The light curve of asteroid 2867 Steins measured by VIRTIS-M during the Rosetta fly-by     

F. Tosi  A. Coradini  G. Filacchione  M.C. De Sanctis  M.A. Barucci  S. Mottola  E. Dotto  The VIRTIS Team 《Planetary and Space Science》2010,58(9):1066-1076

On 5 September 2008, the Rosetta spacecraft encountered the asteroid 2867 Steins on its way to the comet 67P/Churyumov-Gerasimenko. This was the first of two planned asteroid fly-bys performed by the probe, the second fly-by being with the much larger asteroid 21 Lutetia in July 2010. The VIRTIS imaging spectrometer (IFOV 0.250 mrad, overall spectral range 0.25-5.1 μm) onboard Rosetta acquired data of Steins already before the closest approach phase, when the target was spatially unresolved, in order to obtain a light curve of the asteroid in the infrared spectral range extending up to 5 μm, that was never explored before. The VIRTIS light curve campaign started at 11:30 UTC onboard time, when the spacecraft was about 221,377 km away from the target, and ended at 17:58 UTC, at a distance of 20,741 km away from Steins. During this timeframe, the solar phase angle of the asteroid was roughly constant, ranging from 38.2° to 36.3°.Assuming the most recent value derived for the rotational period of Steins (Lamy et al., 2008), the VIRTIS observations covered slightly more than one rotation of the asteroid. In this interval, VIRTIS collected 8 hyperspectral cubes where Steins was captured 119 times, both in the visual and in the infrared range. Given the low signal and the unresolved appearance of the source, for which the instrument was not designed, only a small subset of wavelengths turned out to be suitable to sample the light curve. Nevertheless, in both the VIS and NIR ranges we find a similar trend, with two different maxima and minima during one rotational period, and amplitudes consistent with the results in the visual range obtained in previous works, including the data set acquired by the OSIRIS camera onboard Rosetta. We also report the presence of a new broad feature centered at approximately 0.81-0.82 μm, which is seen in the visual data throughout the rotation of the asteroid.  相似文献   

Abundances of Jupiter's trace hydrocarbons from Voyager and Cassini     

C.A. Nixon  R.K. Achterberg  P.N. Romani  X. Zhang  P.G.J. Irwin 《Planetary and Space Science》2010,58(13):1667-1680

The flybys of Jupiter by the Voyager spacecraft in 1979, and over two decades later by Cassini in 2000, have provided us with unique datasets from two different epochs, allowing the investigation of seasonal change in the atmosphere. In this paper we model zonal averages of thermal infrared spectra from the two instruments, Voyager 1 IRIS and Cassini CIRS, to retrieve the vertical and meridional profiles of temperature, and the abundances of the two minor hydrocarbons, acetylene (C₂H₂) and ethane (C₂H₆). The spatial variation of these gases is controlled by both chemistry and dynamics, and therefore their observed distribution gives us an insight into both processes. We find that the two gases paint quite different pictures of seasonal change. Whilst the 2-D cross-section of C₂H₆ abundance is slightly increased and more symmetric in 2000 (northern summer solstice) compared to 1979 (northern fall equinox), the major trend of equator to pole increase remains. For C₂H₂ on the other hand, the Voyager epoch exhibits almost no latitudinal variation, whilst the Cassini era shows a marked decrease polewards in both hemispheres. At the present time, these experimental findings are in advance of interpretation, as there are no published models of 2-D Jovian seasonal chemical variation available for comparison.  相似文献   

Gemini-N mid-IR observations of the dust properties of the ejecta excavated from Comet 9P/Tempel 1 during Deep Impact     

David E. Harker  Charles E. Woodward  R. Scott Fisher 《Icarus》2007,190(2):432-453

We present mid-infrared spectra and images from the Gemini-N (+MICHELLE) observational campaign of Comet 9P/Tempel 1 before, during, and after its encounter with Deep Impact. We use our thermal grain model to probe the 10 μm properties of the dust grains in the coma of the comet. Before impact (3 July 2005 UT), and more than 24 h after impact (5, 16, and 28 July 2005 UT), the comet dust grains were composed mostly of amorphous olivine, and were relatively large (peak of the grain size distribution ). For the night of impact, we extract spectra by centering on the nucleus, and offset 1″ from the nucleus in the direction of the impact ejecta plume. We find small dust grains (∼0.2 μm) of a diverse mineralogy (amorphous olivine, amorphous pyroxene, amorphous carbon, and crystalline olivine) populating the ejecta. The submicron sized dust grains move faster than the other, larger grains (?0.7 μm), with amorphous olivine and amorphous carbon traveling together, and amorphous pyroxene and crystalline olivine dispersing at a similar rate. Deriving a velocity law from a time-of-flight analysis, we find that the material traveled with a velocity law scaled by and with a power of p=0.5. This velocity power-law requires a sustained release of grains for the duration of 45-60 min after impact. Since the mineral species are traveling at different speeds, and there was a sustained release of grains due to a possible “gas-plume,” we conclude that the different minerals did not originate from grain aggregates destroyed by the impact, but instead arise from an inhomogeneous nucleus.  相似文献   

