Observations of large‐amplitude, parallel, electrostatic waves associated with the Kelvin‐Helmholtz instability by the magnetospheric multiscale mission

Abstract On 8 September 2015, the four Magnetospheric Multiscale spacecraft encountered a Kelvin‐Helmholtz unstable magnetopause near the dusk flank. The spacecraft observed periodic compressed current sheets, between which the plasma was turbulent. We present observations of large‐amplitude (up to...

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書誌詳細
出版年:Geophysical Research Letters
主要な著者: Victoria Wilder, R. E. Ergun, S. J. Schwartz, D. L. Newman, S. Eriksson, J. E. Stawarz, M. V. Goldman, K. A. Goodrich, D. J. Gershman, D. M. Malaspina, J. C. Holmes, A. P. Sturner, J. L. Burch, R. B. Torbert, P.‐A. Lindqvist, G. T. Marklund, Y. Khotyaintsev, R. J. Strangeway, C. T. Russell, C. J. Pollock, B. L. Giles, J. C. Dorrelli, L. A. Avanov, W. R. Patterson, F. Plaschke, W. Magnes
フォーマット: 論文
言語:英語
出版事項: Wiley 2016-09-01
主題:
オンライン・アクセス:https://doi.org/10.1002/2016GL070404
その他の書誌記述
要約:Abstract On 8 September 2015, the four Magnetospheric Multiscale spacecraft encountered a Kelvin‐Helmholtz unstable magnetopause near the dusk flank. The spacecraft observed periodic compressed current sheets, between which the plasma was turbulent. We present observations of large‐amplitude (up to 100 mV/m) oscillations in the electric field. Because these oscillations are purely parallel to the background magnetic field, electrostatic, and below the ion plasma frequency, they are likely to be ion acoustic‐like waves. These waves are observed in a turbulent plasma where multiple particle populations are intermittently mixed, including cold electrons with energies less than 10 eV. Stability analysis suggests a cold electron component is necessary for wave growth.
ISSN:0094-8276
1944-8007