云海撞击盆地的恢复及其地质演化研究

研究月海撞击盆地,尤其是古老的月海撞击盆地,有助于深入认识月球乃至太阳系中两种动力学即内动力和外动力地质作用的演化过程,也是研究月球早期演化和现今状态的重要纽带。云海撞击盆地为古老的撞击盆地之一,形成于前酒海纪,在后期的内外动力地质作用下,盆地有很大程度的改造。为了恢复云海撞击盆地原貌,深入认识该地区的地质演化过程,本文利用了LRO宽角相机影像数据、LOLA地形数据和GRAIL重力数据等多种类型的遥感数据,开展了云海撞击盆地演化的研究。结果显示,云海盆地是由一次撞击事件形成,具中央隆起的三环结构的撞击盆地,三环直径分别约为740km、500km、340km,盆地中心约为16°W,21°S。云海撞击盆地事件破坏了该地区原始月壳结构,随后岩浆喷出或溢流充填在撞击盆地中形成云海,塑造了现今观察到的云海地形特征和重力异常特征。     

中亚干旱区马雷绿洲和于田绿洲LUCC演变对比研究

当前新疆与中亚国家的经济形势进入平稳发展的新时期,新疆在经济合作中的地位逐渐明晰,产业结构、资源条件等是开展合作的直接影响主因。利用遥感技术开展LUCC研究,可直观探讨自然和非自然因素对LUCC影响,为区域可持续发展提供决策依据。以土库曼斯坦马雷绿洲1976年、2001年、2010年和中国新疆于田绿洲1977年、2000年和2011年共6期TM和MSS影像为数据源,对中亚地区两个生态环境皆较脆弱的绿洲进行土地利用/覆被变化（LUCC）分析,对比研究干旱区绿洲LUCC,并分析其自然和非自然因素。在研究期间,马雷绿洲中轻度盐渍地变化最多,相对变化达到2.21,净变化速度为3.49%,面积下降最多的是沙漠类型,相对变化为-0.59,净变化速度为-2.60%;于田绿洲水体面积变化最多,相对变化为5.54,净变化速度达5.51%,沙漠面积也下降最多,相对变化为-0.97,净变化速度为-9.31%。结果表明：（1）马雷绿洲和于田绿洲具有相似的地类变化趋势：耕地、中轻度盐渍地、其它地类面积有所增加,而林地、重度盐渍地、沙漠面积减少;（2）LUCC是由自然因素和非自然因素共同作用引起的。     

Evidence for Late Messinian seismites,Nijar Basin,south‐east Spain

The Feos Formation of the Nijar Basin comprises sediments deposited during the final stage of the Messinian salinity crisis when the Mediterranean was almost totally isolated. Levels of soft‐sediment deformation structures occur in both conglomeratic alluvial sediments deposited close to faults and the hyposaline Lago Mare facies, a laminated and thin‐bedded succession of whitish chalky marls and intercalated sands alternating with non‐marine coastal plain deposits. Deformation structures in the coarse clastics include funnel‐shaped depressions filled with conglomerate, liquefaction dykes terminating downwards in gravel pockets, soft‐sediment mixing bodies, chaotic intervals and flame structures. Evidence for soft‐sediment deformation in the fine‐grained Lago Mare facies comprises syndepositional faulting and fault‐grading, sandstone dykes, mixed layers, slumping and sliding of sandstone beds, convolute bedding, and pillar and flame structures. The soft‐sediment deformed intervals resemble those ascribed elsewhere to seismic shaking. Moreover, the study area provides the appropriate conditions for the preservation of deformation structures induced by seismicity; such as location in a tectonically active area, variable sediment input to produce heterolithic deposits and an absence of bioturbation. The vertical distribution of soft‐sediment deformation implies frequent seismic shocks, underlining the importance of seismicity in the Betic region during the Late Messinian when the Nijar Basin became separated from the Sorbas Basin to the north. The presence of liquefied gravel injections in the marginal facies indicates strong earthquakes (M ≥ 7). The identification of at least four separate fissured levels within a single Lago Mare interval suggests a recurrence interval for large magnitude earthquakes of the order of millennia, assuming that the cyclicity of the alternating Lago Mare and continental intervals was precession‐controlled. This suggestion is consistent with the present‐day seismic activity in SE Spain.     

