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首页> 外文期刊>Journal of Geophysical Research. Biogeosciences >Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejections
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Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejections

机译:日冕图像的日冕物质抛射速度与相关行星际日冕物质抛射的行星际特征之间的关系

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摘要

With an eye to toward space weather forecasting and the planned Solar Terrestrial Relations Observatory mission, a combination of Solwind and SMM coronagraph data and Helios-1 and Pioneer Venus Orbiter interplanetary field and plasma data are used to study statistical relationships between the speeds of coronal mass ejections (CMEs) observed near the Sun and key characteristics of the associated interplanetary disturbances (interplanetary coronal mass ejections (ICMEs)) detected near the ecliptic at <= 1 AU. When confident associations can be made between the coronagraph observations and interplanetary observations, a predictable relationship is found between observed coronagraph CME speeds and subsequently observed ICME bulk plasma speeds. Consistent with earlier work, the CMEs, regardless of their speed, produce ICMEs moving at least as fast as the minimum solar wind speed. As a rule, the CMEs observed at speeds below the average solar wind speed produce ICMEs that travel faster than the associated CME, implying acceleration, while CMEs with coronagraph speeds above the average solar wind speed produce ICMEs that travel slower than the associated CME, implying deceleration of initially fast low-heliolatitude ejecta. A formula is provided for estimating ICME speed from CME speed. As also previously found, faster CMEs tend to produce ICMEs with large internal magnetic field magnitudes. While the size and occurrence of southward Bz in an ICME are not generally related to the observed CME speed, Bz in the sheath region preceding the ICME shows some positive correlation. These observations confirm that while the occurrence of large interplanetary magnetic field magnitudes and high bulk plasma speeds associated with ICME passage may be predictable from coronagraph-derived CME speeds other important ICME features like large-magnitude southward Bz require other diagnostics and tools for forecasts.
机译:考虑到空间天气预报和计划中的太阳陆地关系天文台任务,结合了Solwind和SMM日冕仪数据以及Helios-1和Pioneer Venus轨道星际行星和等离子体数据来研究日冕质量速度之间的统计关系在太阳附近观测到的CMEs和相关的星际干扰(星际冠状物质抛射(ICMEs))的关键特征在黄土附近<= 1 AU被检测到。当可以在日冕仪观测值和行星际观测值之间建立可靠的关联时,可以在观测到的日冕仪CME速度与随后观测到的ICME体等离子体速度之间找到可预测的关系。与早期工作一致,CME不管其速度如何,其产生的ICME的移动速度至少与最小太阳风速一样快。通常,以低于平均太阳风速的速度观测到的CME产生的ICME的运行速度要快于相关CME,这意味着加速,而日冕仪速度高于平均太阳风速的CME产生的ICME的运行速度要慢于相关的CME,这意味着最初快速的低螺旋弹射的减速。提供了用于根据CME速度估算ICME速度的公式。也如先前所发现的,更快的CME倾向于产生具有较大内部磁场强度的ICME。虽然ICME中向南Bz的大小和发生通常与观测到的CME速度无关,但ICME之前的鞘层区域中的Bz显示出一些正相关。这些观察结果证实,虽然可以通过日冕仪得出的CME速度来预测与ICME通过有关的大行星际磁场强度和高体等离子体速度的发生,但其他重要的ICME特征(例如大震度向南的Bz)仍需要其他诊断方法和预测工具。

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