Sabrina F. Tigik, Daniel B. Graham, Yuri V. Khotyaintsev
{"title":"Electron-Scale Energy Transfer Due To Lower Hybrid Waves During Asymmetric Reconnection","authors":"Sabrina F. Tigik, Daniel B. Graham, Yuri V. Khotyaintsev","doi":"10.1029/2024JA033503","DOIUrl":null,"url":null,"abstract":"<p>We use Magnetospheric Multiscale mission data to investigate electron-scale energy transfer due to lower hybrid drift waves during magnetopause reconnection. We analyze waves observed in an electron-scale plasma mixing layer at the edge of the magnetospheric outflow. Using high-resolution <span></span><math>\n <semantics>\n <mrow>\n <mn>7.5</mn>\n <mspace></mspace>\n <mi>m</mi>\n <mi>s</mi>\n </mrow>\n <annotation> $7.5\\hspace*{.5em}\\mathrm{m}\\mathrm{s}$</annotation>\n </semantics></math> electron moments, we obtain an electron current density with a Nyquist frequency of <span></span><math>\n <semantics>\n <mrow>\n <mo>∼</mo>\n <mn>66</mn>\n <mspace></mspace>\n <mi>H</mi>\n <mi>z</mi>\n </mrow>\n <annotation> ${\\sim} 66\\hspace*{.5em}\\mathrm{H}\\mathrm{z}$</annotation>\n </semantics></math>, sufficient to resolve most of the lower hybrid drift wave power observed in the event. We then employ wavelet analysis to evaluate <span></span><math>\n <semantics>\n <mrow>\n <mi>δ</mi>\n <mi>J</mi>\n <mspace></mspace>\n <mo>⋅</mo>\n <mspace></mspace>\n <mi>δ</mi>\n <mi>E</mi>\n </mrow>\n <annotation> $\\delta \\mathbf{J}\\,\\cdot \\,\\delta \\mathbf{E}$</annotation>\n </semantics></math>, which accounts for the phase differences between the fluctuating quantities. The analysis shows that the energy exchange is localized within the plasma mixing layer, and it is highly fluctuating, with energy bouncing between waves and electrons throughout the analyzed time and frequency range. However, the cumulative sum over time indicates a net energy transfer from the waves to electrons. We observe an anomalous electron flow toward the magnetosphere, consistent with diffusion and electron mixing. These results indicate that waves and electrons interact dynamically to dissipate the excess internal energy accumulated by sharp density gradients. We conclude that the electron temperature profile within the plasma mixing layer is produced by a combination of electron diffusion across the layer, as well as heating by large-scale parallel potential and lower hybrid drift waves.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 4","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-04-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA033503","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
We use Magnetospheric Multiscale mission data to investigate electron-scale energy transfer due to lower hybrid drift waves during magnetopause reconnection. We analyze waves observed in an electron-scale plasma mixing layer at the edge of the magnetospheric outflow. Using high-resolution electron moments, we obtain an electron current density with a Nyquist frequency of , sufficient to resolve most of the lower hybrid drift wave power observed in the event. We then employ wavelet analysis to evaluate , which accounts for the phase differences between the fluctuating quantities. The analysis shows that the energy exchange is localized within the plasma mixing layer, and it is highly fluctuating, with energy bouncing between waves and electrons throughout the analyzed time and frequency range. However, the cumulative sum over time indicates a net energy transfer from the waves to electrons. We observe an anomalous electron flow toward the magnetosphere, consistent with diffusion and electron mixing. These results indicate that waves and electrons interact dynamically to dissipate the excess internal energy accumulated by sharp density gradients. We conclude that the electron temperature profile within the plasma mixing layer is produced by a combination of electron diffusion across the layer, as well as heating by large-scale parallel potential and lower hybrid drift waves.
利用磁层多尺度任务数据,研究了磁层顶重联过程中较低混合漂移波引起的电子尺度能量传递。我们分析了磁层出口边缘的电子尺度等离子体混合层中观测到的波。利用高分辨率7.5 m s $7.5\hspace*{.5em}\mathrm{m}\mathrm{s}$电子矩,我们得到奈奎斯特频率为~ 66 hz ${\sim} 66\hspace*{.5em}\mathrm{H}\mathrm{z}$的电子电流密度。足以解决大多数较低的混合漂移波能观测到的事件。然后,我们利用小波分析来计算δ J·δ E $\delta \mathbf{J}\,\cdot \,\delta \mathbf{E}$,它可以解释波动量之间的相位差。分析表明,能量交换局限于等离子体混合层内,且波动较大,在分析的时间和频率范围内,能量在波和电子之间弹跳。然而,随着时间的累积和表明从波到电子的净能量转移。我们观察到一个反常的电子流向磁层,与扩散和电子混合一致。这些结果表明,波和电子动态地相互作用,以耗散由急剧密度梯度积累的多余内能。我们得出结论,等离子体混合层内的电子温度分布是由电子在等离子体混合层内的扩散以及大尺度平行电位和低混合漂移波的加热共同产生的。