控制点布设对冰川区无人机摄影测量精度的影响

冰川监测是冰冻圈科学研究中的一项重要基础内容,获取高质量冰川DEM和DOM数据是研究的基础。随着无人机技术的兴起,给冰川监测提供了全新的技术手段,然而冰川区开展无人机摄影测量时,地面控制点的布设与测量成为能否获取高精度数据产品的关键,而山地冰川往往伴随着地形复杂,行走困难,野外实地测量难以全面实施等不利因素。本研究中以位于祁连山西段大雪山地区的老虎沟12号冰川末端部分为研究区域,设计实施了多种控制点布设方案,使用低空微型无人机飞行3个架次,获取研究区航摄影像。通过对比控制点在不同分布情况及数量情况下,DEM和DOM数据检查点的精度,评价不同控制点布设方案的可行性。对比结果显示,在航飞过程中使用单格网模式即可获取高精度的影像数据;实施地面控制作业时,使用5—7个控制点均匀分布在测量区即可获取较高精度的图像数据;当冰川区不能满足均匀布设控制点时,可沿冰川主流线布设足够数量的控制点,所得图像精度也可以满足冰川学研究要求;若只能在冰川中下部或者中上部布设控制点,则控制点应覆盖冰面起伏较大的区域。     

日本绒螫蟹放流群体12S rRNA序列研究

参考果蝇与蚤状溞序列进行了日本绒螯蟹放流群体的线粒体DNA 12S rRNA基因片段的引物设计、PCR扩增及序列测定,得到457bp的碱基序列,其A、T、G、C含量分别为158bp(34.57%)、178bp(38.95%)、51bp(11.16%),70bp(15.32%),与果蝇与蚤状相同基因片段序列含量相似.     

都江堰震后土地利用/覆被变化信息提取方法研究

快速和精确评估"5·12"汶川地震后的土地利用/覆被变化对科学减灾、灾后重建及生态环境恢复具有重要意义。常规方法从遥感图像上提取土地利用/覆被变化信息时,多以研究区整体为处理对象,直接对全图像进行分类提取,容易忽略地形地貌和地质构造等背景因素对分类结果的影响。本文以都江堰为试验区,根据地质构造展布特征及地形地貌发育形态将其分成平原区(Ⅰ区)、低山区(Ⅱ区)、中高山区(Ⅲ区)和高山区(Ⅳ区)。对Ⅰ区采用ISODATA方法进行非监督分类;对Ⅱ区和Ⅲ区分别采用最大似然(ML)分类法进行监督分类;对Ⅳ区采用人机交互解译方法进行分类。试验结果表明,基于地理地质环境的分块分类方法是高效、精确的。     

A mathematical and numerical model for reactive fluid flow systems

We formulate mathematical and numerical models for multispecies, multi-phase and non-isothermal reactive fluid flow in porous media focusing on the chemical reactions and the transport of solutes. Mass conservation and stability in the time integration are emphasized. We use cell-centered finite volume differencing in space and an implicit Runge-Kutta method in time. Assuming two space dimensions, we introduce flux approximation for arbitrarily shaped convex quadrilaterals. On equidistant and variable sized rectangular grids we choose limited κ= related schemes to approximate the advective flux and the central difference scheme for the diffusive flux. On non-rectangular grids we recommend the VF9 scheme for the estimation of the diffusive flux. Our model exists as a code. This revised version was published online in July 2006 with corrections to the Cover Date.     

Ammonia observations of the nearby molecular cloud MBM 12

We present NH₃(1,1) and (2,2) observations of MBM 12, the closest known molecular cloud (65-pc distance), aimed at finding evidence for on-going star formation processes. No local temperature (with a T _rot upper limit of 12 K) or linewidth enhancement is found, which suggests that the area of the cloud that we have mapped (15-arcmin size) is not currently forming stars. Therefore this nearby 'starless' molecular gas region is an ideal laboratory to study the physical conditions preceding new star formation.
A radio continuum source has been found in Very Large Array archive data, close to but outside the NH₃ emission. This source is likely to be a background object.     

Spectral study of the object HH12

Spectral studies of one of the brightest Herbig-Haro objects, HH12, using a multiaperture (multi-pupil) spectrograph are reported. We identify nine knots (densification nodes) in intensity diagrams. Hα emission mainly predominates in this object, except in two of the knots (C and M) which have a lower excitation level, given their high [SII] line intensity. The average electron temperature across the object is 6700 K. It is shown that the radial velocity of the object as a whole is low, i.e., its motion is mostly in the celestial plane. The excitation source for HH12 is also discussed. __________ Translated from Astrofizika, Vol. 49, No. 1, pp. 71–79 (February 2006).