毫米和亚毫米波长范围光度法测定表面起伏度的可能性

2007 International Kharkov Symposium Physics and Engrg. of Millimeter and Sub-Millimeter Waves (MSMW) Pub Date : 2007-06-25 DOI:10.1109/MSMW.2007.4294807

I. A. Dulova, Y. Kornienko, S. Skuratovskiy

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摘要

本文研究了分光光度法在毫米波和亚毫米波波长范围内测定行星表面起伏的可能性。本文考虑的是使用侧视雷达获取初始图像的情况，重点关注所获得的图像序列相对于所需浮雕的信息性问题。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Possibilities of Surface Relief Determination by Photometric Method in Millimeter and Submillimeter Wavelength Range

In this paper, possibilities of planet surface relief determination by photometric method in millimeter and submillimeter wavelength range were studied. Considered in this paper was the case where the initial images were acquired with a side-looking radar, focusing attention upon the issue of informativity of obtained image series relative to the relief desired.

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2007 International Kharkov Symposium Physics and Engrg. of Millimeter and Sub-Millimeter Waves (MSMW)

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