太阳周期 24 期间 RSTN 检测到的公制 II 型射电暴目录

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Bendict Lawrance, Pooja Devi, Ramesh Chandra, Rositsa Miteva
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引用次数: 0

摘要

在这项研究中,我们利用射电太阳望远镜网络(RSTN)编制了一份米II型射电暴目录,以研究射电暴的发生、关联和性质及其母体太阳活动现象。根据射电发射特征的强度和清晰度,我们将米II型射电暴分为两个定性类别,即确定的和不确定的。我们分析了太阳周期 24(2009-2019 年)的 RSTN 数据,这些数据可从四个全球台站免费获得:这些数据可从 Learmonth、Sanvito、Sagamore Hills 和 Palehua 四个全球站点免费获取。通过仔细的目视检查,我们收集了在 25 - 180 MHz 范围内探测到的所有公制 II 型爆发。研究了这些脉冲串与太阳爆发事件(如太阳耀斑和日冕物质抛射)之间的关系,并对结果进行了介绍和讨论。研究结果可用于从地面无线电角度揭示太阳和空间天气活动的发生。将向太阳科学界免费提供新收集的公转 II 型和相关太阳活动目录。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 24

A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 24

A Catalog of Metric Type II Radio Bursts Detected by RSTN During Solar Cycle 24

In this study, we compile a catalog of metric type II radio bursts using the Radio Solar Telescope Network (RSTN) to study the occurrence, associations, and properties of the emission and their parent solar activity phenomena. According to the intensity and clarity of the radio emission features, we have divided the m-type II radio bursts into two qualitative categories, namely certain and uncertain. We analyzed RSTN data in Solar Cycle 24 (2009 – 2019), which is freely available from four worldwide stations: Learmonth, Sanvito, Sagamore Hills, and Palehua. Through careful visual inspection, we have collected all metric type II bursts detected in the range of 25 – 180 MHz. The relationships between these bursts and solar eruptive events, such as solar flares and coronal mass ejections (CMEs), are studied, and the results are presented and discussed. The outcomes could be used to reveal the occurrence of solar and space-weather activities based on the ground-based radio perspective. The newly assembled catalog of metric type II and associated solar events will be made freely available to the solar scientific community.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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