基于粗糙度的雨海地形及撞击坑特征分析

以月球雨海地区为研究区,利用Matlab编程语言,结合分辨率为118 m的DEM数据,得出了该地区的均方根高程及均方根偏差分布图,并在研究区内选取18条剖面线,对其进行多种粗糙度参数计算。结果表明雨海地区粗糙度较大的区域主要分布在环形山和撞击坑等区域,粗糙度较小值则主要分布在被火山熔岩流填充的平原等区域,可以确定在百米尺度上环形山和撞击坑是影响雨海地形粗糙度的重要因素。对单个撞击坑而言,坑壁粗糙度最大,坑缘次之,坑底较为平坦,粗糙度最小。坑底粗糙度增大的现象可初步推断该撞击坑存在中央峰。     

月球富钛玄武岩喷发对月球生热元素丰度的约束

近几十年来,对月球的遥感观测以及对月岩样品的分析揭示了月海玄武岩、镁铁质月球玻璃等的时间和空间分布特征,其被认为与月幔的热化学演化密切相关,并且引出了许多解释模型.本文考虑月球结晶末期在上部形成的致密的钛铁矿层和下部的月幔,由于密度原因钛铁矿层发生倒转,之后受热上涌产生玄武质岩浆等的演化过程,从热化学演化的角度为月海玄...     

月球重力异常的小波多尺度分析

本文将小波多尺度分析引入月球重力场的研究,选取测量数据质量较好的月球近区作为实验区域,以“Clementine”探测器获得的自由空气重力异常作为原始数据对主要月海盆地进行了局部的重力异常分解,解释了月球内部基本分层结构,并利用主要月海盆地的实验结果分析了月海下部质量异常以及莫霍面的起伏形态,与已有研究成果进行比较证明了方法的适用性及结果的合理性.     

Lago Mare and the Messinian Salinity Crisis: Evidence from the Alboran Sea (S. Spain)

This paper provides a new environmental, sedimentological and stratigraphic context of the Lago Mare deposits from the North Alboran region and clarifies their chronologic location with respect to the Messinian Salinity Crisis. We present new micropalaeontological data (dinoflagellate cysts, calcareous nannoplankton, planktonic foraminifers), correlated with field observations and offshore seismic interpretations. We show that the Lago Mare event known in three onshore localities (Río Mendelín near Malaga, Zorreras near Sorbas, Gafares near Níjar) follows the marine reflooding of the Mediterranean Basin which ended the Messinian Salinity Crisis. Chronologically, these Lago Mare deposits last from the latest Messinian to the early Zanclean. In fact, the first influx of Paratethyan organisms is revealed by the dinoflagellate cyst record from near Malaga within a Gilbert-type fan delta overlying the Messinian Erosional Surface. Invading molluscs and/or ostracods may have persisted in lagoonal coastal areas more or less affected by discontinuous marine influxes (Sorbas and Níjar). The Malaga area is convenient for a palaeogeographic and sedimentary reconstruction which shows the prevalent forcing of sea-level changes during the time-interval 5.600–5.332 Ma at the difference of the usually solicited prevalent tectonics. The studied Lago Mare event is the third episode resulting in such a palaeobiological assemblage in the Mediterranean region and corresponds to the final two-way water exchange at high sea level between the Mediterranean and the former Paratethys. It documents the onset of the modern marine circulation in the Mediterranean after the reflooding ending the Messinian Salinity Crisis.     

基于DEM的月球雨海地区粗糙度研究

月球表面粗糙度是揭示月表地貌形态空间分异特征的重要指标,并在一定程度上映射月表地貌的形成与演化机理。运用基于中国“嫦娥一号”卫星获取的DEM数据,提取月球雨海地区的月表粗糙度,并在月球正面地质图数据辅助下,分析月表粗糙度分布特征及其与地质单元岩性以及地质年龄的关系。结果显示:月球雨海地区的粗糙度与地质单元岩性存在较强相关关系,且随着地质年龄的增长,玄武岩单元的粗糙度呈现增大的趋势。此外,在小于7 km的尺度范围内,雨海地区受持续撞击作用的影响,Hurst指数分布在0.7~0.9之间,地形较为粗糙;在更大尺度上,由于受到火山熔岩流充填机制的控制,Hurst指数不断减小,地形不断趋于平缓。     

Reflectance spectra of analog basalts; implications for remote sensing of lunar geology

Lunar mare basalts, highland anorthosites and KREEP are the three major lunar rock types reported from the lunar surface. In the present study, we interpret the reflectance spectral behavior of lunar analog basalts including massive basalt, vesicular basalt and amygdaloidal basalt collected from the Deccan basaltic region, which are considered as equivalent of lunar mare basalts. Reflectance spectra of analog basalts were measured at three different environments: in the field, under controlled field conditions and in the lab. In field conditions the reflectance spectra were measured under 350-1050 nm spectral range. During controlled field and lab condition, reflectance spectra were measured under 350-2500 nm range covering the UV, visible, NIR, and SWIR regions. The spectral characteristics of basalts measured under different environments and their merits and demerits were discussed. However, lab spectra have given clear, reliable diagnostic spectral information for our present objective. The major oxides and minerals of analog basalts were compared with lunar mare basalts. The presence of Ca-pyroxene, ferrous and ferric iron and their diagnostic spectral features in basalts are discussed for study of lunar mare region.