浅析新时期土地变更调查

2010年我国开始按照新机制,采用新方法开展土地变更调查,但从目前情况看,土地变更调查工作还存在体制不顺,标准不一,调查不全,精度不高,数据不实,调查时间长等一系列问题。本文从讨论历年土地变更调查的特点及有关情况入手,筛查现阶段土地变更调查工作存在的问题并分析原因,提出了新时期做好土地变更调查工作的若干思路。     

Letters to the editor

A preliminary scuba survey of oligotrophic Lake Rotoma in 1972 revealed a vegetation mainly composed of native hydrophytes in which exotics were at an early stage of colonisation. In 1973 the presence of species was recorded in 5708 quadrats (625 cm²) at 1 m intervals along a total of 50 line transects placed systematically around the lake. Water depth was measured, and quadrat cover and substrate type were subjectively estimated. Species frequency calculations showed that the dominant vegetation pattern was a characean meadow of Chara fibrosa f. acanthopitys (A.Br.) R.D.W., Nitella leptostachys var. leonhardii (R.D.W.) R.D.W., and N. pseudoflabellata var. mucosa (Nordst.) Bailey. The charophytes extended over a depth range of 1–17.5 m on a wide variety of substrates and gradients. Native vascular plants were absent from many transects, and had a depth range only from 0 to 4.5 m, with most occurring above 3.5 m. The Low Mixed Community, found in shallow water less than 1.25 m in depth at the northeast end of the lake, provided this area with a high species diversity. Exotic hydrophytes had established in many areas around the lake. The distribution of Lagarosiphon major (Ridley) Moss and Elodea canadensis Michx. appeared to coincide with boating access and fallen submerged trees over a depth range of 0–6.0 m, although much of the available habitat had not yet been exploited. Emergent species were most abundant within the southwest inlet and also in the lagoons surrounding the lake where sheltered conditions and shallow gradients prevail.     

双参数混合正则化方法及在电导率反演成像中的应用

通过引入带有二阶正则算子的正则化项,建立了一种双参数混合正则化方法.为确定最佳正则化参数,这里主要应用L-曲线法、偏差原理和广义交叉校验准则的优化组合来确定.首先对理论模型进行了数值模拟,通过与截断奇异值分解法、共轭梯度法及标准Tikhonov正则化法的结果比较,表明该方法不仅精度高,而且对于数据的随机扰动具有稳定性.然后将此方法应用于对电导率反演成像的计算中,得到的电导率反演成像精确细致可靠,也符合实际情况.这表明该方法求解地球物理反问题时,在增强反演的稳定性及减少多解性的同时,还能进一步提高反演计算速度.     

Testing deprojection algorithms on mock angular catalogues: evidence for a break in the power spectrum

We produce mock angular catalogues from simulations with different initial power spectra to test methods that recover measures of clustering in three dimensions, such as the power spectrum, variance and higher order cumulants. We find that the statistical properties derived from the angular mock catalogues are in good agreement with the intrinsic clustering in the simulations. In particular, we concentrate on the detailed predictions for the shape of the power spectrum, P ( k ). We find that there is good evidence for a break in the galaxy P ( k ) at scales in the range 0.02< k <0.06 h Mpc⁻¹, using an inversion technique applied to the angular correlation function measured from the APM Galaxy Survey. For variants on the standard cold dark matter (CDM) model, a fit at the location of the break implies Ω h =0.45±0.10, where Ω is the ratio of the total matter density to the critical density, and Hubble's constant is parametrized as H ₀=100 h km s⁻¹ Mpc⁻¹. On slightly smaller, though still quasi-linear scales, there is a feature in the APM power spectrum where the local slope changes appreciably, with the best match to CDM models obtained for Ω h ≃0.2. Hence the location and narrowness of the break in the APM power spectrum combined with the rapid change in its slope on quasi-linear scales cannot be matched by any variant of CDM, including models that have a non-zero cosmological constant or a tilt to the slope of the primordial P ( k ). These results are independent of the overall normalization of the CDM models or any simple bias that exists betwen the galaxy and mass distributions.     

Color-Redshift Relations and Photometric Redshift Estimations of Quasars in Large Sky Surveys

With a recently constructed composite quasar spectrum and the X2 minimization technique, we describe a general method for estimating the photometric redshifts of a large sample of quasars by deriving theoretical color-redshift relations and comparing the theoretical colors with the observed ones. We estimated the photometric redshifts from the 5-band SDSS photometric data of 18678 quasars in the first major data release of SDSS and compared them with their spectroscopic redshifts. The difference is less than 0.1 for 47% of the quasars and less than 0.2 for 68%. Based on the calculation of the theoretical color-color diagrams of stars, galaxies and quasars both on the SDSS system and on the BATC system, we expect that we would be able to select candidates of high redshift quasars more efficaciously with the latter than with the former, provided the BATC survey can detect objects with magnitudes fainter than 21.     

