�ռ�����ؾֲ�ָ��Moranָ����Gϵ���о�   总被引：15，自引：0，他引：15  

张松林  张昆 《大地测量与地球动力学》2007,27(3):31-34

?о????????????????????????????Moran?????G???????????????????????Щ?д?????????????????м??????????????????????ó????G?????????Moran?????????  相似文献   

CO Clouds around SNR G21.8-0.6 and G32.8-0.1     

Jian-Jun Zhou Xi-Zheng Zhang Hong-Bo Zhang Jarken Esimbek Ju-Yong Zhang Bing-Gang Ju 《中国天文和天体物理学报》2007,7(5):705-711

We made the first CO(I—0) mapping to SNR G21.8-0.6 and SNR G32.8-0.1, both associated with OH 1720 MHz maser.Based on the morphological correspondence and velocity and position agreement between the radio remnant and the CO clouds,we tentatively identify the clouds that are respectively interacting with the two SNRs.  相似文献   

加蓬G4-188区块钻井技术实践认识     

石强 《海洋地质译丛》2008,(1):82-87

加蓬G4-188区块是一个新的海外勘探区块,在钻井过程中遇到了井壁垮塌、气侵、井斜控制困难等诸多难题,影响了钻井施工的速度。针对这些难题,实施了解决G4-188区块钻井施工难点的各项技术措施,为G4-188区块后续钻井施工提供了有益的技术支持。  相似文献   

Historical Evidence for the Birth of the Newly Discovered Pulsar PSR J1833-1034     

Zhen-Ru Wang  Min Li  Yi Zhao Astronomy Department  Nanjing University  Nanjing  Institute of Chinese Classics  Nanjing University  Nanjing 《中国天文和天体物理学报》2006,6(5)

Stimulated by the recent discovery of PSR J1833-1034 in SNR G21.5-0.9 and its age parameters presented by two groups of discovery, we demonstrate that the PSR J1833-1034 was born 2053 years ago from a supernova explosion, the BC 48 guest star observed in the Western Han (Early Han) Dynasty by ancient Chinese. Based on a detailed analysis of the Chinese ancient record of the BC 48 guest star and the new detected physical parameters of PSR J1833-1034, agreements on the visual position, age and distance between PSR J1833-1034 and the BC 48 guest star are obtained. The initial period P0 of PSR J1833-1034 is now derived from its historical and current observed data without any other extra assumption on P0 itself, except that the factor PP is a constant in its evolution until now.  相似文献   

Tourmaline from the Archean G.R.Halli gold deposit,Chitradurga greenstone belt,Dharwar craton （India）： Implications for the gold metallogeny     

Susmita Gupta  ;M. Jayananda  ;Fareeduddin 《地学前缘(英文版)》2014,5(6):877-892

Tourmaline occurs as a minor but important mineral in the alteration zc,ne of the Archean orogenic gold deposit of Guddadarangavanahalli （G.R.Halli） in the Chitradurga greenst~ne belt of the western Dharwar craton, southern India. It occurs in the distal alteration halo of the G.R.Halli golcl deposit as （a） clusters of very fine grained aggregates which form a minor constituent in the natrix of the altered metabasalt （AMB tourmaline） and （b） in quartz-carbonate veins （vein tourmaline）. ~[＇he vein tourmaline, based upon the association of specific carbonate minerals, is further grouped as （i） albite-tourmaline-ankerite-quartz veins （vein-1 tourmaline） and （ii） albite-tourmaline-calcite-quartz veins （vein-2 tourmaline）. Both the AMB tourmaline and the vein tourmalines （vein-I and vein-2） belong to the alkali group and are clas- sified under schorl-dravite series. Tourmalines occurring in the veins are zoned while the AMB tour- malines are unzoned. Mineral chemistry and discrimination diagrams 1eveal that cores and rims of the vein tourmalines are distinctly different. Core composition of the ve：n tourmalines is similar to the composition of the AMB tourmaline. The formation of the AMB tourmaline and cores of the vein tour- malines are proposed to be related to the regional D1 deformational event associated with the emplacement of the adjoining ca. 2.61 Ga Chitradurga granite whilst rims of the vein tourmalines vis-a- vis gold mineralization is spatially linked to the juvenile magmatic accretion （2.56-2.50 Ga） east of the studied area in the western part of the eastern Dharwar craton.  相似文献   

