Ahmad Lalti, Yuri V. Khotyaintsev, Daniel B. Graham, Andris Vaivads
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We use a method based on the interferometry of the electric field measured aboard the magnetospheric multiscale spacecraft to analyze the evolution of the properties of electrostatic waves across four quasi-perpendicular shocks, with <span></span><math>\n <semantics>\n <mrow>\n <mn>1.4</mn>\n <mo>≤</mo>\n <msub>\n <mi>M</mi>\n <mi>A</mi>\n </msub>\n <mo>≤</mo>\n <mn>4.2</mn>\n </mrow>\n <annotation> $1.4\\le {M}_{A}\\le 4.2$</annotation>\n </semantics></math> and <span></span><math>\n <semantics>\n <mrow>\n <mn>66</mn>\n <mo>°</mo>\n <mo>≤</mo>\n <msub>\n <mi>θ</mi>\n <mrow>\n <mi>B</mi>\n <mi>n</mi>\n </mrow>\n </msub>\n <mo>≤</mo>\n <mn>87</mn>\n <mo>°</mo>\n </mrow>\n <annotation> $66{}^{\\circ}\\le {\\theta }_{Bn}\\le 87{}^{\\circ}$</annotation>\n </semantics></math>. Most of the analyzed wave bursts across all four shocks have a frequency in the plasma frame <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>f</mi>\n <mrow>\n <mi>p</mi>\n <mi>l</mi>\n </mrow>\n </msub>\n </mrow>\n <annotation> ${f}_{pl}$</annotation>\n </semantics></math> lower than the ion plasma frequency <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>f</mi>\n <mrow>\n <mi>p</mi>\n <mi>i</mi>\n </mrow>\n </msub>\n </mrow>\n <annotation> ${f}_{pi}$</annotation>\n </semantics></math> and a wavelength on the order of 20 Debye lengths <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>λ</mi>\n <mi>D</mi>\n </msub>\n </mrow>\n <annotation> ${\\lambda }_{D}$</annotation>\n </semantics></math>. Their direction of propagation is predominantly field-aligned upstream and downstream of the bow shock, while it is highly oblique within the shock transition region, which might indicate a shift in their generation mechanism. The similarity in wave properties between the analyzed shocks, despite their different shock parameters, indicates the fundamental nature of electrostatic waves for the dynamics of collisionless shocks.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 7","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-07-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2025JA033881","citationCount":"0","resultStr":"{\"title\":\"Debye-Scale Electrostatic Waves Across Quasi-Perpendicular Shocks\",\"authors\":\"Ahmad Lalti, Yuri V. Khotyaintsev, Daniel B. Graham, Andris Vaivads\",\"doi\":\"10.1029/2025JA033881\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The evolution of the properties of short-scale electrostatic waves across collisionless shocks remains an open question. We use a method based on the interferometry of the electric field measured aboard the magnetospheric multiscale spacecraft to analyze the evolution of the properties of electrostatic waves across four quasi-perpendicular shocks, with <span></span><math>\\n <semantics>\\n <mrow>\\n <mn>1.4</mn>\\n <mo>≤</mo>\\n <msub>\\n <mi>M</mi>\\n <mi>A</mi>\\n </msub>\\n <mo>≤</mo>\\n <mn>4.2</mn>\\n </mrow>\\n <annotation> $1.4\\\\le {M}_{A}\\\\le 4.2$</annotation>\\n </semantics></math> and <span></span><math>\\n <semantics>\\n <mrow>\\n <mn>66</mn>\\n <mo>°</mo>\\n <mo>≤</mo>\\n <msub>\\n <mi>θ</mi>\\n <mrow>\\n <mi>B</mi>\\n <mi>n</mi>\\n </mrow>\\n </msub>\\n <mo>≤</mo>\\n <mn>87</mn>\\n <mo>°</mo>\\n </mrow>\\n <annotation> $66{}^{\\\\circ}\\\\le {\\\\theta }_{Bn}\\\\le 87{}^{\\\\circ}$</annotation>\\n </semantics></math>. Most of the analyzed wave bursts across all four shocks have a frequency in the plasma frame <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>f</mi>\\n <mrow>\\n <mi>p</mi>\\n <mi>l</mi>\\n </mrow>\\n </msub>\\n </mrow>\\n <annotation> ${f}_{pl}$</annotation>\\n </semantics></math> lower than the ion plasma frequency <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>f</mi>\\n <mrow>\\n <mi>p</mi>\\n <mi>i</mi>\\n </mrow>\\n </msub>\\n </mrow>\\n <annotation> ${f}_{pi}$</annotation>\\n </semantics></math> and a wavelength on the order of 20 Debye lengths <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>λ</mi>\\n <mi>D</mi>\\n </msub>\\n </mrow>\\n <annotation> ${\\\\lambda }_{D}$</annotation>\\n </semantics></math>. Their direction of propagation is predominantly field-aligned upstream and downstream of the bow shock, while it is highly oblique within the shock transition region, which might indicate a shift in their generation mechanism. The similarity in wave properties between the analyzed shocks, despite their different shock parameters, indicates the fundamental nature of electrostatic waves for the dynamics of collisionless shocks.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"130 7\",\"pages\":\"\"},\"PeriodicalIF\":2.6000,\"publicationDate\":\"2025-07-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2025JA033881\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Geophysical Research: Space Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1029/2025JA033881\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2025JA033881","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
摘要
短尺度静电波在无碰撞冲击中的性质演变仍然是一个悬而未决的问题。利用磁层多尺度航天器上实测电场的干涉测量方法,分析了静电波在四种准垂直激波上的性质演变。1.4≤M A≤4.2 $1.4\le {M}_{A}\le 4.2$, 66°≤θ BN≤87°$66{}^{\circ}\le {\theta }_{Bn}\le 87{}^{\circ}$。在所有四种冲击中,大多数分析的波爆发在等离子体框架中的频率为p1 ${f}_{pl}$低于离子等离子体频率fp i ${f}_{pi}$和大约20个德拜长度λ D ${\lambda }_{D}$的波长。它们的传播方向主要在弓形激波的上游和下游呈场向排列,而在激波过渡区内则呈高度倾斜,这可能表明它们的产生机制发生了转变。尽管所分析的冲击参数不同,但它们之间的波性质相似,这表明静电波在无碰撞冲击动力学中的基本性质。
Debye-Scale Electrostatic Waves Across Quasi-Perpendicular Shocks
The evolution of the properties of short-scale electrostatic waves across collisionless shocks remains an open question. We use a method based on the interferometry of the electric field measured aboard the magnetospheric multiscale spacecraft to analyze the evolution of the properties of electrostatic waves across four quasi-perpendicular shocks, with and . Most of the analyzed wave bursts across all four shocks have a frequency in the plasma frame lower than the ion plasma frequency and a wavelength on the order of 20 Debye lengths . Their direction of propagation is predominantly field-aligned upstream and downstream of the bow shock, while it is highly oblique within the shock transition region, which might indicate a shift in their generation mechanism. The similarity in wave properties between the analyzed shocks, despite their different shock parameters, indicates the fundamental nature of electrostatic waves for the dynamics of collisionless shocks.