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Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era

机译:地球的范艾伦辐射带:从发现到范艾伦探针时代

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Discovery of the Earth's Van Allen radiation belts by instruments flown on Explorer 1 in 1958 was the first major discovery of the Space Age. The observation of distinct inner and outer zones of trapped megaelectron volt (MeV) particles, primarily protons at low altitude and electrons at high altitude, led to early models for source and loss mechanisms including Cosmic Ray Albedo Neutron Decay for inner zone protons, radial diffusion for outer zone electrons and loss to the atmosphere due to pitch angle scattering. This scattering lowers the mirror altitude for particles in their bounce motion parallel to the Earth's magnetic field until they suffer collisional loss. A view of the belts as quasi-static inner and outer zones of energetic particles with different sources was modified by observations made during the Solar Cycle 22 maximum in solar activity over 1989-1991. The dynamic variability of outer zone electrons was measured by the Combined Radiation Release and Effects Satellite launched in July 1990. This variability is caused by distinct types of heliospheric structure that vary with the solar cycle. The launch of the twin Van Allen Probes in August 2012 has provided much longer and more comprehensive measurements during the declining phase of Solar Cycle 24. Roughly half of moderate geomagnetic storms, determined by intensity of the ring current carried mostly by protons at hundreds of kiloelectron volts, produce an increase in trapped relativistic electron flux in the outer zone. Mechanisms for accelerating electrons of hundreds of electron volts stored in the tail region of the magnetosphere to MeVenergies in the trapping region are described in this review: prompt and diffusive radial transport and local acceleration driven by magnetospheric waves. Such waves also produce pitch angle scattering loss, as does outward radial transport, enhanced when the magnetosphere is compressed. While quasilinear simulations have been used to successfully reproduce many
机译:1958年在探险家中飞行的仪器发现地球范艾伦辐射带是空间年龄的第一次重大发现。观察捕获的兆元电伏(MEV)颗粒的不同内部和外部区域,主要是在高海拔低空和电子处于低空的质子,导致源极和损耗机制的早期模型,包括用于内部区域质子的宇宙射线Albedo中子衰减,径向扩散对于外部区域电子和由于俯仰角散射而对大气的损失。这种散射在与地球磁场平行于地球磁场的反弹运动中的镜子高度降低了颗粒,直到它们遭受碰撞损失。通过在8089-1991的太阳能活动中最大的太阳能循环22在太阳能循环22期间的观察结果来修改带有不同来源的准静态内和外部区域的挡板。通过1990年7月推出的组合辐射释放和效果卫星测量了外部区域电子的动态变化。这种可变性是由太阳循环变化的不同类型的螺旋体结构引起的。 2012年8月推出的双van艾伦探针在太阳循环阶段的下降期间提供了更长且更全面的测量。大约一半的中等地磁风暴的一半,由戒指电流的强度决定,由数百千电子元数量的质子携带伏特,在外区域中产生截图相对论电子通量的增加。本文描述了在捕获区域中储存在磁层的尾部区域中的数百个电子伏的电子的机制:通过磁磁波驱动的提示和漫射径向传输和局部加速度。这种波还产生俯仰角散射损失,如向外径向传输,当压缩磁层时增强。虽然Quasilinear模拟已被用于成功重现许多

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