大陆岩石圈有效弹性厚度的计算及其地质意义   总被引：4，自引：1，他引：4  

袁炳强  Yvette H.Poudjom Djomani  程顺有  陆关祥 《地球学报》2002,23(3):269-272

大陆范围内Te值有很大的范围，不同构造单元有不同的Te值。Te值的大小与岩石圈的热结构（热年龄）、壳幔耦合等因素有关。同时Te值和地壳厚度、地表有关矿产的分布、岩石圈地幔的物质组成等也有一定关系。  相似文献   

午后多重极光弧观测研究          下载免费PDF全文

温艳波  杨惠根  韩德胜  T.Araki  艾勇  刘瑞源  刘勇华  胡泽骏  陈卓天  邓忠新  刘嵘  王晶 《极地研究》2005,17(4):255-263

本文利用2001-2003年南极中山站175天全天空摄像机观测,对午后多重极光弧的出现率及其与Kp指数的关系进行了统计分析,结果表明午后多重极光弧出现率呈一单峰分布,最大发生率出现在1445UT(1645MLT),其位置在1500MLT极光热点(1300-1700MLT)近夜侧的部分。与地磁活动指数Kp的相关统计分析表明,Kp值为2-3之间时多重极光弧有较大的出现率,这说明中等地磁活动情形下午后多重极光弧有较高的出现率。事件分析表明多重极光弧的强度变化与地磁Pc5脉动具有较高的相关性,并且有类似的频谱特征,这说明午后多重极光弧可能与同时出现的Pc5地磁脉动有关。  相似文献   

Interpretation of the solar continuum from 1680 to 600 Å. Model of the transition region photosphere-chromosphere and of the chromosphere     

Yvette Cuny 《Solar physics》1971,16(2):293-313

An interpretation is given of the observations of the continuous solar radiation in the spectral range 600–1700 Å. The model allows for deviations from LTE of H, C, Si and S, and is in hydrostatic equilibrium. The predicted intensity from 1680 to 1520 Å has virtually no dependence on the electron temperature variation in the optical depth range 10^–3–4 × 10^–5, at 5000 Å; the brightness temperature is compatible with a low electronic temperature minimum near the optical depth 10^–4. The model of the low chromosphere is characterized by a steep temperature gradient. The model satisfies observations at millimeter wavelengths.  相似文献   

Evolution du spectre de la Nova Delphini 1967 dans le proche infrarouge en 1969     

Yvette Andrillat  Leo Houziaux 《Astrophysics and Space Science》1970,9(3):410-417

Spectra of Nova Del 1967 have been obtained in the photographic infrared during the period March to November 1969. The gradient in the region 1.3–1.7 µ^–1 has decreased from 3.06 in November 1968 to 2.57 in November 1969. The main spectral features occurring in the wavelength range 5800–9600 Å are described, while the profiles of some strong lines are displayed on Figures 2–6.

---

---

Les observations ont été effectuées à l'Observatoire de Haute-Provence (CNRS).  相似文献   

中山站高频雷达观测结果初步分析          下载免费PDF全文

刘二小胡红桥  刘瑞源吴振森吴铭君  杨惠根张北辰 《极地研究》2012,24(4):397-407

中山站高频相干散射雷达于2010年4月建成投入观测,并加盟SuperDARN雷达观测网,成为我国探测电离层对流的重要手段。首先简要介绍中山站高频雷达的工作原理及工作模式,然后利用该雷达第一年的观测数据,给出了每个波束观测的电离层回波总数随距离和回波强度、多普勒速度及谱宽的分布,以及电离层回波发生率随频率的变化特性。观测结果和射线追踪的模拟计算表明,由于波束指向不同,电波波矢方向与地磁场形成正交条件的区域有所不同,因此会造成不同频率下,不同波束观测的电离层回波发生率的差别。  相似文献   

Corrections for Wind-Speed Errors from Sodar and Lidar in Complex Terrain     

Stuart Bradley  Yvette Perrott  Paul Behrens  Andy Oldroyd 《Boundary-Layer Meteorology》2012,143(1):37-48

