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Performance in Solar Orientation Determination for Regular Pyramid Sun Sensors.

Jiang Wang1, Yongchao Zhang2, Yin Zhang3

  • 1School of Communication and Information Engineering, University of Electronic Science and Technology of China, Chengdu 610054, Sichuan, China. rivers2000@163.com.

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PubMed
Summary
This summary is machine-generated.

This study introduces a novel frequency-domain method for precise solar orientation determination in spacecraft sun sensors. The new approach effectively suppresses interference, enhancing accuracy without adding size or mass.

Keywords:
regular pyramid arrayssolar orientationsun sensors

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Area of Science:

  • Spacecraft instrumentation
  • Attitude determination and control systems
  • Optical sensing technologies

Background:

  • Non-planar sun sensors utilize existing components to determine solar orientation, minimizing spacecraft size and mass.
  • Current limitations in accuracy stem from insufficient performance assessments of interference suppression techniques.

Purpose of the Study:

  • To develop a novel frequency-domain method for accurate solar orientation determination using regular pyramid sun sensors.
  • To establish formulations for evaluating solar azimuth and elevation angle errors in this new method.
  • To analyze the relationship between interference, sensor geometry, and orientation accuracy.

Main Methods:

  • Development of a frequency-domain solar orientation determination method for regular pyramid sun sensors.
  • Establishment of two error evaluation formulations for solar azimuth and elevation angles.
  • Mathematical analysis of interference spectrum, array geometry, solar irradiance, and angle errors.
  • Validation through simulations and field experiments.

Main Results:

  • A new frequency-domain method for solar orientation determination was successfully developed.
  • Formulations for error evaluation in solar azimuth and elevation angles were established.
  • The mathematical relationship between interference sources and orientation error was elucidated for the first time.
  • Internal detection system interference can be completely suppressed, and constant interference eliminated in azimuth estimation.

Conclusions:

  • The proposed frequency-domain method significantly enhances solar orientation accuracy in spacecraft.
  • The developed error formulations provide a robust tool for performance assessment and sensor design.
  • Interference suppression capabilities are mathematically defined, improving understanding of sensor limitations and performance.