太阳自转每隔11年受到行星系统反方向旋转切向力的作用

发布时间：2018-07-26 13:58

【摘要】：基于创建的行星会合指数(K)运动学方程,得到太阳绕太阳系质心绕转的真正周期为准22.1826年.在整个太阳系角动量守恒前提下,根据K指数所指代的太阳绕太阳系质心运动轨迹推出:太阳绕转和太阳自转各自角动量虽不守恒,但二者角动量之和守恒.当行星系统处于最大相背离状态,太阳自转角动量增加,太阳自转受到逆时针方向旋转切向力的作用;当行星系统处于最大会合状态,太阳自转角动量减小,太阳自转受到顺时针方向旋转切向力的作用.行星系统远日4颗大质量行星和近日4颗小质量行星对太阳引力的合力沿太阳绕转轨道半径垂直方向的分力,具有准22年周期变化,而且该力的方向就是沿太阳旋转运动轨迹的切向方向.该分力11年与太阳自转方向同向,另11年与太阳自转方向反向,且分别对应太阳自转角动量11年增大和11年减小的变化.这为研究太阳22年磁周期动力学机制探寻到一种新的思想方法.
[Abstract]:Based on the (K) kinematics equation of the planetary rendezvous exponent, the true period of the sun orbiting around the center of mass of the solar system is obtained, which is quasi-22.1826 years. On the premise of the conservation of angular momentum in the whole solar system, according to the orbit of the motion of the sun around the center of mass of the solar system referred to by the K exponent, it is deduced that the sum of the angular momentum of the solar rotation and the solar rotation is not conserved, but the sum of the angular momentum of the two is conserved. When the planetary system is in the maximum phase deviation state, the solar rotation angular momentum increases, the solar rotation is affected by the counterclockwise rotation tangential force, and when the planetary system is in the maximum convergence state, the solar rotation angular momentum decreases. The rotation of the sun is subjected to a clockwise rotating tangential force. The combined forces of the four massive planets and the four perihelion planets on the sun's gravitational force perpendicular to the radius of the sun's orbiting orbit have a quasi-22 year period. And the direction of the force is the tangential direction along the track of the sun's rotation. The component force is in the same direction as the sun's rotation direction for 11 years and opposite to the solar rotation direction for the other 11 years, and corresponds to the increase of the solar rotation angular momentum for 11 years and the decrease of the solar rotation angular momentum for 11 years, respectively. This provides a new method for studying the dynamical mechanism of the solar magnetic period in 22 years.
【作者单位】：齐齐哈尔大学理学院地理系;南京师范大学地理科学学院;中科院南京地理与湖泊研究所湖泊与环境国家重点实验;
【基金】：国家自然科学基金(41101372,41271204) 江苏高校优势学科建设工程资助项目(164320H101) 国家自然科学基金青年基金(41301215) 江苏省自然科学基金(BK20131058)联合资助
【分类号】：P182.1

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