The quality of lidar and sodar wind estimates is generally judged through comparisons with mast-mounted instruments, and the resulting regressions. Evaluation of the relative merits of lidars versus sodars is complicated by the fact that lidars are generally placed close to a mast whereas sodars are generally placed some distance from a mast so that acoustic reflections off the mast are reduced. This leads to the two technologies, lidar and sodar, not being compared in similar situations. Differences arising from the two geometries can be expected to be larger in complex terrain, where the wind regime can vary significantly spatially. The current work explores these differences in moderately complex terrain. Lidar–mast comparisons are performed with the lidar close to an 80 m mast, and sodar–mast comparisons performed with the sodar 300 m from the mast. Systematic variations in estimated wind speed are found to occur with height, consistent with predictions from a simple flow model. When the lidar was moved to the sodar location, further from the mast, there were significant changes in the estimated wind speeds and a reduction in correlation with the mast-based wind speeds, as expected. However, the correlation between collocated lidar and sodar winds was high. This finding emphasizes that any comparison of two remote sensing instruments needs to be through similar experiments, and that differences in accuracy often reported for the lidar and sodar technologies are likely to be contaminated due to poor comparison configurations. A method was devised to simulate the sodar being collocated with the mast, by using the lidar–sodar measurements and the lidar–mast measurements. It was found that there was then no statistically detectable difference between lidar–mast regressions and sodar–mast regressions for the particular lidar and sodar tested. Both remote sensing instruments were also found to be good estimators of Weibull parameters, as compared with those derived from mast data. The conclusion is that the sodar measured the winds above the sodar with a similar accuracy to the lidar measuring winds above the lidar.  相似文献   

Proactive Management of Ecosystem Services in Oil Sands Pre-mining Phase     

Omotehinse  A. O.  De Tomi  G.  Baninla  Yvette 《Natural Resources Research》2020,29(2):949-965

Natural Resources Research - Ecosystems and their services are essential to human well-being, but mining activities often cause adverse impacts on these services. Although impact of mining...  相似文献   

1980—2012年5—9月川渝盆地小时强降水特征研究     

李强  邓承之  张勇  何跃  邹倩  何慧根 《气象》2017,43(9):1073-1083

利用四川和重庆123个气象观测站1980—2012年小时降水资料,分析川渝地区主汛期5—9月小时强降水频次、强度和持续性等时间演变和空间分布特征。结果表明,≥20、≥30和≥50 mm·h-1三种强度阈值强降水时间演变上,1980—2012年年际和日变化具有较好的一致性,三种强降水年平均频次分别为504、184和28次。≥20 mm·h-1 强降水空间分布上,在山地地形动力辐合抬升,以及盆地西部较大的地形梯度作用下,≥20 mm·h-1强降水高频次区主要分布于盆地西北部的龙山山脉、西南部雅安及乐山周围与盆地过渡区。≥20 mm·h-1强降水频次的日峰值空间分布上,盆地南部主要出现在20:00—01:00（北京时,下同）,而盆地中部、北部和东部主要在02:00—07:00。持续不同小时时间尺度的强降水事件日变化上,具有双峰型结构,午后为第一个降水峰值,20:00至第二天07:00为第二个峰值,白天多为短时间（2~6 h）强降水事件,而傍晚开始至第二天清晨,持续2~18 h强降水事件均有发生。不同开始时间强降水事件的强度与频次和降水量具有一致性的日变化特征,呈现单峰型结构,峰值主要发生在18:00—06:00,且不同开始时间事件频次和降水量空间分布上,白天（09:00—20:00）相对于夜间（21:00—08:00）偏小,即夜间强降水事件特征表现明显。  相似文献   