Integration of intensity textures and local geometry descriptors from Terrestrial Laser Scanning to map chert in outcrops     

《ISPRS Journal of Photogrammetry and Remote Sensing》2014

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高精度住房空置率的地理空间影响因素定量研究     

张栋  李德平  周亮  王嘉丞  马宇  易敏 《测绘通报》2022,(2):100-105

为揭示住房空置率对地理空间因素的依赖性,本文首先以50 m×50 m格网为基本单位,通过建模等方式计算格网尺度的住房空置率、自然因子、社会因子,然后对研究区进行不同级别的划分和相关性分析,最后采用地理探测器法对自然因子的影响机制进行进一步研究。结果表明：①研究区住房空置率与所选地理空间因子均呈显著性相关,植被占比对住房空置率的影响程度最大,其他自然因子的影响程度普遍偏小;②由于非建成区尚处于快速发展阶段,有较大的发展潜力,因此非建成区对于社会因子和自然因子的依赖程度均大于建成区;③各街道的住房空置率受坡度的影响程度普遍小于其他自然因子,各因子两两之间的交互作用对住房空置率的解释力具有显著增强的效果。本文为小区域住房空置率的影响因素剖析提供了参考。  相似文献   

壳聚糖和PDMDAAC改性膨润土用于处理含油废水的研究   总被引：1，自引：0，他引：1  

邵红  刘相龙  王大卫  徐微雪 《岩矿测试》2014,33(3):426-432

含油废水污染范围广,对人类和生态环境危害大。采用常规方法(如浮选法、絮凝法、电化学法、膜分离法和生物法)处理的除油率不高于91%,成本较高,因此急需开发一种高效低廉的吸附剂。膨润土是一种优良的吸附剂,但用其直接处理含油废水的效果较低。本文选用壳聚糖和PDMDAAC两种有机物作为改性剂,对钠基膨润土改性,使膨润土能有效地处理含油废水。通过实验比较了两种有机改性膨润土处理含油废水的最佳去除条件,探讨了表征对其吸附性能的影响。去油效果结果表明:壳聚糖改性膨润土的除油率可达87.8%,PDMDAAC改性膨润土的除油率可达89.3%,处理所需时间少于15 min;除油效率和处理时间都优于常规方法。吸附性能表征结果显示,两种改性剂均以负载的方式和钠基膨润土颗粒结合,吸附性能良好;相比而言,PDMDAAC改性膨润土的处理效果比壳聚糖改性膨润土更好。PDMDAAC应用于含油废水的处理,具有成本低、效率高、操作简单的特点,在含油废水处理领域具有较好的应用前景。  相似文献   

红外光谱/扫描电镜等现代大型仪器岩石矿物鉴定技术及其应用   总被引：4，自引：3，他引：1  

杜谷  王坤阳  冉敬  王风玉  潘忠习 《岩矿测试》2014,33(5):625-633

传统的光学显微镜由于分辨率、放大倍数的限制,对于细微颗粒的定性分析不准确,矿物的定量分析存在一定的误差,对纳米-微米级矿物形貌及结构特征的观察束手无策。随着油气勘探及地质找矿的不断深入,需要提供岩石中所有矿物、孔隙及微量元素的信息,因此整合傅里叶红外光谱仪、X射线衍射仪、拉曼光谱仪、扫描电镜的优点,建立以大型仪器为基础的岩石矿物鉴定方法是当前地质工作的需要。红外光谱光谱范围为7500~370 cm-1,能对固、液、气样品中含量高于30%的矿物进行快速、准确的定性分析;主要用于有机质分析,其次还可对部分具有极性键的无机化合物及金属氧化物进行分析。X射线衍射仪能快速地对样品中含量大于15%的矿物进行较为准确的定量分析;现今主要用于各类晶质矿物的定性分析,同时也可对碳酸盐岩矿物等不含水矿物进行定量分析。拉曼光谱仪光谱范围为200~1000 nm,空间分辨率为横向0.5μm、纵向2μm,通过对包裹体进行测试能直接获得成岩过程中的温度、压力、流体成分等信息;目前主要用于流体包裹体成分的测试,其次还可对分子极化度会发生变化的液态、粉末及固体样品进行定性分析。扫描电镜分辨率达到1 nm,能清晰地观察到纳米-微米级矿物的形貌特征及矿物的结构特征;主要用于纳米-微米级的任何非磁性固体矿物的形貌及相关关系的观察。通过大型仪器建立的岩石矿物鉴定方法具有更高的分辨率,显著地提高了岩矿鉴定的精准度,大大拓宽了岩矿鉴定的范围(如鉴定纳米/微米级的矿物、矿物的不同变种等),能够全面、精准地提供岩石矿物的矿物含量和矿物组成、客观准确的成岩作用信息、清晰的矿物微观形貌及结构特征,而且仪器功能相互重叠,测试结果相互验证,保证了测试结果的可靠性。与传统光学显微镜鉴定方法相比,现代大型仪器岩石矿物鉴定技术为揭示矿物间的共生、反应、演化、岩石的成因、沉积/成岩环境等提供了依据,为地质工作提供准确、全面的矿物定性定量、组构特征及成岩作用等信息,为地质工作的顺利完成奠定了坚实的基础。  相似文献   

