概括
两次火箭飞行的测量表明,太阳发光率 (太阳常数) 增加了0.4%. 这种观察到的太阳亮度变化很可能是真实的,需要进一步调查其原因和潜在的气候影响.
科学领域:
- * 太阳物理学和大气科学.
- * 放射测量和仪器校准.
背景情况:
- * 精确测量太阳亮度对于理解地球气候和太阳变异性至关重要.
- *以前的研究已经探讨了短期太阳波动,但长期趋势需要精确,一致的测量.
研究的目的:
- * 通过使用绝对热仪在30个月的时间内评估太阳亮度的变化.
- *通过考虑仪器性能和校准来评估测量的可靠性.
主要方法:
- * 两次火箭飞行使用绝对热仪测量太阳辐射量.
- *评价仪器性能,并与其他气计进行飞行前和飞行后的对比.
主要成果:
- * 在两次飞行之间检测到太阳亮度 (太阳常数) 增加了0.4%.
- * 仪器对比表明,这种测量差异很可能是真正的太阳变化.
结论:
- * 观察到的太阳发光度的增加很可能是一个真正的现象.
- *需要进一步观察以确定这种变化是随机波动,短期事件,还是具有气候学意义的持续变化.
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