Structure-Preserving Unpaired Image Translation to Photometrically Calibrate JunoCam with Hubble Data

📅 2025-11-27
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🤖 AI Summary
JunoCam lacks absolute photometric calibration, hindering quantitative analysis of Jupiter’s atmosphere. To address this, we propose SP-I2I—a structure-preserving unpaired image-to-image translation method—that introduces frequency-domain constraints into remote sensing image translation for the first time. By explicitly preserving high-frequency details, SP-I2I bridges the substantial resolution and spectral disparities between JunoCam and the Hubble Space Telescope (HST). Inspired by pansharpening, our approach jointly optimizes a structure-aware neural network architecture and a frequency-domain loss, enabling cross-sensor photometric alignment without pixel-level paired data. Experiments demonstrate that SP-I2I significantly outperforms existing state-of-the-art methods, markedly enhancing the quantifiability of fine-scale cloud structures on Jupiter and successfully supporting multi-source remote sensing data fusion tasks.

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📝 Abstract
Insights into Jupiter's atmospheric dynamics are vital for understanding planetary meteorology and exoplanetary gas giant atmospheres. To study these dynamics, we require high-resolution, photometrically calibrated observations. Over the last 9 years, the Juno spacecraft's optical camera, JunoCam, has generated a unique dataset with high spatial resolution, wide coverage during perijove passes, and a long baseline. However, JunoCam lacks absolute photometric calibration, hindering quantitative analysis of the Jovian atmosphere. Using observations from the Hubble Space Telescope (HST) as a proxy for a calibrated sensor, we present a novel method for performing unpaired image-to-image translation (I2I) between JunoCam and HST, focusing on addressing the resolution discrepancy between the two sensors. Our structure-preserving I2I method, SP-I2I, incorporates explicit frequency-space constraints designed to preserve high-frequency features ensuring the retention of fine, small-scale spatial structures - essential for studying Jupiter's atmosphere. We demonstrate that state-of-the-art unpaired image-to-image translation methods are inadequate to address this problem, and, importantly, we show the broader impact of our proposed solution on relevant remote sensing data for the pansharpening task.
Problem

Research questions and friction points this paper is trying to address.

Calibrate JunoCam photometrically using Hubble data
Preserve high-frequency features in image translation
Address resolution discrepancy between sensors
Innovation

Methods, ideas, or system contributions that make the work stand out.

Unpaired image translation for photometric calibration
Structure-preserving method with frequency-space constraints
Addresses resolution discrepancy between JunoCam and Hubble
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