藏南沙拉岗锑矿流体包裹体红外显微测温研究   总被引：4，自引：0，他引：4  

孙晓明  莫儒伟  翟伟  韦慧晓  周峰  梁业恒  张相国  易建洲 《岩石学报》2014,30(1):189-198

沙拉岗锑矿是藏南金锑成矿带内最具有代表性的锑矿床。为了更直接地了解该矿床的流体物理化学特征,本文利用红外显微镜对辉锑矿及紧密共生石英中的流体包裹体进行了显微测温研究。红外显微测温分析结果表明,辉锑矿中包裹体均一温度在134.9～221.9℃,峰值在160～190℃之间,盐度在1.7%～7.3%NaCleqv,峰值在5.0%～6.0%NaCleqv之间,密度在0.879～0.958g/cm3之间,平均值为0.934g/cm3;共生石英中包裹体均一温度在142.5～205.6℃,峰值在160～190℃之间,盐度在2.3%～7.0%NaCleqv,峰值在4.0%～6.0%NaCleqv之间,密度在0.910～0.947g/cm3之间,平均值为0.929g/cm3。通过对比研究认为沙拉岗辉锑矿及共生石英形成于同一物理化学条件,捕获同一成矿流体。结合石英中单个流体包裹体激光拉曼成分分析认为成矿流体为含微量CO2、N2、CH4气体的低温、低盐度和低密度的NaCl-H2O热液体系。成矿流体的沸腾作用是辉锑矿大量沉淀主要原因。  相似文献   

广西国土空间格局演变特征与形成机理     

林树高  陆汝成  叶宗达  刘少坤  包博建  邓诗语 《地理科学》2022,42(11):1963-1974

国土空间格局演化与形成机理是人地系统交互关系研究的科学问题和国土空间规划的关键前提。采用地学图谱、标准差椭圆和空间自相关方法,分析2000—2018年广西国土空间格局演变特征,并运用地理探测器揭示其形成机理。结果表明：① 广西城镇空间加速挤占农业、生态空间形成了“一增双减”的面积变化特征,国土空间动态变化速度加快;② 广西国土空间相互转化频繁,转移轨迹多样性特征明显,农业空间与生态空间加速互换以及生态空间内部结构加快重组;③ 城镇空间与农业空间互竞主导了广西国土空间的迁移路径,城镇、农业空间存在“南高北低”和生态空间存在“北高南低”的集聚特征;④ 广西国土空间格局演变受自然地理与社会经济因素的共同作用影响,自然环境条件的限制作用减弱,社会经济发展水平驱动力增强,政策调控力度驱动作用深远。下一步可通过国土空间规划、调整产业布局和引导生产生活方式优化国土空间格局。  相似文献   

盗窃犯罪易发地的构成、影响及其区域异质性：基于地理探测器方法     

张延吉  庄宇丹  邓伟涛  郭华贵 《地理研究》2022,41(11):2884-2896

本文旨在识别盗窃犯罪易发地的主要类型、影响强度及其区域异质性特征,同时厘清地理探测器在犯罪地理研究中的适用性。利用北京中心城区的多源大数据,研究发现：① 在全域范围内,37类设施均属显著的盗窃易发地,道路边界、行政边界、用地边界也是盗窃高发的边缘地带,影响力突出的盗窃易发地更具备犯罪模式理论提及的犯罪引致条件。② 如社会解组理论所言,随着社会解组程度减弱,犯罪易发地的类型数量及其对盗窃分布的影响逐渐下降。除低解组区外,各类设施及边界的相对影响排序基本相同。③ 因未考虑混淆因素干扰,地理探测器容易高估解释变量的作用,与负二项回归结果的吻合度不高。而结合排除控制法,将混淆因素同质化的样本进行分区分析是规避外生变异和稳健运用地理探测器的可行路径。  相似文献