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31.
笔者从相对海平面升降对礁生长发育控制角度建立新的生物礁成因分类(进积礁、并进礁和退积礁),提出南盘江地区(含十万大山盆地)茅口期为由两向东进积的进积礁,长兴期为并进礁.据此推断南盘江盆地和十万大山盆地均有可能存在茅口期层位相当于Yabeina和Neomisellina化石带的潜伏礁带,但存在长兴期潜伏礁的可能性不大. 相似文献
32.
Pull-apart Basins and the Total Lateral Displacement Along the Haiyuan Fault Zone in Cenozoic 总被引:2,自引:0,他引:2
INTRODUCTIONItisdebatedaboutthetotallateraldisplacementalongthemainboundaryfaultsofintraplateblocksineasternAsiacontinentinCenozoicera .Inthe 1 970sof2 0thcentury ,somescientistshades timatedlateraldisplacementbasedongeomorphicdata .Theyproposedthatthetotald… 相似文献
33.
I.horoductionPleNorthwestPacificOceanisti1elnostfrequentlyaffeCtedareaoftropicalcyclone(TC).AboLIt36percentTCoftheworldoccurinffosarea[2],andthenumberofTCWhichlandedonChinawiti1n1akimumwindforcescalesoverlOisabout35percentofti1atintheeastemcoastalcoLUitriesofAsia[l].BothrainstormsandfloodsMide,theidriuenceofTCareheaVyinChina,suchastherainfalldePthof2749mm/3datXinliao,Taiwanandpeakdischargeof44,6oOm'/satHuanggo(55,42okn'),YalujiangRjver.Therefore,TCisanimportantfaCtorforflooddisas… 相似文献
34.
35.
登陆过程中热带风暴"黄蜂"螺旋云带的分析 总被引:2,自引:2,他引:0
分析了热带风暴"黄蜂"在登陆过程中逐小时高分辨红外云图上的螺旋云带及其强对流云团的变化规律.从强对流云团发展为主螺旋云带的演变过程中,螺旋云带主要表现为其前端的对流逐渐加强,其余部分逐渐减弱,以及前端的强对流云团总体表现为旋入运动且维持时间较长,而其余部分的云团总体表现为远离中心等的特征.初步探讨了螺旋云带结构变化与风暴强度之间的关系和"黄蜂"在登陆后迅速减弱的可能原因. 相似文献
36.
1 INTRODUCTIONThat the radar data are reasonably ingested into theassimilation analysis system to improve the analysisquality and prediction precision is one of the problemsmeteorologists currently try to resolve. Many scholarshave already obtained some r… 相似文献
37.
1 INTRODUCTIONThe initial state of the atmosphere is one of the keyfactors that affect the result of NWP. With thedevelopment of increasingly finer NWP, the quality ofinitial atmospheric state has been drawing more andmore attention[1-7]. GRAPES 3D- Var(G… 相似文献
38.
Comparison of manual and automatic methods for measurement of methane emission from rice paddy fields 总被引:29,自引:0,他引:29
Zheng Xunhu Wang Mingxing Wang Yuesi Shen Renxing Li Jing J. Heyer M. Kogge Li Laotu Jin Jisheng 《大气科学进展》1998,15(4):569-579
The methane emission flux from rice paddies was simultaneously measured with automatic and manual methods in the suburban of Suzhou. Both methods were based on the static chamber/ GC-FID techniques. Detail analysis of the experimental results indicates: a) The data of methane emission measured with the automatic method is reliable. b) About 11 or 19 o’clock of local time is recommended as the optimum sampling time for the manual spot measurement of methane emission from rice paddies. The methane emission fluxes measured by manual sampling at local time other than the optimum time have to be corrected. The correction coefficient may be determined by automatic and continuous measurement. c) In order to get a more accurate result, an empirical correction factor, such as 18%, is recommended to correct the seasonally total amount of measured methane emission by enlarging the au-tomatically measured data or reducing the manually measured ones. 相似文献
39.
Yun-Chun Jiang Yuan-Deng Shen Jing-Xiu Wang National Astronomical Observatories / Yunnan Observatory Chinese Academy of Sciences Kunming National Astronomical Observatories Chinese Academy of Sciences Beijing 《中国天文和天体物理学报》2007,7(1):129-140
1 INTRODUCTION Filaments are cool, dense material suspended in the hot, tenuous corona. It is widely accepted that the global magnetic field surrounding the filaments plays a key role in their formation, structure and stability (Tandberg-Hanssen1995). Fil… 相似文献
40.
Wen-Feng Luo Jun Yang Lang Cui Xiang Liu Zhi-Qiang Shen 《中国天文和天体物理学报》2007,7(5):611-619
We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4,1.7,2.3,5.0,8.4,15.4GHz and the European VLBI Network at 6.7 GHz.The low frequency(1.4,1.7 and 2.3GHz)ob- servations reveal a weak and extended steep-spectrum component at about 30mas away at position angle-110°,which may be a remnant emission.The radio structure of OQ 208 con- sists of two mini-lobes at 5.0,6.7,8.4 and 15.4 GHz.Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region.By fitting the 8.4 GHz images from 1994 to 2005,we obtain a separation speed of 0.031±0.006 mas yr~(-1)between the two mini-lobes.This indicates a jet proper motion of 0.105±0.020 c and a kinematic age of 219±42 yr for the radio source. 相似文献