论文标题
关于有节奏的太阳半径变化的起源
On the origin of the rhythmic Sun's radius variation
论文作者
论文摘要
太阳在太阳能最大值期间缩小，在太阳能最小值期间再生几公里。我们在这里首次观察到太阳半径变化显示了行星关系。这表明必须存在一些远程行星链接，即使这在已知的物理学中是出乎意料的。因此，我们推测其原因，这是这项调查背后的驱动想法。也就是说，它必须是黑暗宇宙中的一些通用流媒体物质。相关的能量变化是巨大的，尽管它从几个月延长到几年。随着时间的流逝，暂定无形的大规模物质的影响会累积，从而缓慢触发基础过程。这项研究表明，太阳大小的响应短达几个月。然后，假设来自黑暗部门，太阳系是仍然未识别的外部影响的目标和天线。
The Sun shrinks during solar maximum and regrows during solar minimum by a few kilometers. Here, we observe, for the first time, that the solar radius variation shows planetary relationship. This suggests that some remote planetary links must exist, even though this is unexpected within known physics. Therefore, we speculate about its cause, which is the driving idea behind this investigation. Namely, it must be some generic as yet invisible streaming matter from the dark Universe. The associated energy change is massive although it extends from months to several years. The impact by the tentative invisible massive matter accumulates with time, triggering slowly the underlying processes. This study shows that the sun size response is as short as a few months. Then, the solar system is the target and the antenna of still unidentified external impact, assuming to be from the dark sector.
