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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Dependence of solar proton events on their associated activities: Coronal mass ejection parameters
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Dependence of solar proton events on their associated activities: Coronal mass ejection parameters

机译:太阳质子事件的依赖相关活动:日冕物质抛射参数

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In this study we have examined the occurrence probability of solar proton events (SPEs) and their peak fluxes depending on coronal mass ejection (CME) parameters, linear speed (V), angular width (AW), and location (L). For this we used the NOAA SPE list and their associated CME data from 1997 to 2006. We found that the probability strongly depends on CME speed and angular width as follows. The highest association (36.1%) is found for the full halo CMEs with V 1500 kms ~(-1) but the lowest association (0.9%) is found for the partial halo CMEs with 400 kms ~(-1) V < 1000 kms ~(-1). The SPE occurrence probabilities are different as much as 4.9 to 23 times according to CME speed and 1.6 to 6.5 times to angular width. The probabilities depending on CME speed and location increase from the eastern region to the western region and with speed. We have also examined the relationship between CME speed and SPE flux as well as its dependence on angular width (partial halo and full halo), longitude (east, center, and west) and direction parameter (<0.4 and ≥0.4). Our results show that the relationships strongly depend on longitude as well as direction parameter.
机译:在这项研究中,我们调查了发生(spe)和太阳质子事件的概率峰值流量取决于日冕物质弹射(CME)参数、线性速度(V),角宽度(AW)、位置(L)。我们利用NOAA SPE列表和它们相关的芝加哥商品交易所从1997年到2006年的数据。强烈依赖于芝加哥商品交易所的速度和概率角宽度如下。(36.1%)被发现的完整的光环cme与V1500公里~(1)但最低协会(0.9%)是偏光环cme发现400公里~ (1) V < 1000公里~(1)。概率是不同的高达4.9 - 23所示*根据CME速度和1.6至6.5倍角宽度。CME东部增长速度和位置给西部地区和速度。还研究了芝加哥商品交易所之间的关系吗速度和SPE通量以及依赖角宽度(部分光环,光环),经度(东、中心和西部)和方向参数(< 0.4和≥0.4)。强烈依赖于经度的关系方向参数。

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