摘要
本文对1980年SMM(峰年卫星)/ACRIM日射计观测的太阳常数与伴有快速变化的异常磁结构黑子群面积进行了比较分析,结果表明:当日面出现伴有快速变化的异常磁结构黑子群时,太阳常数减少。另一方面,当结构简单的“剩余”黑子群占优势时,太阳常数值轻微地增加。
The comparation of the values of solar contain obtained by the SMM/ACRIM radiometer and the areas of the sunspot groups with fast variation and abnormal magnetic configuration was made in this paper. The result shows that the values of the solar constant decrease when this kind of sunspot group exists on the solar disk; on the other hand, the values of the solar constant increase when the 'remaining' sunspot group with simple magnetic configuration dominates on the solar disk.
关键词
太阳
常数
黑子群
Sun (the)-Solar constant-Sunspot groups