☀️定义
耀斑是太阳大气中局部区域的突然、强烈的能量释放，通常伴随着电磁辐射的增强和高能粒子的发射。它们通常与太阳磁场的剧烈活动有关，是太阳活动最直观的表现之一。
☀️成因
太阳耀斑的成因与太阳磁场的变化紧密相关，包括
磁场线扭曲和太阳黑子活动。
☀️ 分类
耀斑按照它们释放的能量强度分为不同的级别，从若到强分别是A级、B级、C级、M级、X级。
☀️影响
包括通讯干扰，地磁暴，极光活动，航天器风险等。
☀️观测
包括用太阳望远镜、太阳观测卫星，以及预报系统。
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