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Coincident particle and optical observations of nightside subauroral proton precipitation

机译:同时粒子和光学的观察阴面subauroral质子降水

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We report two instances of nightside subauroral proton precipitation observed during a geomagnetic storm: (1) An arc at è 50° magnetic latitude (MLAT), which extended roughly from midnight to 6 magnetic local time (MLT), and (2) A corotating spot at 51.5° MLAT, postmidnight. The proton precipitation was observed by both the IMAGE SI-12 proton aurora (Doppler-shifted Lyman- α) imager, and low-altitude Polar-orbiting Operational Environmental Satellites (POESs) that serendipitously traversed both the arc and the spot, providing in situ particle measurements. The Lyman-alpha emission and the particle observations match closely. The particle measurements showed that the energies of the precipitating protons extended to several hundred keV, but no enhancements in the protons below 20 keV were observed. Cluster observations showed that the ring current contained protons with energies extending from tens of eV to several hundred keV; thus, the particles are scattered into the atmosphere from an existing reservoir. Outside the luminous regions, but at the same magnetic latitude, the POES satellites observed localized regions with enhanced proton fluxes outside, but close to, the loss cone. This shows that the protons along a large region in MLT are subjected to pitch angle scattering. Model calculations of the plasmasphere show that the arc and the proton precipitation are located just inside the plasmapause. The intensity and longitudinal extension of the arc are modulated by the dynamical pressure in the solar wind. In the dusk sector, ground stations recorded electromagnetic ion cyclotron waves associated with localized proton precipitation just inside the plasmapause. This suggests that the proton precipitation is caused by wave/particle interaction. Key points Sub-auroral proton aurora is reported, with coincident in-situ measurements The pitch angle scattering extends beyond the luminous regions The location of the precipitation suggests a relation to EMIC waves
机译:我们报告两个实例的阴面subauroral质子降水期间观察到的磁暴:(1)电弧在e 50°磁纬度(MLAT)延长约当地时间午夜6磁(MLT),和(2)共转点为51.5°MLAT postmidnight。质子降水都被观察到莱曼-图像秉风质子极光(因都卜勒频移α)成像仪,低空极轨运行环境卫星(POESs)遍历弧和的意外收获点,提供原位颗粒测量。莱曼-阿尔法辐射和粒子密切观察匹配。测量显示的能量沉淀质子扩展到数百凯文,但没有增强质子低于20凯文被观察到。环电流包含质子能量从数万eV几个几百keV;从现有的水库到大气中。外发光区域,但是在相同的磁纬度,阿宝卫星观测到的局部地区增强质子通量外面,但接近,损失锥。MLT质子沿大地区螺旋角散射。计算等离子体层的显示弧和质子降水在等离子体层顶。纵向扩展弧的调制在太阳风的动态压力。黄昏部门、地面站记录电磁相关离子回旋波局部质子降水就在里面等离子体层顶。降水是由波/粒子引起的交互。报道,重合的原位测量吗超出投掷角扩散过程发光区域的位置降水关系表明位的波

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