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991.
Yu. N. Korenkov V. V. Klimenko M. Förster V. A. Surotkin J. Smilauer 《Annales Geophysicae》1997,14(12):1362-1374
Near-earth plasma parameters were calculated using a global numerical self-consistent and time-dependent model of the thermosphere, ionosphere and protonosphere (GSM TIP). The model results are compared with experimental data of different origin, mainly EISCAT measurements and simultaneous satellite data (Ne and ion composition). Model runs with varying inputs of auroral FAC distributions, temperature of vibrationally excited nitrogen and photoelectron energy escape fluxes are used to make adjustments to the observations. The satellite data are obtained onboard Active and its subsatellite Magion –2 when they passed nearby the EISCAT station around 0325 and 1540 UT on 31 July 1990 at a height of about 2000 and 2200 km, respectively. A strong geomagnetic disturbance was observed two days before the period under study. Numerical calculations were performed with consideration of vibrationally excited nitrogen molecules for high solar-activity conditions. The results show good agreement between the incoherent-scatter radar measurements (Ne, Te, Ti) and model calculations, taking into account the excited molecular nitrogen reaction rates. The comparison of model results of the thermospheric neutral wind shows finally a good agreement with the HWM93 empirical wind model. 相似文献
992.
Properties of wave velocity for two types of granitoids at high pressure and temperature and their geological meaning 总被引:1,自引:0,他引:1
Shufeng Yang Hanlin Chen Jishuang Jiang Guoqiang Zhu Hongshen Xie Wei Hou Yueming Zhang Huigang Xu 《中国科学D辑(英文版)》1997,40(5):470-476
The wave velocity for two types of granitoids was measured using the analytic method of full-wave vibration at high pressure
and high temperature. The laws of velocity changes for them differ with the pressure boost and temperature rise, and the velocity
change of S-type is more violent than that of I-type. The “softening point” of compressional wave velocity (V μ) is also revealed
during the measurement for two types of granitoids imitating the pressure and temperature at a certain depth. But the depth
of “softening”, Vp after “softening” and the percentage of Vp’s drop around the “sofrening point” for two types of granitoids are obviously different. The depth of “softening” is 15 km
approximately and Vp after “softening” is 5.62 km/s for S-type granitoid. But for I-type granitoid the depth of “softening” is 26 km approximately
and Vp after “softening” is 6. 08 km/s. Through careful analysis of rock slices after the experiment, it was found that the “softening”
of elastic-wave velocity is caused by the partial melting of granite. Combined with the results of geophysical prospecting,
these results suggest that the low-velocity layers developing in the interior of Earth crust are related to thc partial melting
of different types of granitoids. The formation of the low-velocity layer in the upper-middle Earth crust is closely related
to the development of S-type granitoid, but that in the lower Earth crust is closely related to the development of I-type
granitoid. 相似文献
993.
S. Klimov S. Romanov E. Amata J. Blecki J. Büchner J. Juchniewicz J. Rustenbach P. Triska L. J. C. Woolliscroft S. Savin Yu. Afanas’yev U. de Angelis U. Auster G. Bellucci A. Best F. Farnik V. Formisano P. Gough R. Grard V. Grushin G. Haerendel V. Ivchenko V. Korepanov H. Lehmann B. Nikutowski M. Nozdrachev S. Orsini M. Parrot A. Petrukovich J. L. Rauch K. Sauer A. Skalsky J. Slominski J. G. Trotignon J. Vojta R. Wronowski 《Annales Geophysicae》1997,15(5):514-527
The plasma-wave experiment ASPI (analysis of spectra of plasma waves and instabilities) on board the INTERBALL spacecraft is a combined wave diagnostics experiment. It performs measurements of the DC and AC magnetic field vector by flux-gate and searchcoil sensors, the DC and AC electric field vector by Langmuir double probes and the plasma current by Langmuir split probe. Preliminary data analysis shows the low noise levels of the sensors and the compatibility of new data with the results of previous missions. During several months of in-orbit operation a rich collection of data was acquired, examples of which at the magnetopause and plasma sheet are presented in second part of the paper. 相似文献
994.
Hydrologic model parameters obtained from regional regression equations are subject to uncertainty. Consequently, hydrologic
model outputs based on the stochastic parameters are random. This paper presents a systematic analysis of uncertainty associated
with the two parameters, N and K, in Nash's IUH model from different regional regression equations. The uncertainty features
associated with N and K are further incorporated to assess the uncertainty of the resulting IUH. Numerical results indicate
that uncertainty of N and K from the regional regression equations are too significant to be ignored. 相似文献
995.