长江中下游成矿带及邻区Moho深度与成矿背景探讨

长江中下游成矿带是我国最主要的铜铁金多金属成矿带之一。本文利用卫星重力数据计算布格重力异常,采用波数域迭代的Parker-Oldenburg位场迭代反演方法,通过重力数据反演获得长江中下游成矿带及邻区的三维Moho面结构,结合研究区已有的研究成果,探讨了研究区的深部构造格局。研究结果表明:研究区范围内Moho面总体从南西往北东有逐渐变浅趋势,最浅处位于长江口海域和杭州湾海域约28~29km,最深处位于大别山区约38~39km;长江中下游及邻区下方Moho面的隆起形态呈"V"字型,与地表的"V"字型构造特征相呼应,Moho面隆起的最深处位于"V"字型转折端附近,向两侧Moho面呈抬升状,北东走向的"V"字型东支隆起幅度和规模都要明显大于北西走向的"V"字型西支;卫星化极磁异常显示长江中下游成矿带的正磁异常高值集中分布在"V"字型东支的宁芜、庐枞、繁昌、怀宁等火山岩盆地;钦杭成矿带东段Moho面也明显上隆,隆起的中心沿钦杭成矿带的南侧边界断裂的东南侧线性分布。长江中下游成矿带和钦杭成矿带东段的Moho面条带状隆起带可能指示了地幔上隆、岩浆上涌并在壳幔边界处与下地壳发生底侵作用的深部边界,来自于壳、幔的深部含矿岩浆通过深大断裂等地壳薄弱点向上运移,并在适当的位置形成金属矿集区。     

中国大陆动力学研究内涵与轨迹的思考

大陆动力学已成为21世纪地球科学研究中的热点和中坚,在它面对当今资源、能源、灾害和环境等社会与经济快速发展需求日益增长的同时,是机遇,却也是挑战.因此厘定其研究的内涵和导向是十分重要的.基于多年的研究实践和探索,本文将对以下五个方面进行讨论:1)大陆动力学研究的内涵与界定;2)大陆动力学研究的导向和轨迹;3)大陆动力学研究中地球物理反演结果和解释中的矛盾;4)强化发展学科交叉以构成交叉科学;5)对2011年大陆动力学委员会学术活动的思考.     

南巴伦支海磁场异常及其与海底地质结构的对比(英文)

对1986—2001年间巴伦支海南部海洋磁力测量的数据处理结果进行了研究。南巴伦支海底的地磁测量揭示出其复杂多期的地质构造结构,其中以两期分离型的构造为主导:(1)具NW走向的里菲-文德期继承性裂谷构造;(2)NE向转换叠加断层正交系统。晚泥盆世碱性侵入体及其相关的金属矿化作用恰位于这些构造系统的交点上。     

Optimizing point-source parameters for scanning satellite surveys

We describe a method for deriving the position and flux of point and compact sources observed by a scanning survey mission. Results from data simulated to test our method are presented, which demonstrate that at least a 10-fold improvement is achievable over that of extracting the image parameters, position and flux, from the equivalent data in the form of pixel maps. Our method achieves this improvement by analysing the original scan data and performing a combined, iterative solution for the image parameters. This approach allows for a full and detailed account of the point-spread function (PSF), or beam profile, of the instrument. Additionally, the positional information from different frequency channels may be combined to provide the flux-detection accuracy at each frequency for the same sky position. Ultimately, a final check and correction of the geometric calibration of the instrument may also be included. The Planck mission was used as the basis for our simulations, but our method will be beneficial for most scanning satellite missions, especially those with non-circularly symmetric PSFs.     

Habitat associations of floating debris and marine birds in the North East Pacific Ocean at coarse and meso spatial scales

While many surface foraging seabirds ingest plastic, the spatial overlap of these far-ranging predators with debris aggregations at-sea is poorly understood. We surveyed concurrent distributions of marine birds and debris along a 4400 km cruise track within a debris accumulation area in the North East Pacific Ocean using line and strip transect methods. Analysis of debris and bird distributions revealed associations with oceanographic and weather variables at two spatial scales: daily surveys and hourly transects. Hourly bird abundance (densities; 0-9 birds km⁻²) was higher in lower wind and shallower water. Hourly debris abundance (densities; 0-15,222 pieces km⁻²) was higher in lower wind, higher sea-level atmospheric pressure and deeper water. These results suggest that debris and seabird abundance and community structure are influenced by similar environmental processes, but in opposing ways, with only three far-ranging seabird species (Black-footed Albatross, Cook’s Petrel and Red-tailed Tropicbird) overlapping with high debris concentrations over meso-scales.