太阳黑子活动区与太阳耀斑和太阳质子事件的发生有紧密的关系。选取活动区特征参量包括太阳黑子群面积,磁分类,McIntosh分类,10cm射电流量,统计和耀斑发生的产率关系;还统计了太阳活动区的位置,软X射线通量和质子事件的产率关系。对于磁分类,McIntosh分类的每一种分类类型计算了耀斑产率,对黑子群面积和10cm射电流量和软X射线通量用函数拟合了它们和太阳耀斑和太阳质子事件的产率关系。对活动区位置采用了分段统计质子事件产率的方法。统计结果显示我们选取的活动区特征参量与太阳耀斑和质子事件有较强的相关性。统计结果可作为以后建立太阳耀斑,太阳质子事件预报模型中预报因子的选取的基础。
Solar sunspots active region has a close connection with the occurrence of solar flare and solar proton event. A statistic analysis was made on the correlations of the solar flare and the active region parameters including the area of sunspot groups, the magnetic class. Besides, the active region location and the soft X-ray flux was chosen to make a statistic on the occurrence of solar proton events. The flare productivity of each class of the magnetic classification and the McIntosh classification is calculated. The flare productivities of the area of sunspot groups and the solar radio flux are computed and their correlations with the flares are fitted by Gauss function. The active region location is divided by sub-sections and the proton event productivity for each sub-sections is calculated. The statistic results show that solar flare and proton event productivity closely connects with the active region parameters. The concrete statistic results may become the basis of the research for solar flare and proton event forecasting.