论文标题
太阳能无线电III爆发和太空天气影响的统计研究
A Statistical Study of Solar Radio Type III Bursts and Space Weather Implication
论文作者
论文摘要
太阳能无线电爆发（SRB）是在太阳能电晕和星际介质（IPM）中发生的各种现象的签名。在本文中，我们研究了III型爆发的发生及其与黑子数的相关性。这项研究证实，III型爆发的发生与黑子数量很好。此外，使用使用E-Callisto网络获得的数据，我们研究了孤立的III型爆发的漂移率和III型爆发群的持续时间。由于II型，III型和IV型爆发是太阳耀斑和/或CMES的签名，因此我们可以使用无线电观测值来预测太空天气危害。在本文中，我们讨论了两个导致近地无线电停电的事件。由于电子卡利斯托在不同的纵向上包含152个以上的电台，因此我们可以每天24小时使用它来监视太阳能电晕的无线电排放。这些观察结果在监测和预测空间天气危害的几分钟之内到几个小时内起着至关重要的作用。
Solar radio bursts (SRBs) are the signatures of various phenomena that happen in the solar corona and interplanetary medium (IPM). In this article, we have studied the occurrence of Type III bursts and their association with the Sunspot number. This study confirms that the occurrence of Type III bursts correlates well with the Sunspot number. Further, using the data obtained using the e-CALLISTO network, we have investigated the drift rates of isolated Type III bursts and the duration of the group of Type III bursts. Since Type II, Type III, and Type IV bursts are signatures of solar flares and/or CMEs, we can use the radio observations to predict space weather hazards. In this article, we have discussed two events that have caused near-Earth radio blackouts. Since e-CALLISTO comprises more than 152 stations at different longitudes, we can use it to monitor the radio emissions from the solar corona 24 hours a day. Such observations play a crucial role in monitoring and predicting space weather hazards within a few minutes to hours of time.
