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Kilho Baek

Publications and source records attributed to Kilho Baek.

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On-Orbit Calibration of Danuri/PolCam. II. Radiometric Calibration

Danuri, South Korea's first lunar orbiter, was launched on August 5, 2022, and has successfully operated its two-year nominal mission phase. The wide-angle Polarimetric Camera (PolCam) onboard Danuri is the first instrument to conduct global polarimetric observations from lunar orbit. This paper presents the comprehensive radiometric calibration pipeline for PolCam's on-orbit data, consisting of dark current removal, smear correction, and flat-fielding. Notably, PolCam's raw data exhibit severe smear artifacts induced by the frame-transfer CCD architecture, which significantly degrade both radiometric fidelity and the accuracy of polarimetric measurements. These smear artifacts have been effectively mitigated through a rigorous correction algorithm, restoring data quality to a level sufficient for scientific analysis and facilitating the precise derivation of the degree of linear polarization (DoLP). Finally, we present representative examples of polarimetric measurements to validate calibration performance. Although the current calibration focuses on restoring data quality for qualitative scientific analysis, these results clearly demonstrate the expected inverse relationship between intensity and polarization. The absolute photometric calibration required for quantitative DoLP analysis is reserved for a subsequent publication.

astro-ph.IM

On-Orbit Calibration of Danuri/PolCam. I. Geometric Calibration

The wide-angle Polarimetric Camera (PolCam) onboard South Korea's first lunar orbiter, Danuri, is a pioneering instrument designed to conduct the first global polarimetric and high-phase-angle survey of the Moon. Precise geometric calibration is critical for this mission, particularly due to PolCam's highly oblique viewing geometry, which introduces significant topographic distortion. We present a comprehensive on-orbit geometric calibration that relies on 160,256 tie points derived from matching features between PolCam images and the well-orthorectified global map of the Kaguya Multiband Imager (MI). This dataset allows us to address two fundamental challenges: (1) the accurate reconstruction of the observation time for each line of an observation strip via a simple linear model, and (2) the refinement of the precise camera model, geometric model for PolCam optics. Our optimization method for these two challenges transforms the 2D image coordinates of identified features into 3D lunar coordinates and minimizes the reprojection error against the reference coordinates provided by the Kaguya MI map. From the refined observation time and camera model, we compute the precise longitude, latitude, and elevation of each pixel of an observed image. These estimated 3D coordinates are then used to generate orthorectified images, the final product of the geometric calibration. The resulting calibration achieves a geometric precision comparable to that of previous lunar orbiters and establishes the foundational framework necessary to produce geometrically-corrected data products of PolCam.

astro-ph.EP