Wakefield acceleration in planetary atmospheres: A possible source of MeV electrons. The collisionless case.
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| Title: | Wakefield acceleration in planetary atmospheres: A possible source of MeV electrons. The collisionless case. |
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| Authors: | Arrayás, M.1 manuel.arrayas@urjc.es, Cubero, D.2, Montanya, J.3, Seviour, R.4, Trueba, J.L.1 |
| Source: | Journal of Atmospheric & Solar-Terrestrial Physics. Jul2018, Vol. 172, p69-74. 6p. |
| Subjects: | Electromagnetic pulses, Plasma oscillations, Plasma gases, Electromagnetic waves, Electronic excitation |
| Abstract: | Intense electromagnetic pulses interacting with a plasma can create a wake of plasma oscillations. Electrons trapped in such oscillations can be accelerated under certain conditions to very high energies. We study the optimal conditions for the wakefield acceleration to produce MeV electrons in planetary plasmas under collisionless conditions. The conditions for the optimal plasma densities can be found in the Earth atmosphere at higher altitudes than 10–15 km, which are the altitudes where lightning leaders can take place. [ABSTRACT FROM AUTHOR] |
| Copyright of Journal of Atmospheric & Solar-Terrestrial Physics is the property of Pergamon Press - An Imprint of Elsevier Science 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: | Engineering Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: egs DbLabel: Engineering Source An: 129231571 AccessLevel: 6 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| Items | – Name: Title Label: Title Group: Ti Data: Wakefield acceleration in planetary atmospheres: A possible source of MeV electrons. The collisionless case. – Name: Author Label: Authors Group: Au Data: <searchLink fieldCode="AR" term="%22Arrayás%2C+M%2E%22">Arrayás, M.</searchLink><relatesTo>1</relatesTo><i> manuel.arrayas@urjc.es</i><br /><searchLink fieldCode="AR" term="%22Cubero%2C+D%2E%22">Cubero, D.</searchLink><relatesTo>2</relatesTo><br /><searchLink fieldCode="AR" term="%22Montanya%2C+J%2E%22">Montanya, J.</searchLink><relatesTo>3</relatesTo><br /><searchLink fieldCode="AR" term="%22Seviour%2C+R%2E%22">Seviour, R.</searchLink><relatesTo>4</relatesTo><br /><searchLink fieldCode="AR" term="%22Trueba%2C+J%2EL%2E%22">Trueba, J.L.</searchLink><relatesTo>1</relatesTo> – Name: TitleSource Label: Source Group: Src Data: <searchLink fieldCode="JN" term="%22Journal+of+Atmospheric+%26+Solar-Terrestrial+Physics%22">Journal of Atmospheric & Solar-Terrestrial Physics</searchLink>. Jul2018, Vol. 172, p69-74. 6p. – Name: Subject Label: Subjects Group: Su Data: <searchLink fieldCode="DE" term="%22Electromagnetic+pulses%22">Electromagnetic pulses</searchLink><br /><searchLink fieldCode="DE" term="%22Plasma+oscillations%22">Plasma oscillations</searchLink><br /><searchLink fieldCode="DE" term="%22Plasma+gases%22">Plasma gases</searchLink><br /><searchLink fieldCode="DE" term="%22Electromagnetic+waves%22">Electromagnetic waves</searchLink><br /><searchLink fieldCode="DE" term="%22Electronic+excitation%22">Electronic excitation</searchLink> – Name: Abstract Label: Abstract Group: Ab Data: Intense electromagnetic pulses interacting with a plasma can create a wake of plasma oscillations. Electrons trapped in such oscillations can be accelerated under certain conditions to very high energies. We study the optimal conditions for the wakefield acceleration to produce MeV electrons in planetary plasmas under collisionless conditions. The conditions for the optimal plasma densities can be found in the Earth atmosphere at higher altitudes than 10–15 km, which are the altitudes where lightning leaders can take place. [ABSTRACT FROM AUTHOR] – Name: AbstractSuppliedCopyright Label: Group: Ab Data: <i>Copyright of Journal of Atmospheric & Solar-Terrestrial Physics is the property of Pergamon Press - An Imprint of Elsevier Science 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: 10.1016/j.jastp.2018.03.019 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 6 StartPage: 69 Subjects: – SubjectFull: Electromagnetic pulses Type: general – SubjectFull: Plasma oscillations Type: general – SubjectFull: Plasma gases Type: general – SubjectFull: Electromagnetic waves Type: general – SubjectFull: Electronic excitation Type: general Titles: – TitleFull: Wakefield acceleration in planetary atmospheres: A possible source of MeV electrons. The collisionless case. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Arrayás, M. – PersonEntity: Name: NameFull: Cubero, D. – PersonEntity: Name: NameFull: Montanya, J. – PersonEntity: Name: NameFull: Seviour, R. – PersonEntity: Name: NameFull: Trueba, J.L. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 07 Text: Jul2018 Type: published Y: 2018 Identifiers: – Type: issn-print Value: 13646826 Numbering: – Type: volume Value: 172 Titles: – TitleFull: Journal of Atmospheric & Solar-Terrestrial Physics Type: main |
| ResultId | 1 |
