夜侧各向同性边界的纬向剖面图:自适应磁层模式观测与预测的比较

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
V. A. Sergeev, M. V. Kubyshkina, I. V. Kubyshkin, A. Artemyev, V. Angelopoulos
{"title":"夜侧各向同性边界的纬向剖面图:自适应磁层模式观测与预测的比较","authors":"V. A. Sergeev,&nbsp;M. V. Kubyshkina,&nbsp;I. V. Kubyshkin,&nbsp;A. Artemyev,&nbsp;V. Angelopoulos","doi":"10.1029/2025JA034428","DOIUrl":null,"url":null,"abstract":"<p>There is significant interest in monitoring the instantaneous magnetic configurations and dynamic states of the magnetotail and understanding what controls them. A unique and attractive opportunity is provided by remote sensing of the radial profile of the equatorial magnetic field curvature based on low-latitude energetic particle measurements of isotropy boundaries (IBs), providing that you can determine the origin of isotropic precipitation. To validate the magnetic field line curvature scattering (FLCS) as the main mechanism of the isotropy boundary formation, we compare coarse energy versus latitude IB profiles (in 3 + 3 energy channels) measured during a few dozen passes of POES and ELFIN spacecraft with the theoretical predictions of the adapted (AM03) magnetospheric model. Two studied intervals in August 2022 include substorm events of various intensities for which good spacecraft coverage in the near magnetotail helps reconstruct the adaptive model in the areas where the IBs are formed. We find a general agreement between the predicted and observed <i>coarse</i> IB profiles' shape and latitude, validating the FLCS hypothesis. Deviations are also observed, and we discuss the factors that can influence identification of the true FLCS profiles in observations and predictions, including limitations of adaptive modeling, non-monotonic radial structure of the tail magnetic field, and interference of FLCS with other precipitation mechanisms related to wave-particle interactions. Most can be avoided by improving the sensitivity, energy coverage, and resolution in future instruments.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 10","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2025-10-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Latitudinal Profiles of Nightside Isotropy Boundaries: Comparison of Observations and Predictions of Adaptive Magnetospheric Model\",\"authors\":\"V. A. Sergeev,&nbsp;M. V. Kubyshkina,&nbsp;I. V. Kubyshkin,&nbsp;A. Artemyev,&nbsp;V. Angelopoulos\",\"doi\":\"10.1029/2025JA034428\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>There is significant interest in monitoring the instantaneous magnetic configurations and dynamic states of the magnetotail and understanding what controls them. A unique and attractive opportunity is provided by remote sensing of the radial profile of the equatorial magnetic field curvature based on low-latitude energetic particle measurements of isotropy boundaries (IBs), providing that you can determine the origin of isotropic precipitation. To validate the magnetic field line curvature scattering (FLCS) as the main mechanism of the isotropy boundary formation, we compare coarse energy versus latitude IB profiles (in 3 + 3 energy channels) measured during a few dozen passes of POES and ELFIN spacecraft with the theoretical predictions of the adapted (AM03) magnetospheric model. Two studied intervals in August 2022 include substorm events of various intensities for which good spacecraft coverage in the near magnetotail helps reconstruct the adaptive model in the areas where the IBs are formed. We find a general agreement between the predicted and observed <i>coarse</i> IB profiles' shape and latitude, validating the FLCS hypothesis. Deviations are also observed, and we discuss the factors that can influence identification of the true FLCS profiles in observations and predictions, including limitations of adaptive modeling, non-monotonic radial structure of the tail magnetic field, and interference of FLCS with other precipitation mechanisms related to wave-particle interactions. Most can be avoided by improving the sensitivity, energy coverage, and resolution in future instruments.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"130 10\",\"pages\":\"\"},\"PeriodicalIF\":2.9000,\"publicationDate\":\"2025-10-02\",\"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://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JA034428\",\"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://agupubs.onlinelibrary.wiley.com/doi/10.1029/2025JA034428","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

人们对监测磁尾的瞬时磁结构和动态状态以及了解是什么控制它们非常感兴趣。基于低纬度高能粒子测量的各向同性边界(IBs)遥感赤道磁场曲率的径向剖面提供了一个独特而有吸引力的机会,如果你可以确定各向同性降水的起源。为了验证磁场线曲率散射(FLCS)是各向同性边界形成的主要机制,我们将POES和ELFIN航天器在几十次飞行中测量的粗能量与纬度IB剖面(在3 + 3能量通道中)与改进的(AM03)磁层模型的理论预测进行了比较。2022年8月的两个研究间隔包括不同强度的亚暴事件,在近磁尾的良好航天器覆盖有助于重建ibb形成区域的自适应模型。我们发现预测和观测到的粗IB剖面的形状和纬度大致一致,验证了FLCS假设。我们还观察到偏差,并讨论了在观测和预测中可能影响FLCS真实剖面识别的因素,包括自适应建模的局限性、尾部磁场的非单调径向结构以及FLCS与其他与波粒相互作用相关的降水机制的干扰。在未来的仪器中,通过提高灵敏度、能量覆盖范围和分辨率,可以避免大多数问题。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Latitudinal Profiles of Nightside Isotropy Boundaries: Comparison of Observations and Predictions of Adaptive Magnetospheric Model

Latitudinal Profiles of Nightside Isotropy Boundaries: Comparison of Observations and Predictions of Adaptive Magnetospheric Model

There is significant interest in monitoring the instantaneous magnetic configurations and dynamic states of the magnetotail and understanding what controls them. A unique and attractive opportunity is provided by remote sensing of the radial profile of the equatorial magnetic field curvature based on low-latitude energetic particle measurements of isotropy boundaries (IBs), providing that you can determine the origin of isotropic precipitation. To validate the magnetic field line curvature scattering (FLCS) as the main mechanism of the isotropy boundary formation, we compare coarse energy versus latitude IB profiles (in 3 + 3 energy channels) measured during a few dozen passes of POES and ELFIN spacecraft with the theoretical predictions of the adapted (AM03) magnetospheric model. Two studied intervals in August 2022 include substorm events of various intensities for which good spacecraft coverage in the near magnetotail helps reconstruct the adaptive model in the areas where the IBs are formed. We find a general agreement between the predicted and observed coarse IB profiles' shape and latitude, validating the FLCS hypothesis. Deviations are also observed, and we discuss the factors that can influence identification of the true FLCS profiles in observations and predictions, including limitations of adaptive modeling, non-monotonic radial structure of the tail magnetic field, and interference of FLCS with other precipitation mechanisms related to wave-particle interactions. Most can be avoided by improving the sensitivity, energy coverage, and resolution in future instruments.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信