下辽河坳陷现代应力场特征 总被引:2,自引:0,他引:2
本文通过辽河油田的钻孔崩落资料及小地震震源机制解,推断出辽河坳陷地区现代构造应力场的特征。两种方法得到的结果基本一致,即区域应务场和局部应力场的结果一致,该地区处于走滑断层型应力状态。 相似文献
996.
黄河上游径流预报的灰色拓扑方法 总被引:5,自引:6,他引:5
以龙羊峡水库年平均入库流量预报为例,根据灰色系统理论的建模方法,利用龙羊峡水库入库水量代表站唐乃亥水文站的实测径流资料,建立了一个GM(1,1)拓扑预测模型,用于黄河上游径流的长期预报,并取得了较为满意的结果。 相似文献
997.
云南省东北部拱王山第四纪冰川遗迹研究 总被引:7,自引:6,他引:7
云南省东北部的拱王山海拔3100m以上的山地发生过第四纪冰川作用,典型的冰川遗迹集中分布在轿子山峰附近和妖精塘-牛洞坪两个地区,遗存的冰川地貌主要有冰斗,冰蚀岩盆和侧碛堤。根据冰川地貌的组合特征,以及它们生成的先后顺序,将拱王山第四纪冰川作用划分为末次冰期的倒数第二期冰期。 相似文献
998.
连续两届国际深部地震讨论会成果累累。对深部地震的资料采集、处理、解释技术以及几类专门地质地球物理问题的研究进行了综述。研究成果在理论、方法方面是该领域的世界先进水平:在地震学应用于陆缘、陆壳与壳幔过渡带等地质问题方面有明显的提高。提出了值得讨论的问题,最后探讨了发展趋势 相似文献
999.
鹤岗盆地晚侏罗世石头河子组沉积环境及幕式聚煤作用 总被引:3,自引:0,他引:3
鹤岗盆地是一中-新生代内陆盆地,主要含煤地层上侏罗统石头河子组是一套非海相含煤地层,充填于盆地底部,自下而上可划分为三个岩性段,五个亚段和26个含煤旋回。底部第一亚段沉积期以冲积扇、辫状河环境为主;第二亚段以河流环境为主;第三亚段以河流-三角洲-湖泊环境为主;第四亚段演化为河流环境;第五亚段则以河流、冲积扇环境为主。垂向上五个亚段对应于盆地的填平补齐-扩张-稳定沉降-差异沉降-收缩五个演化阶段。富煤带位于同沉积中心的侧翼,一般含砂率60%~70%的区域含煤性最好。含煤旋回受控于盆地周期性地快-慢沉降,聚煤作用发育于每期幕式沉降的缓慢稳定沉降阶段。厚-特厚煤层都与湖泊三角洲冲积平原大面积沼泽化有关。 相似文献
1000.
应用岩石学、矿物学、地球化学及岩浆物理学等的理论和方法,对苏州地区I型和A型花岗岩的特征及成因进行了对比研究,得出以下主要结论:I型花岗岩为晚侏罗世火山弧压性环境产物,侵位较深;而A型者为A2型花岗岩,为早白垩世造山后张性环境产物,侵位较浅,具晶洞构造.A型比I型花岗岩以酸度、碱度、Al,F含量高而H2O+含量低,以REE及不相容元素丰度高,负Eu异常强,而w(LREE)/w(HREE)低为特色.A型者矿物结晶顺序先浅色后暗色,暗色矿物以富铁贫镁、REE分配系数高及负Eu异常明显及长石富碱贫钙,而与I型花岗岩不同.A型者副矿物40余种,属锆石-褐帘石-萤石型,锆石结晶温度高,(110),(111)晶面发育;而I型者仅10余种,属榍石-锆石-磷灰石型,锆石结晶温度低,(100),(311)晶面发育.I型花岗岩为幔源岩浆与下地壳部分熔融岩浆混合及AFC作用产物,而A型花岗岩为残余下地壳(麻粒岩相)熔融后分离结晶产物,二者并非同源岩浆演化关系.A型比I型岩浆来源浅,酸度大,含水少;故岩浆密度小,粘度大,上升慢,冷凝长.受密度筛影响,A型花岗岩岩浆房及侵位深度小于I型 相似文献