{"title":"Generation of UHR Waves as Inferred From Wave and Electron Flux Measurements by Van Allen Probes","authors":"D. R. Shklyar, E. E. Titova, N. S. Artekha","doi":"10.1029/2025JA033815","DOIUrl":null,"url":null,"abstract":"<p>Observations of upper hybrid resonance (UHR) waves by Van Allen Probes show that the intensity of these waves increases significantly when their frequency is close to an integer multiple of electron gyrofrequency. This article aims at explaining these observations. The explanation assumes that the UHR waves are excited due to cyclotron instability at higher-order cyclotron resonances. Since UHR waves have relatively small group velocity, propagation effect should not play an important role in spectrum evolution of these waves. Thus, the spectrum observed at a given point should be closely related to the wave growth rate at the same point. We calculate the linear growth rate of UHR waves along Van Allen Probe trajectory using the registered plasma parameters and energetic electron density deduced from differential flux measurements. Apart from the hot plasma density, we use other parameters of model distribution compatible with but not inferred from flux measurements. The growth rate along the satellite trajectory calculated in this way fits well the simultaneous spectrum observations.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 6","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2025-06-14","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/10.1029/2025JA033815","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
Observations of upper hybrid resonance (UHR) waves by Van Allen Probes show that the intensity of these waves increases significantly when their frequency is close to an integer multiple of electron gyrofrequency. This article aims at explaining these observations. The explanation assumes that the UHR waves are excited due to cyclotron instability at higher-order cyclotron resonances. Since UHR waves have relatively small group velocity, propagation effect should not play an important role in spectrum evolution of these waves. Thus, the spectrum observed at a given point should be closely related to the wave growth rate at the same point. We calculate the linear growth rate of UHR waves along Van Allen Probe trajectory using the registered plasma parameters and energetic electron density deduced from differential flux measurements. Apart from the hot plasma density, we use other parameters of model distribution compatible with but not inferred from flux measurements. The growth rate along the satellite trajectory calculated in this way fits well the simultaneous spectrum observations.
Van Allen探针对高混合共振(UHR)波的观测表明,当其频率接近电子回旋频率的整数倍时,这些波的强度显著增加。本文旨在解释这些观察结果。这种解释假定超高频波是由于高阶回旋加速器共振的不稳定性而被激发的。由于超高频波具有较小的群速,因此传播效应在超高频波的频谱演化中不应起重要作用。因此,在某一点观测到的光谱应与同一点的波增长率密切相关。我们利用记录的等离子体参数和从差分通量测量中推导出的高能电子密度,计算了UHR波沿范艾伦探测器轨迹的线性增长率。除了热等离子体密度外,我们还使用了与通量测量相容但不是从通量测量推断出来的模型分布的其他参数。用这种方法计算的沿卫星轨迹的增长率与同期的光谱观测结果吻合得很好。