Exploring the influence of Turbulence Models on the planetary wind field prediction values of optical sensing satellites

YU-HSUAN HUANG^1*

¹Department of Chinese Literature, National Chung Hsing University, Taichung, Taiwan

* Presenter:YU-HSUAN HUANG, email:fortune2262@gmail.com

The objective of this study is to use the long-range plan for space technology development of the National Space Center of the National Experimental Research Institute as the front guide to verify the planetary wind coefficient value affected by Turbulence Models.The method is Wolfram Mathematica, Python, and PlotDB. Open data such as data Seismometer to Investigate Ice and Ocean Structure; Turbulence Models: Data from Other Experiments: FAITH Hill 3-D Separated Flow; DAO V4 Late Look Special Subset Daily Global Climatology.The results of the study are based on planetary physics and quantum metrology to derive the circumscribed sphere radius of the decision tree numerical space; the circumscribed sphere area equation; the inscribed sphere radius formula; the inscribed sphere area formula; the two sphere radius difference formula; the two sphere area difference formula .The conclusion of the study is to learn the two-plane infrastructure formula of planetary physics as the theorem output of this paper. The two theorem is derived from the decision tree algorithm to determine the cosmological model that can be optimized by Turbulence Models.

Keywords: optoelectronics, astrophysics, cosmology, planetary science, Multiverse