Virtual Sensing Model for Power Prediction of Satellite Solar array: J₂ Perturbation Dynamics Resolution via Dual-Coordinate Transformation and Adaptive Runge-Kutta

This model resolves <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">${J} _{{2}}$ </tex-math></inline-formula> perturbation orbital dynamics equations via dual-coordinate transformation, utilizing the Earth-centered inertial (ECI) coordinate system for orbital dynamics and the geocentric solar ecliptic (GSE) system for solar vector alignment. Adaptive Runge–Kutta integral solution for ordinary differential equations (ODEs) converts initial orbital parameters into continuous power profiles to achieve high-precision and long-term forecasting for satellite solar arrays with replacing physical measurements. To mitigate the error accumulation issue inherent in conventional methods that overlook orbital perturbations, the proposed model integrates <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">${J} _{{2}}$ </tex-math></inline-formula> perturbation effects to refine orbital parameters and utilizes an adaptive Runge–Kutta algorithm to effectively resolve satellite attitude dynamics. The use of dual-coordinate transformation and decoupled dynamics analysis substantially reduces computational complexity. Additionally, an equivalent power model for solar array under illumination and eclipse conditions is developed based on a cylindrical projection method, enabling rapid calculations in complex lighting environments. The experimental results indicate that the proposed method achieves long-term power forecasting using only initial orbital parameters, obviating the need for professional tools or frequent data updates. Compared to traditional two-body models, this approach demonstrates significant advantages in computational efficiency (requiring only one-third of STK’s runtime) and prediction accuracy (achieving a 60% reduction in mean squared error), thereby providing reliable theoretical support for dynamic power management and mission planning in satellite energy systems.

Authors

Publication Details

Journal
IEEE Sensors Journal
Published
2025-01-01
DOI
https://doi.org/10.1109/jsen.2025.3596233
Primary Topic
Inertial Sensor and Navigation
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Virtual Sensing Model for Power Prediction of Satellite Solar array: J₂ Perturbation Dynamics Resolution via Dual-Coordinate Transformation and Adaptive Runge-Kutta

Shuiwang Duan, Xianrui Zeng, Ying Peng, He Liu et al.
IEEE Sensors Journal
Inertial Sensor and Navigation
article

Virtual Sensing Model for Power Prediction of Satellite Solar array: J₂ Perturbation Dynamics Resolution via Dual-Coordinate Transformation and Adaptive Runge-Kutta

Shuiwang Duan, Xianrui Zeng, Ying Peng, He Liu, Mao Li, Wenhao Geng
article en

Abstract

This model resolves <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">${J} _{{2}}$ </tex-math></inline-formula> perturbation orbital dynamics equations via dual-coordinate transformation, utilizing the Earth-centered inertial (ECI) coordinate system for orbital dynamics and the geocentric solar ecliptic (GSE) system for solar vector alignment. Adaptive Runge–Kutta integral solution for ordinary differential equations (ODEs) converts initial orbital parameters into continuous power profiles to achieve high-precision and long-term forecasting for satellite solar arrays with replacing physical measurements. To mitigate the error accumulation issue inherent in conventional methods that overlook orbital perturbations, the proposed model integrates <inline-formula xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink"> <tex-math notation="LaTeX">${J} _{{2}}$ </tex-math></inline-formula> perturbation effects to refine orbital parameters and utilizes an adaptive Runge–Kutta algorithm to effectively resolve satellite attitude dynamics. The use of dual-coordinate transformation and decoupled dynamics analysis substantially reduces computational complexity. Additionally, an equivalent power model for solar array under illumination and eclipse conditions is developed based on a cylindrical projection method, enabling rapid calculations in complex lighting environments. The experimental results indicate that the proposed method achieves long-term power forecasting using only initial orbital parameters, obviating the need for professional tools or frequent data updates. Compared to traditional two-body models, this approach demonstrates significant advantages in computational efficiency (requiring only one-third of STK’s runtime) and prediction accuracy (achieving a 60% reduction in mean squared error), thereby providing reliable theoretical support for dynamic power management and mission planning in satellite energy systems.

IEEE Sensors Journal
Affordable and clean energy, Climate action
Openalex Percentile: Top 72%
Inertial Sensor and Navigation
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.