首页> 美国卫生研究院文献>Nature Communications >Strong whistler mode waves observed in the vicinity of Jupiter’s moons
【2h】

Strong whistler mode waves observed in the vicinity of Jupiter’s moons

机译:在木星卫星附近观测到强烈的吹口哨模式波

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

Understanding of wave environments is critical for the understanding of how particles are accelerated and lost in space. This study shows that in the vicinity of Europa and Ganymede, that respectively have induced and internal magnetic fields, chorus wave power is significantly increased. The observed enhancements are persistent and exceed median values of wave activity by up to 6 orders of magnitude for Ganymede. Produced waves may have a pronounced effect on the acceleration and loss of particles in the Jovian magnetosphere and other astrophysical objects. The generated waves are capable of significantly modifying the energetic particle environment, accelerating particles to very high energies, or producing depletions in phase space density. Observations of Jupiter’s magnetosphere provide a unique opportunity to observe how objects with an internal magnetic field can interact with particles trapped in magnetic fields of larger scale objects.
机译:对波浪环境的理解对于理解粒子如何在空间中加速和丢失至关重要。这项研究表明,在分别具有感应磁场和内部磁场的欧罗巴和木卫三附近,合唱波功率显着增加。对于木卫三,观测到的增强是持久的,并且比波浪活动的中值超出6个数量级。产生的波可能对木星磁层和其他天体物理物体中粒子的加速和损失产生明显影响。产生的波能够显着地改变高能粒子的环境,将粒子加速到非常高的能量,或产生相空间密度的耗尽。对木星磁层的观测为观察具有内部磁场的物体如何与较大规模的物体的磁场中捕获的粒子相互作用提供了独特的机会。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号