Articles | Volume 35, issue 3
https://doi.org/10.5194/angeo-35-659-2017
https://doi.org/10.5194/angeo-35-659-2017
Regular paper
 | 
17 May 2017
Regular paper |  | 17 May 2017

Contrast analysis between the trajectory of the planetary system and the periodicity of solar activity

Wei Sun, Jian Wang, JinRu Chen, Ying Wang, GuangMing Yu, and XianHai Xu

Abstract. The relationship between the periodic movement of the planetary system and its influence on solar activity is currently a serious topic in research. The kinematic index of the planet juncture index has been developed to find the track and variation of the Sun around the centroid of the solar system and the periodicity of solar activity. In the present study, the kinematic index of the planetary system's heliocentric longitude, developed based on the orbital elements of planets in the solar system, and it is used to investigate the periodic movement of the planetary system. The kinematic index of the planetary system's heliocentric longitude and that of the planet juncture index are simulated and analyzed. The numerical simulation of the two kinematic indexes shows orderly orbits and disorderly orbits of 49.9 and 129.6 years, respectively. Two orderly orbits or two disorderly orbits show a period change rule of 179.5 years. The contrast analysis between the periodic movement of the planetary system and the periodicity of solar activity shows that the two phenomena exhibit a period change rule of 179.5 years. Moreover, orderly orbits correspond to high periods of solar activity and disorderly orbits correspond to low periods of solar activity. Therefore, the relative movement of the planetary system affects solar activity to some extent. The relationship provides a basis for discussing the movement of the planetary system and solar activity.

Download
Short summary
In this study, the kinematic index of planet heliocentric longitude is created based on the orbital elements of planets in the solar system. Both the planet juncture index and heliocentric longitude are used to investigate the periodic planetary system movement around the mass center of the solar system. The kinematic index of planet heliocentric longitude represents the exact location of the barycenter of the planetary system relative to that of the solar system.