/2018JA025341 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 10 StartPage: 6161 Subjects: – SubjectFull: Solar wind Type: general – SubjectFull: Space vehicles Type: general – SubjectFull: Electron spectrometers Type: general – SubjectFull: Hydrogen ions Type: general – SubjectFull: Electron temperature Type: general Titles: – TitleFull: Production of Negative Hydrogen Ions Within the MMS Fast Plasma Investigation Due to Solar Wind Bombardment. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Gingell, Imogen – PersonEntity: Name: NameFull: Schwartz, Steven J. – PersonEntity: Name: NameFull: Gershman, Daniel J. – PersonEntity: Name: NameFull: Paterson, William R. – PersonEntity: Name: NameFull: Desai, Ravindra T. – PersonEntity: Name: NameFull: Giles, Barbara L. – PersonEntity: Name: NameFull: Pollock, Craig J. – PersonEntity: Name: NameFull: Avanov, Levon A. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 08 Text: Aug2018 Type: published Y: 2018 Identifiers: – Type: issn-print Value: 21699380 Numbering: – Type: volume Value: 123 – Type: issue Value: 8 Titles: – TitleFull: Journal of Geophysical Research. Space Physics Type: main |
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