太阳耀斑及其预测方法

O. Boyarkin, A. Kapskaya
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引用次数: 0

摘要

预测太阳耀斑是太阳物理学中的一项重要任务。太阳耀斑的发生高度依赖于太阳磁场的结构和拓扑结构。太阳耀斑造成的干扰影响地面通信、导航、警报系统的运行,扰乱空间物体和飞机上的机载电子设备的功能。考虑到这些因素,有一个预测这种现象的问题。这项工作调查了太阳耀斑的发生过程,预测方法的发展以及在这种情况下出现的困难。同时介绍了一种最常见的太阳耀斑探测方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
SOLAR FLARES AND THEIR PREDICTION METHODS
Predicting solar flares is an important task in solar physics. The occurrence of solar flares is highly dependent on the structure and topology of the Sun’s magnetic fields. Disturbances caused by solar flares affect the operation of ground-based communications, navigation, warning systems, disrupt the functioning of on-board electronic equipment on space objects and aircrafts. In connection with these factors, there is an issue of predicting this phenomenon. This work investigates the process of occurrence of solar flares, the development of methods for predicting them and the difficulties that arise in this case. Also it presents one of the most common methods of solar flares.
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