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介绍了碱沟山矿区区域构造地质背景，总结了控煤构造特征及其与聚煤规律的关系，探讨了研究区控煤构造的演化过程，旨在对碱沟山矿区勘探和开发具有指导意义。 相似文献
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In this paper, we analyze the results of ground-based and space-born photometric observations of the major satellites of Uranus—Miranda, Ariel, Umbriel, Titania, and Oberon. All sets of photometric observations of the satellites available in the literature were examined for uniformity and systematic differences and summarized to a unified set by wavelength ranging from 0.25 to 2.4 μm. This set covers the interval of phase angles from 0.034° to 35°. The compound phase curves of brightness of the satellites in the spectral bands at 0.25, 0.41, 0.48, 0.56, 0.75, 0.91, 1.4, and 1.8 μm, which include a pronounced opposition surge and linear part, were constructed. For each satellite, the geometric albedo was found in different spectral bands taking into account the brightness opposition effect, and its spectral dependence was studied. It has been shown that the reflectance of the satellites linearly depends on the wavelength at different phase angles, but has different spectral gradients. The parameters of the phase functions of brightness, including the amplitude and the angular width of the brightness opposition surge, the phase coefficient, and the phase angle at which the nonlinear increase in brightness starts, were determined and their dependences on wavelength and geometric albedo were analyzed. Our investigations show that, in their optical properties, the satellites Miranda and Ariel, Titania and Oberon, and Umbriel present three types of surfaces. The observed parameters of the brightness opposition effect for the Uranian satellites, some ice satellites of Jupiter and Saturn, and the E-and S-type asteroids are analyzed and compared within the framework of the coherent backscattering and mutual shadowing mechanisms. 相似文献
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M. Fränz J.D. Winningham E. Roussos S. Barabash M. Holmström M. Yamauchi R.A. Frahm J.R. Scherrer Y. Soobiah D.O. Kataria T. Säles W. Schmidt J. Kozyra E. Roelof S. Livi K.C. Hsieh M. Grande J.-A. Sauvaud J.-J. Thocaven S. Orsini M. Maggi P. Bochsler K. Asamura 《Icarus》2006,182(2):406-412
Using data of the ASPERA-3 instrument on board the European Mars Express spacecraft we investigate the effect of the martian crustal fields on electrons intruding from the magnetosheath. For the crustal field strength we use published data obtained by the Mars Global Surveyor MAG/ER instrument for a fixed altitude of 400 km. We use statistics on 13 months of 80-100 eV electron observations to show that the electron intrusion altitude determined by a probability measure is approximately linearly dependent on the total field strength at 400 km altitude. We show that on the dayside the mean electron intrusion altitude describes the location of the Magnetic Pile-Up Boundary (MPB) such that we can quantify the effect of the crustal fields on the MPB. On the nightside we quantify the shielding of precipitating electrons by the crustal fields. 相似文献
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城市空间具有市场、规划双向驱动的特点,但中国学界对两者空间影响尺度的研究却相对较少。本文以1980—2010年浙江10个城市的城乡过渡带为案例,以其兼有市场、规划驱动的院落组级、街坊级、小区级、居住区级约60 m至约800 m的空间尺度为研究对象,利用5年期数据对这一微中观空间进行了广义空间多重分形分析。整体分析显示,规律化、趋势化和无序化土地斑块演变组分的耦合,在城乡过渡带形成了3个基本尺度区间：市场驱动为主的院落组级空间,规划驱动为主的居住区级空间,两者过渡的街坊级、小区级空间。空间拓展的主导性分析表明,因市场、规划在各尺度上引领作用的不同,院落组级、小区级、居住区级空间演变的趋势化与规律化相复合的特征明显,街坊级则偏于趋势化与无序化复合下的空间演变。主体性分析进一步显示,各尺度区间在相应驱动力的作用下,院落组级空间以趋势化的集聚、小区级、居住区级空间以趋势化的扩散为主;街坊级则突出表现为无序化的空间拓展。本文的贡献在于通过f(a)-a(q)曲线上规律化、趋势化、无序化区间的组合及时序变化,量化地认识了城乡过渡带常为趋势化与规律化相复合的空间拓展所主导、但却以趋势化的空间拓展为主体的客观现象,为国土空间规划中市场、规划的空间影响尺度划分、“多层级特征的系统辨识”提供具体的科学依据。 相似文献
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L. V. Ksanfomality 《Solar System Research》2007,41(6):463-482
In this paper, we consider the physical properties and characteristic features of extrasolar planets and planetary systems, those, for which the passage of low-orbit giant planets across the stellar disk (transits) are observed. The paper is mostly a review. The peculiarities of the search for transits are briefly considered. The main attention in this paper is given to the difference in the physical properties of low-orbit giant planets. A comparison of the data obtained during the transits of “hot Jupiters” points to the probable existence of several distinct subtypes of low-orbit extrasolar planets. “Hot Jupiters” of low density (HD 209458b), “hot Jupiters” with massive cores composed of heavy elements (HD 149026b), and “very hot Jupiters” (HD 189733b) are bodies that probably fall into different categories of exoplanets. Dissipation of the atmospheres of low-orbit giant planets estimated from the experimental data is compared with the calculated Jeans atmospheric losses. For “hot Jupiters”, the expected Jeans mass losses due to atmospheric escape on a cosmogonic time scale hardly exceed a few percent. Low-orbit giant planets should have a strong magnetic field. Since the orbital velocity of “hot Jupiters” is close to the magnetosonic velocity (or can even exceed it), the moving planet should actively interact with the “stellar wind” plasma. The possession of a magnetic field by extrasolar planets and the effects of their interaction with plasma can be used to search for extrasolar planets. 相似文献
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