冰后回弹对全球及中国参考框架的影响分析     

于男  程鹏飞  成英燕  李兵 《测绘科学》2014,39(12)

文章利用ICE-5G模型发布的最新预报值,计算分析了冰后回弹对全球和中国区域的影响,发现冰后回弹不仅会引起垂直方向的地壳运动,而且还会引起水平方向的地壳运动,但是水平方向的量级要明显小于垂直方向.全球范围内最大回弹区域位于加拿大,大约为16mm/a,而由冰后回弹所引起的地壳水平方向运动达3mm/a.这个回弹量级对于维持毫米级ITRF的稳定所造成的影响是不容忽视的.中国范围内回弹值大概在0～0.7mm/a,这个量级对于参考框架的影响基本可以忽略.  相似文献   

Characteristics of the supernova remnant G351.7+0.8 and a distance argument against its association with PSR J1721−3532     

W. W. Tian  M. Haverkorn †  H. Y. Zhang 《Monthly notices of the Royal Astronomical Society》2007,378(4):1283-1286

New images of the supernova remnant (SNR) G351.7+0.8 are presented based on 21-cm H  i -line emission and continuum emission data from the Southern Galactic Plane Survey. SNR G351.7+0.8 has a flux density of 8.4 ± 0.7 Jy at 1420 MHz. Its spectral index is 0.52 ± 0.25 ( S = v ^−α) between 1420 and 843 MHz, typical of adiabatically expanding shell-like remnants. H  i observations show structures possibly associated with the SNR in the radial velocity range of −10 to −18 km s⁻¹, and suggest a distance of 13.2 kpc and a radius of 30.7 pc. The estimated Sedov age for G351.7+0.8 is less than  6.8×10⁴ yr  . A young radio pulsar PSR J1721−3532 lies close to SNR G351.7+0.8 on the sky. The new distance and age of G351.7+0.8 and recent proper motion measurements of the pulsar strongly argue against an association between SNR G351.7+0.8 and PSR J1721−3532. There is an unidentified, faint X-ray point source 1RXS J172055.3−353937 which is close to G351.7+0.8. This may be a neutron star potentially associated with G351.7+0.8.  相似文献   

基于3G与3S集成的土地利用执法检查应用     

董廷旭  王建华  陈朝镇  张新合 《地球信息科学学报》2011,13(2):260-265

土地卫片执法检查是政府实施土地严格管理的重要手段.本文以绵阳市2009年度遥感土地执法检查为例,选用2008年和2009年两个时相的中巴资源卫星02B遥感图像作为信息源,对3G与3S集成技术在土地利用执法检查中应用方法进行了研究.该方法利用RS获取土地利用变化信息,利用VRS-GPS技术采集变化图斑空间与属性特征信息,...  相似文献   

2种江蓠藻体切段的再生     

赵素芬  庄承纪 《广东海洋大学学报》1999,(2)

初步研究了细基江蓠繁枝变种（Ｇ． ｔｅｎｕｉｓｔｉｐｉｔａｔａ ｖａｒ． ｌｉｕｉ）和细基江蓠（Ｇ． ｔｅｎｕｉｓｔｉｐｉｔａｔａ）切段培养的适宜培养基及其切段的再生特点。在此基础上，还研究了几种植物生长调节剂对江蓠藻体切段再生的影响。研究表明，江蓠藻体在改良ＰＥＳ培养基中生长良好。两种藻体的外皮层细胞均可产生长成新枝的生长点，并且表现出相同的再生极性。无论细基江蓠繁枝变种还是细基江蓠的切段都是在形态学上端切口处产生新枝，下端不再生；带分枝的切段，其分枝断口处亦可再生新枝。适宜的植物生长调节剂可明显促进藻体芽的产生和生长。１ ｍ ｇ／ ＬＢＡ 明显促进细基江蓠繁枝变种切段的再生，２ ｍ ｇ／ Ｌ ＢＡ＋ ０．５ ｍ ｇ／Ｌ ＮＡＡ 显著促进细基江蓠切段的再生  相似文献   

The magnetic field structure of SNR G328.4+0.2 from polarimetric observations at 19 GHz     

Simon Johnston  N. M. McClure-Griffiths  Bärbel Koribalski 《Monthly notices of the Royal Astronomical Society》2004,348(2):L19-L22

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