Imaging methods and improvements for the cislunar orbit ultralong wavelength satellite array

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Key Points

To explore the imaging methods for the cislunar orbit ultralong wavelength satellite array aimed at high-resolution astronomical observations.
Review of imaging techniques suitable for a satellite array in cislunar orbit.
Consideration of unique characteristics such as all-day field of view and three-dimensional dynamic baselines.
Analysis of computational demands and algorithm efficiency for handling large data volumes.
Potential for acquiring high-resolution images below 30 MHz, offering new insights into ultralong wave astronomical sources.
Identification of challenges in traditional imaging technologies due to the dynamic nature of the lunar environment.
Emphasis on the need for advanced algorithms capable of high-speed processing for large datasets.

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Review of imaging methods for ultralong wavelength detection in cislunar orbit, highlighting the advancements in space radio astronomy.

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Xuelei et al. (2026) studied this question.

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