arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 0906.4371physics.gen-phphysics.space-ph
收藏

用冲击波解释太阳黑子的起源来解释太阳活动的行星效应

Impact Generated Shockwaves are Proposed for the Origin of Sunspots to Explain the Detected Planetary Effects on the Solar Activity

Jozsef Garai

摘要:

发现了太阳黑子活动与类木行星轨道位置之间的五种新的相关性。为了解释这些相关性,有人提出,外行星的共振使柯伊伯带天体的轨道不稳定,并产生了对太阳的周期性撞击频率。该物体的蒸发启动了一个冲击波,破坏了等离子体的上涌,导致太阳黑子的形成。该模型能够解释太阳活动周期的长度、黑子的纬度分布以及太阳活动周期的长期稳定性。计算木星行星在合相和冲相时的位置可以对太阳活动进行长期预测。

英文摘要:

Five new correlations between sunspot activity and orbiting position of the Jovian planets are detected. In order to explain these correlations it is suggested that the resonance of the outer planets destabilizes the orbit of Kuiper Belt Objects and generates a cyclical impact frequency on the Sun. The vaporization of the object initiates a shock way disrupting the upwelling of the plasma resulting in a sunspot formation. The proposed model is able to explain the length of the cycle, the latitude distribution of the sunspots and the extremely long term stability of the cycles. Calculating the positions of the Jovian planets at conjunction and opposition allows the long term prediction of the solar activity.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