深空探测学报
深空探測學報
심공탐측학보
Journal of Deep Space Exploration
2014年
3期
210-213
,共4页
尖晶石%光谱特征%Hapke 模型%太空风化
尖晶石%光譜特徵%Hapke 模型%太空風化
첨정석%광보특정%Hapke 모형%태공풍화
spinel%spectral feature%Hapke model%space weathering
简要介绍了不同太空风化条件下尖晶石的光谱特性,特别是利用 Hapke 模型计算了不同太空风化条件下尖晶石的二向性反射率分布特征。模拟的结果显示,对 M3数据,可比较0.6μm 和1.9μm 附近的吸收特征;对 IIM 数据,则需要先分析太空风化程度,然后比较0.6μm 和0.9μm 附近的吸收特征来判断是否为尖晶石。该结论为选择探月传感器的波段组合识别尖晶石提供了依据,也为应用 M3数据和“嫦娥1号”IIM 数据的尖晶石判别奠定了基础。
簡要介紹瞭不同太空風化條件下尖晶石的光譜特性,特彆是利用 Hapke 模型計算瞭不同太空風化條件下尖晶石的二嚮性反射率分佈特徵。模擬的結果顯示,對 M3數據,可比較0.6μm 和1.9μm 附近的吸收特徵;對 IIM 數據,則需要先分析太空風化程度,然後比較0.6μm 和0.9μm 附近的吸收特徵來判斷是否為尖晶石。該結論為選擇探月傳感器的波段組閤識彆尖晶石提供瞭依據,也為應用 M3數據和“嫦娥1號”IIM 數據的尖晶石判彆奠定瞭基礎。
간요개소료불동태공풍화조건하첨정석적광보특성,특별시이용 Hapke 모형계산료불동태공풍화조건하첨정석적이향성반사솔분포특정。모의적결과현시,대 M3수거,가비교0.6μm 화1.9μm 부근적흡수특정;대 IIM 수거,칙수요선분석태공풍화정도,연후비교0.6μm 화0.9μm 부근적흡수특정래판단시부위첨정석。해결론위선택탐월전감기적파단조합식별첨정석제공료의거,야위응용 M3수거화“항아1호”IIM 수거적첨정석판별전정료기출。
This paper briefly introduces the bidirectional reflectance feature of spinel based on space weathering. The distribution of the bidirectional reflectance feature of spinel under the different conditions of space weathering was simulated using the Hapke model.The results show that the absorption features at 0.6μm and 1.9μm could be used to determine spinel when the Moon Mineralogy Mapper (M3 )data is applied.However,when the Chang’e-1 Interference Imaging Spectrometer (IIM)data is used,the space weathering level should be first analyzed,and then the absorption features at 0.6 μm and 0.9 μm could be applied to identify the mineral.These results provide the basis of identifying spinel using absorptive positions and depths of the spinel,which can also be applied to M3 data and Chang’e-1 IIM data processing.