Estimation of solar zenith passage on the Earth's surface by a simple harmonic motion
Paco Talero, Fernanda Santana y C\'esar Mora

TL;DR
This paper models the solar zenith passage on Earth as a simple harmonic motion using a uniform circular motion approach, comparing it with Stellarium data to validate the analytical model.
Contribution
It introduces a simple harmonic motion model for solar zenith passage based on Earth's rotation and compares it with software data for validation.
Findings
Uncertainty of about 1 day in the model's predictions
Model effectively describes solar zenith passage as simple harmonic motion
Provides a basis for further kinematic studies of Earth's solar interactions
Abstract
The kinematics of the Solar zenith passage on the Earth was shown as a simple harmonic motion. This analytical model used the uniform circular motion to describe the Earth's rotation relative to its axis and relative to the Sun, also this model considered the sunlight beams parallel and constant the obliquity of the ecliptic. We made a contrast between some data taken from of the software Stellarium 0.12.1 and the model, we obtained an uncertainty ; this result allow to project the model as an astronomical context conducive to develop the kinematics of simple harmonic motion.
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Taxonomy
TopicsSolar Radiation and Photovoltaics · Experimental and Theoretical Physics Studies · Solar and Space Plasma Dynamics
