Moon‑based measurements provide planet‑scale, noise‑reduced radiation data, enhancing climate model fidelity and long‑term monitoring capabilities.
Understanding Earth’s radiation budget is central to climate science, yet conventional low‑Earth‑orbit and geostationary satellites struggle with gaps in temporal coverage and spatial consistency. These platforms view only narrow swaths, requiring complex stitching to reconstruct a global picture, which introduces uncertainties especially when trying to isolate planet‑scale signals from regional weather fluctuations. The lunar perspective eliminates many of these constraints by offering a stable, disk‑integrated view that captures the entire illuminated hemisphere in a single frame, delivering continuous, homogeneous data ideal for long‑term trend analysis.
The Chinese Academy of Sciences team leveraged this advantage by employing spherical harmonic decomposition on the moon‑based radiance measurements. Their analysis revealed that first‑ and second‑order harmonics account for about ninety percent of the observed variability, effectively acting as a natural filter that suppresses high‑frequency weather noise. Moreover, the study mapped distinct periodic signatures: synodic‑month cycles driven by lunar phases, sidereal‑month and half‑month patterns tied to the Moon’s orbital latitude shifts, and intraday fluctuations reflecting Earth’s rotation. This harmonic fingerprint not only clarifies the underlying physics of Earth’s emitted energy but also provides a robust framework for comparing satellite and lunar datasets.
The implications for climate monitoring are profound. A noise‑reduced, planet‑scale radiation record can refine estimates of Earth’s energy imbalance, a key metric for assessing global warming trajectories. Integrating lunar observations with existing satellite constellations could improve model initialization, reduce uncertainty in climate projections, and support international climate‑policy assessments. As lunar missions become more frequent and cost‑effective, the prospect of a dedicated, long‑duration lunar radiometer network offers a compelling path toward continuous, high‑fidelity climate surveillance.
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