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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Ionospheric oxygen ions dominant bursty bulk flows: Cluster and Double Star observations
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Ionospheric oxygen ions dominant bursty bulk flows: Cluster and Double Star observations

机译:电离层氧离子主导丛发性批量流:集群和双星观察

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摘要

Two extreme oxygen-rich bursty bulk flows (BBFs) with predominant ionospheric O+ ions have been observed on 8 November 2004 by the Cluster and Double Star spacecraft during a strong magnetic storm time period with Dst = ?373 nT. The oxygen densities in two BBFs are found to be 3–5 times larger than the hydrogen densities and the oxygen thermal pressures in the BBFs are 8 times higher than the hydrogen thermal pressure. These BBFs are associated with nested magnetic structures and are observed simultaneously by the CLUSTER and the DSP TC-1 spacecraft. Thus, the flow braking region should be greatly pushed inside the usual pressure balance region (even inside the inner magnetosphere) since the BBF is dominated by oxygen ions. Results in this paper indicate that oxygen dominated BBFs can be formed during a strong magnetic storm time period. The observations made in this paper suggest that singly charged oxygen ions embedded in the BBFs could be carried into the ring current region by bursty flows during very intense magnetic storms.
机译:两种极端富氧丛发性散装流(bbf)与主要的电离层O +离子集群和观察到的2004年11月8日双星飞船在一个强大的磁场风暴和Dst =时间吗? 373元。氧密度在两个bbf发现3 - 5次比氢密度和氧热压力bbf的8倍比氢热压力。与嵌套磁结构同时观察到的集群和DSP TC-1飞船。制动地区应该大大推动内部通常的压力平衡地区(甚至在里面BBF以来内部磁气圈)由氧离子。表明,氧气就可以形成bbf主导强烈的磁暴期间内。本文观察表明,单独bbf氧离子嵌入可以带进环电流区非常强烈的磁暴期间丛发性流动。

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