长牡蛎两个Dmrt家族基因的时空表达

本文以长牡蛎27个幼虫发育阶段个体以及成体的5个组织织作为实验材料,采用实时荧光定量PCR技术对Dmrt家族中的2个基因（CgDsx和CgDmrtA2）的主要对长牡蛎Dmrt家族中的2个基因（CgDsx和CgDmrtA2）在幼虫时期和成体组织中的表达模式以及在性别决定中可能发挥的作用进行了研究。采用实时荧光定量PCR技术对幼虫27个发育阶段以及成体5个组织的表达进行了测定。结果表明,长牡蛎CgDsx基因在胚胎发育初期有大量表达,其中囊胚期到担轮幼虫初期表达量最高从囊胚期到担轮幼虫初期表达量最高,其后之后表达量开始降低,在D形幼虫后期之后一直维持在极低的表达水平,此后仅在成体的雄性性腺中具有高度表达。该结果表明由此可见,CgDsx 可能也对早期胚胎发育起一定调控作用,除了同时参与了性别决定外,可能也对早期胚胎发育起一定调控作用。CgDmrtA2在长牡蛎所有组织中均有表达,各组织间表达差异不显著,在长牡蛎D形幼虫至壳顶后期表达量较高,表明其参与了胚胎中后期的发育过程说明它参与了胚胎中后期的发育过程,可能与神经的形成相关,但是其具体功能还需要进一步研究。     

一种基于复杂环境信息的导航路径动态规划算法

针对现有路径规划算法受复杂环境信息影响较大的原因,该文通过分析环境信息,综合考虑行车的时效性、安全性要求,提出一种动态路径规划辅助决策方法。该方法通过对实时环境信息进行建模和量化处理,得到不同环境特征下的道路实际权重,为路径动态规划提供先决条件;然后利用基于一阶马尔可夫链的动态路径规划算法对路径进行规划,计算出若干可选路径可供驾驶员根据实际情况进行抉择;并通过与静态权值的路径分析算法相比较得到,它能够更好地满足复杂环境信息下最优路径的规划需求,算法效率受环境因素影响较小。     

基于SLR精密轨道的天文定位精度分析

利用全球卫星激光测距服务系统(ILRS,International Laser Ranging Service)标准点资料对Ajisai卫星进行精密定轨,残差均方根(RMS)优于3 cm,得到该星的精密轨道.进而对长春站40 cm空间碎片光电望远镜获得的Ajisai卫星的天文定位资料进行精度分析,外符合精度约3″左右.单独利用天文定位数据进行轨道改进,内符合精度优于3″.改进轨道的x、y、z坐标3分量在观测数据覆盖范围内的精度在100 m之内.同样地对Jason-1卫星作数据分析,结果和Ajisai卫星精度相当.分析各个弧段的精度变化,发现定标星个数减少,会导致天文定位精度下降.据此提出可以把最少定标星比例作为评定数据质量的参考指标之一.     

C波段转发测轨系统测站偏差的标校

C波段转发测轨体制在GEO卫星测定轨中有突出优势,但其测量系统偏差的标校精度对定轨结果影响显著。基于L波段载波相位多星定轨结果,提出一种基于标准轨道拟合残差的系统偏差标校方法。该方法能够同时标校测量偏差及时标偏差,有利于弥补激光测距标校方法观测量较少的缺陷。利用国内监测站对中国导航卫星实测数据分析结果表明,经过标校后的C波段转发测轨精度可优于5 m,测量偏差及时标偏差具有较好的稳定性。     

GPS测速方法与精度分析

基于GPS测速的基本原理,利用位置微分求速方法,设计了采用白噪声正交多项式最优线性滤波器方法的位置中心平滑软件,GPS测速精度达到了0．01m／s,提高了载波相位差分测速精度。     

Astrometry of Iapetus, Ariel, Umbriel, and Titania from eclipses and occultations

