概括
总太阳辐射量测量显示了变化,与太阳黑子发展相关的下降. 这表明在太阳能活跃区域内存在大量的能量储存.
科学领域:
- 太阳物理 太阳物理
- 天文学 天文学
- 太空科学 太空科学
背景情况:
- 总太阳辐射 (TSI) 是地球气候的一个基本参数.
- TSI 中的变化可能会影响气候和太空天气.
- 以前的测量在精度和时间分辨率方面存在局限性.
研究的目的:
- 来自太阳最大值任务 (SMM) 的 TSI 高精度测量结果.
- 分析 TSI 在最初的 153 天观察期间的变化.
- 调查 TSI 波动与太阳能活动之间的关系.
主要方法:
- 在SMM卫星上使用了主动空腔辐射仪辐射监测仪 (ACRIM).
- 收集了高精度的STI数据,不确定性只有0.001%.
- 分析了轨道对轨道的变化和辐射强度波动的光谱特征.
主要成果:
- 在153天的TSI中观察到显著的变化,幅度约为平均值的+/- 0.05% (1368.31W/m2).
- 确定了与带限噪声相一致的辐射强度波动,高频切断距离接近0.15天-1.1.
- 发现两个主要的辐射下降 (高达0.2%,持续约1周) 与太阳黑子组发育有很强的相关性.
结论:
- TSI在短时间内表现出显著的变化.
- 太阳能活跃区域,特别是太阳黑子,在 TSI 波动中发挥着重要作用.
- 观察到的变异性表明,在活跃区域的太阳对流区内存在大量的能量储存.
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