基于北极黄河站观测的日侧极光研究新进展   总被引：1，自引：0，他引：1       下载免费PDF全文

韩德胜  胡泽骏  陈相材  刘建军  胡红桥  杨惠根 《极地研究》2018,30(3):235-250

回顾了基于中国黄河站全天空极光观测对日侧弥散极光与喉区极光研究的最新进展。首先,利用黄河站极光观测,对日侧弥散极光展开系统性分类与统计研究,对这一重要空间物理现象取得新认识,指出日侧弥散极光对研究日侧外磁层冷等离子体的分布、形成及磁鞘粒子进入磁层都具有重要启示作用;同时发现并定义了一种新型分立极光结构——喉区极光,并推断其可能对应磁层顶的局地变形。喉区极光是指发生在电离层对流喉区附近、从极光卵赤道侧向低纬方向延伸出来的分立极光结构。全天空极光观测表明喉区极光走向大致与电离层对流方向一致。之后,观测验证了喉区极光对应磁层顶局地内陷式变形的推测;统计发现喉区极光是一种非常高发的现象,对应的磁层顶变形尺度可达2—3 Re,并指出这种变形最可能由磁鞘高速流冲击磁层顶产生;发现在喉区极光产生过程中还可能触发磁重联;证实伴随喉区极光的产生,磁鞘粒子会进入磁层并诱发产生一种新型弥散极光。通过喉区极光研究,可以将已有的磁鞘瞬态过程研究和触发式磁重联研究有机地结合在一起,对太阳风-磁层耦合过程形成一种新的认识,即:在磁鞘中局地产生(而不是存在于太阳风中)的瞬态过程可以在日下点附近频繁地导致磁层顶局地变形、触发重联、引发系列地球空间效应,可能对太阳风-磁层耦合具有不可忽略的重要性。以此为基础,讨论了日侧极光研究引出的新课题。  相似文献   

Thermal effects of Caledonian foreland basin formation,based on fission track analyses applied on basement rocks in central Sweden     

Yvette Huigen  Paul Andriessen 《Physics and Chemistry of the Earth》2004,29(10):683-694

Increasing evidence from fission track studies in Sweden indicate that large parts of the Fennoscandian Shield have been affected by a large-scale thermotectonic event in the Palaeozoic. In this study the results of 17 apatite fission track analyses from central Sweden are presented collected along three NW–SE transects trending from the Bothnian Sea to the Caledonides. On the Bothnian coast samples have been collected directly from the Sub-Cambrian Peneplain. The sedimentary cover protecting this surface until recently is responsible for the thermal increase detected through apatite fission track (FT) thermochronology.The apatite FT ages range between 516 ± 46 Ma (±1σ) on the Bothnian coast around sea level to 191 ± 11 Ma in the Caledonides (～500–1500 m.a.s.l.). The mean track lengths vary from 11.3 ± 2.2 μm (±1σ) in the east to 14.2 ± 2.8 μm in the west, indicating a longer stay in the PAZ in the east, versus a continuous cooling pattern in the west. This pattern in combination with other geological constraints indicates that the crystalline basement rocks near the Caledonian deformation front in the west experienced higher temperatures after the formation of the Sub-Cambrian Peneplain followed by denudation, compared with the basement rocks in the east near the Bothnian coast.The apatite FT data near the Caledonian deformation front indicates prevailing temperatures of more than 110 ± 10 °C prior to the Mid Palaeozoic, causing a resetting of the apatite fission track clock. The temperatures were progressively lower away from the deformation front. Apatite fission track analysis of samples collected from the Sub-Cambrian Peneplain along the Bothnian coast indicate maximum temperatures of 90 ± 15 °C during Late Silurian–Early Devonian time. This heating event is argued to be the result of burial beneath a developing foreland basin in front of the Caledonian orogeny. Assuming a geothermal gradient of 20 °C/km, this temperature increase can be converted to a total burial of the samples. The resulting geometry of this basin can be described as an asymmetrical basin at least 3.5 km deep in the vicinity of the Caledonian deformation front decreasing to about 2.5 km on the Bothnian coast, continuing further onto Finland. The width of this basin was in thus in the order of 600 km. Whether this was formed completely synorogenic or partly synorogenic, broadening after cessation of the orogeny, could not be revealed.The Late Palaeozoic and Mesozoic thermal evolution of this area is related to the extensional tectonics in the North Atlantic Domain.  相似文献