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  Large‐Scale Survey of the Structure of the Dayside Magnetopause by MMS

Paschmann, G., Haaland, S., Phan, T. D., Sonnerup, B. U. Ö., Burch, J. L., Torbert, R. B., Gershman, D. J., Dorelli, J. C., Giles, B. L., Pollock, C., Saito, Y., Lavraud, B., Russell, C. T., Strangeway, R. J., Baumjohann, W., & Fuselier, S. A. (2018). Large‐Scale Survey of the Structure of the Dayside Magnetopause by MMS. Journal of Geophysical Research: Space Physics, 123(3), 2018-2033. doi:10.1002/2017JA025121.

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アイテムのパーマリンク: https://hdl.handle.net/21.11116/0000-0001-1DBF-9 版のパーマリンク: https://hdl.handle.net/21.11116/0000-0003-CA71-A
資料種別: 学術論文

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 作成者:
Paschmann, G., 著者
Haaland, Stein1, 著者           
Phan, T. D., 著者
Sonnerup, B. U. Ö., 著者
Burch, J. L., 著者
Torbert, R. B., 著者
Gershman, D. J., 著者
Dorelli, J. C., 著者
Giles, B. L., 著者
Pollock, C., 著者
Saito, Y., 著者
Lavraud, B., 著者
Russell, C. T., 著者
Strangeway, R. J., 著者
Baumjohann, W., 著者
Fuselier, S. A., 著者
所属:
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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キーワード: -
 MPIS_PROJECTS: Cluster
 MPIS_GROUPS: Planetary Plasmas
 要旨: This paper describes the generation and initial utilization of a database containing 80 vector and scalar quantities, for a total of 8,670 magnetopause and magnetosheath current sheet crossings by MMS1, using plasma and magnetic field data from the Fast Plasma Investigation, Fluxgate Magnetometer, and Hot Plasma Composition Analyzer instruments, augmented by solar wind and interplanetary magnetic field data from CDAWeb. Based on a determination of the current sheet width, measured and calculated vector and scalar quantities are stored for the two sides of the current sheet and for selected times within the current sheet. The only manual operations were the classification of the current sheets according to the type of boundary, the character of the magnetic field transition, and the quality of the current sheet fit. To characterize the database, histograms of selected key quantities are presented. We then give the statistics for the duration, motion, and thicknesses of the magnetopause current sheet, using single‐spacecraft techniques for the determination of the normal velocities, obtaining median results of 12.9 s, 38.5 km/s, and 705.4 km, respectively. When scaled to the ion inertial length, the median thickness became 12.6; there were no thicknesses less than one. Next, we apply the Walén relation to find crossings that are rotational discontinuities and thus may indicate ongoing magnetic reconnection. For crossings where the velocities in the outflow region exceed the velocity on the magnetosheath side by at least 250 km/s, 47% meet our rotational discontinuity criteria. If we require the outflow to exceed 250 km/s along the L direction, then the percentage rises to 68%.

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言語: eng - English
 日付: 2018-04-112018
 出版の状態: オンラインで出版済み
 ページ: -
 出版情報: -
 目次: -
 査読: 査読あり
 識別子(DOI, ISBNなど): DOI: 10.1002/2017JA025121
 学位: -

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出版物 1

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出版物名: Journal of Geophysical Research: Space Physics
種別: 学術雑誌
 著者・編者:
所属:
出版社, 出版地: Washington, D.C. : American Geophysical Union
ページ: - 巻号: 123 (3) 通巻号: - 開始・終了ページ: 2018 - 2033 識別子(ISBN, ISSN, DOIなど): ISSN: 0148-0227
CoNE: https://pure.mpg.de/cone/journals/resource/991042728714264