利用高分辨率 Chandrayaan-2 DFSAR 数据确定月球南极附近 Chandrayaan-3 着陆场的极地特征

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Planetary and Space Science Pub Date : 2024-08-28 DOI:10.1016/j.pss.2024.105956
Tathagata Chakraborty, Dharmendra Kr. Pandey, Raghav Mehra, Parikshit Parasher, Deepak Putrevu, V.M. Ramanujam, Nilesh M. Desai
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引用次数: 0

摘要

Chandrayaan-3 号(CH3)维克拉姆着陆器为研究着陆点的雷达散射行为以及月球表面的人造斜面结构提供了一个独特的机会。月壤-2 号轨道飞行器搭载的双频合成孔径雷达(DFSAR)传感器使这一机会成为可能,与任何行星合成孔径雷达传感器相比,该传感器具有最高的分辨率和偏振测量能力。为了探索这一点,我们利用 DFSAR 以混合波尔模式捕获了 CH3 着陆场在着陆前和着陆后状态下的高分辨率图像,像素间距细至 1 米。着陆点表现出与理想二面体几何形状类似的主要体积和均匀反弹雷达散射行为。此外,我们观察到着陆点的圆偏振比值特别高(1.99 ± 0.30),这在月球表面的自然特征中非常罕见。此外,着陆点的平均介电常数值(5.76 ± 3.11)也有所提高。着陆后的 DFSAR 图像显示,CH3 着陆点周围有一个 177 平方米的区域,该区域的特点是 CPR 高、均匀反弹和体积散射高。与着陆前的 DFSAR 观测结果相比,着陆点的平均 CPR 值(7 倍)、介电常数值(2 倍)、均匀反弹和体积散射都急剧增加,这是因为着陆器模块的存在和着陆区域的岩石结构受到干扰。着陆点的极坐标特征将其与月球表面的主要自然特征(如碎屑岩、碎片流和撞击喷出物)区分开来。这项调查极为重要,因为它强调了高分辨率 DFSAR 采集在评估小尺度特征的极坐标行为方面的有效性,这对于在即将进行的飞行任务中确定着陆点的特征非常宝贵。
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Polarimetric characterization of Chandrayaan-3 landing site near lunar south pole using high resolution Chandrayaan-2 DFSAR data

The Chandrayaan-3 (CH3) Vikram lander presents an unique opportunity to study the radar scattering behavior of the landing site as well as human-made dihedral structure on the lunar surface. This opportunity is made possible by the Dual-Frequency Synthetic Aperture Radar (DFSAR) sensor onboard the Chandrayaan-2 orbiter, which has the highest resolution and polarimetric capabilities compared to any planetary SAR sensor. To explore this, we utilized DFSAR to capture high-resolution images of the CH3 landing site during pre-landing and post-landing condition, with a pixel spacing as fine as 1 m, in a hybrid-pol mode. The landing site exhibits dominant volume and even-bounce radar scattering behavior similar to an ideal dihedral geometry. Furthermore, we observed an exceptionally high Circular Polarization Ratio value at the landing site (1.99 ± 0.30), a rarity among natural features on the lunar surface. Besides, the landing site is characterized by enhanced average dielectric constant value (5.76 ± 3.11). The post-landing DFSAR image reveals a 177 m2 area, surrounding the CH3 landing location, characterized by high CPR and elevated even bounce and volume scattering. The drastic enhancement of the average CPR value (7-times), dielectric value (2-times), even bounce and volume scattering in the landing site, in comparison with the pre-landing DFSAR observation, is due to presence of lander module and disturbance in the regolith structure in the landing area. The polarimetric characteristics of the landing site distinguish it from the major natural features on the lunar surface, such as regolith, debris flow, and impact ejecta. This investigation is of utmost importance as it emphasizes the effectiveness of high-resolution DFSAR acquisitions for evaluating the polarimetric behavior of small-scale features, which can be invaluable for characterizing landing sites in upcoming missions.

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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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