Highly accurate astrometric positions obtained from eclipses and occultations of planetary satellites are reported. These measurements may be used to test existing ephemerides, to improve upon them, and to fit system constants such as satellite masses and planetary zonal harmonics. Eclipse and occultation photometry of 5 uranian satellite mutual events has resulted in precise astrometry for 3 of these moons. Relative satellite positions were determined with an uncertainty of less than 10 milli-arcseconds for 4 of the events. These observations plus two additional data from C. Miller and N.J. Chanover (private communication) indicate that predictions based on the SPICE [Acton, C.H., 1996. Planet. Space Sci. 44, 65-70] ephemeris URA083 and those from the LA06 ephemeris in a paper by Arlot et al. [Arlot, J.-E., Lainey, V., Thuillot, W., 2006. Astron. Astrophys. 456, 1173-1179] are significantly more accurate than predictions generated by Christou [Christou, A.A., 2005. Icarus 178, 171-178] using the GUST86 ephemeris in the along-track component of motion. The observations indicate that Ariel, Umbriel and Titania are lagging behind their predicted positions for all of the ephemerides, but by varying distances and significance levels. Analysis of data recorded by Hidas et al. [Hidas, M.G., Christou, A.A., Brown, T.M., 2008. Mon. Not. R. Astron. Soc. 384, L38-L40] suggests a similar lag for Oberon. Photometry recorded during the ingress portion of a saturnian eclipse of Iapetus on 2007 May 5 indicates that the middle of the event occurred at geocentric UTC 02:14:58. At that moment the center of the satellite disk facing the Sun was intersected by a solar-centered ray refracted at a minimum altitude of 240 km above the 1-bar pressure level in the planet's atmosphere. The uncertainty in the timings due to observational scatter was only 5 s which equates to 16 km of Iapetus motion, but other factors increased the overall uncertainty to 111 km or 16 milli-arcseconds at the distance of Saturn from the Sun. The astrometric result is fit very well by the SPICE ephemeris SAT288.     

Did tidal deformation power the core dynamo of Mars?

We first show that 7 out of the 20 giant impact basins of Mars recently reported by Frey [Frey, H., 2008. Geophys. Res. Lett. 35. L13203] trace a great circle on Mars. The other five basins trace another great circle and still the other three basins trace yet another great circle. The latter great circle is in good agreement with the pre-Tharsis equator of Mars that is estimated from modeling crustal magnetic anomalies [Arkani-Hamed, J., 2001. Geophys. Res. Lett. 28, 3409-3412] and diagonalizing the moment of inertia of Mars after removing the loading effects of Tharsis bulge [Sprenke, K.F., Baker, L.L., Williams, A.F., 2005. Icarus 174, 486-489]. It is shown in this paper that the three great circles were likely the equatorial plane of Mars at certain times and Mars experienced appreciable polar wander. The great circles also indicate that the asteroids that created the basins were satellites of Mars whose orbits decayed in time through spin-orbit coupling with tidally deforming Mars, and eventually impacted on the planet creating the giant basins at around 4 Ga. The orbital dynamics of four largest asteroids show that they could have orbited Mars for several hundred million years if they were retrograde satellites. Continual elliptical straining of otherwise circular fluid streamlines of the liquid core of Mars by tidal deformation could have exerted a strong strain that was large enough to overcome dissipation and excite the elliptical instability inside the core. We investigate the physical properties of the martian core that are required to allow the tidal deformation to power the core dynamo, i.e., the growth time of the elliptical instability to become shorter than the dissipation time. The tidal energy dissipation rate inside Mars caused by even only one of the 4 largest asteroids is found to be over two orders of magnitude greater than the magnetic energy dissipation rate in the core, indicating that if only one of the 4 largest asteroids were orbiting in retrograde sense, it would have likely powered the core dynamo of Mars for several hundred million years.     

Predictions for eclipses of Nereid by Neptune

Neptune will eclipse its satellite Nereid (Neptune II) on 2007 April 27 from 00 to 06 h UT and on 2008 April 21 from 12 to 17 h UT, with uncertainties of about 3 h; and a third eclipse may occur on 2009 April 17. These events offer unique opportunities for astrometric and geophysical measurement.     

综合物探方法在煤田采空区圈定和着火区调查中的应用研究

以山西晋城张岭煤田着火区、采空区勘探和着火区探测为例 ,通过对该地区地质构造特征、采空区雷达特征、着火区地温场分布等的描述与分析 ,结合该区钻探、井温测量和气体检测的结果 ,论证了地质雷达与米测温联合方法在煤田采空区圈定和着火区调查中的应用效果 ,并对该方法的应用前景作了相应探讨。     

RS、GPS、TMS相结合在合肥市大房郢水库工程用地测量中的应用

为满足合肥市大房郢水库建设及土地管理部门对用地资井的要求，利用航空遥感片对用地现状进行了调查，采用航测解析法配合其它先进测量手段(GPS全球定位系统、TMS全站仪测量系统)确定用地的各类界线。本文介绍了这次工作的技术路线，土地利用现状调查，用地界线的确定，数字影像线划地籍图的编辑及数据汇总等方面的情况。