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21.
莫苇塘红土型镍矿分为土状矿和岩状矿,矿物成分基本相同,但量上有差异。矿石主要由蛇纹石类硅酸盐矿物和褐铁矿、赤铁矿等氧化物、氢氧化物矿物组成,有用组份镍主要赋存于硅酸盐类矿物和氧化物、氢氧化物类矿物中。  相似文献   
22.
高李阳  王爱萍 《云南地质》2011,30(3):273-274
羊缅金矿位于昌宁-孟连有色金属贵金属成矿带,金矿受压扭性断裂控制,分布于变余辉长辉绿岩中,典型的低温热液蚀变型金矿床。  相似文献   
23.
孙福伟  付义琴 《云南地质》2011,30(3):312-315
芒亨河断裂的次级断裂是主要控矿构造,含矿围岩为上三叠统小定西组(T3xd)富钠质安山岩、玄武岩。受构造、层位、碎屑粒度的制约。  相似文献   
24.
西藏尼木斑岩铜多金属矿区后续地质勘查思考   总被引:1,自引:0,他引:1  
胡光龙 《云南地质》2011,30(4):394-397
根据前期勘查结果,岗讲Ⅰ号矿体品位偏低,矿体厚度、产状变化较大,形态较复杂,应加强矿区基础地质工作,综合地质研究工作,总结铜、钼空间富集规律,建立成矿模式,指导矿区深部及外围找矿的合理化布局。  相似文献   
25.
吴维虎 《云南地质》2011,30(4):404-406,403
普朗岩体外接触带,与热液活动密切相关,受构造裂隙控制,大脉状产出,可寻找大脉型矿体。而北部向深部寻找与斑岩有关的矿体;西南部则可寻找角岩化带矿体。  相似文献   
26.
曾国平  徐权  刘世维 《云南地质》2011,30(4):420-424,430
攀枝花辉长岩体岩浆分异为深源和就地分异并存,可分为两个阶段。原始铁钛氧化物熔浆从下往上分异形成超基性岩—富矿体—辉长岩夹低品级矿石—中品贫矿石—表外矿—辉长岩夹表外矿—辉长岩。依据矿床成因、地质构造、地磁异常特征,认为攀枝花矿尖山矿段深部有望发现大矿。  相似文献   
27.
干溪沟属于湔江的支流,在大地构造部位上位于龙门山断褶带中段前缘,地貌上属于侵蚀构造地貌和河流地貌,切割深,降雨量丰富,河谷、河流较发育.由于人工开采矿石普遍,地质灾害较发育,典型的地质灾害主要有大白岩崩塌体、大团包滑坡体、干溪沟潜在泥石流.大白岩逆冲崩塌体是在汶川大地震发生时,映秀一北川断层发生逆冲,上盘灰岩错出山坡,...  相似文献   
28.
山东省莱州-安丘铁成矿带特征及找矿方向   总被引:1,自引:0,他引:1  
莱州-安丘铁成矿带位于沂沭断裂带东侧,胶北隆起的西南部。成矿带呈NE向展布,长约100 km,宽10~20km。已知区内铁矿类型主要有沉积变质型、岩浆熔离型和岩浆期后热液型,成矿除受地层控制外,还与构造、岩浆活动关系密切。通过对地质和重、磁物理场的分析,确定不同成因类型铁矿的分布范围,并且划分出不同磁异常特征,指出今后的找矿方向。  相似文献   
29.
The SAGE iron addition experiment was conducted from R.V. Tangaroa east of South Island, New Zealand, in late March-early April 2004. A desktop survey of climatological data was completed before the experiment, providing information to inform site selection and experiment design. The desktop survey is presented here in updated and enhanced form in order to explain the site selection and describe the conditions expected at the site during the experiment in comparison with those actually encountered.The experiment site was in Subantarctic waters between the Subtropical and Subantarctic Fronts. These waters are characterised by high surface macronutrient concentration, low iron concentration and low chlorophyll. The preferred site based on the desktop survey was in the vicinity of 173.5°E, 47.5°S, in Southern Bounty Trough. The actual release location was chosen immediately before the release and was 112 km to the northwest of this at 172°32′E, 46°44′S. The surface water here has typically come from the southwest (over the northern Campbell Plateau) or the southeast (through Pukaki Gap) and the mean current is directed towards ENE at ∼0.1 m s−1. The release location is well removed from regions of high eddy kinetic energy to the east (where the Subantarctic Front reaches its northern limit) and the west (where fine-scale instabilities develop on the Southland Front, which flows along the continental shelf). Typical conditions at the release site at the end of March are: surface temperature 12 °C; mixed layer depth 40 m; surface chlorophyll concentration ∼0.3 mg m−3; surface photosynthetically active radiation (PAR) 23 E m−2 d−1; surface nutrient concentrations 8-10 mmol m−3 (nitrate), 0.5-0.8 mmol m−3 (phosphate), 1-2 mmol m−3 (silicate) and 0.1-0.5 nM (iron); 99th percentile wind speed 19-21 m s−1. At this time of year, surface PAR is well below its summer maximum, the mixed layer is beginning its seasonal deepening and the silicate concentration is at its seasonal minimum. These factors may have limited the phytoplankton response to iron addition and were compounded in March-April 2004 by strong winds early in the experiment (substantially exceeding the 99th percentile in speed), lower than the average SST, larger than the average mixed layer depth, silicate concentration at the bottom end of the expected range and initially low PAR.  相似文献   
30.
The impact of in situ iron fertilisation on the production of particulate dimethylsulphoniopropionate (DMSPp) and its breakdown product dimethyl sulphide (DMS) was monitored during the SOLAS air-sea gas exchange experiment (SAGE). The experiment was conducted in the high nitrate, low chlorophyll (HNLC) waters of the sub-Antarctic Southern Ocean (46.7°S 172.5°E) to the south-east of New Zealand, during March-April, 2004. In addition to monitoring net changes in the standing stocks of DMSPp and DMS, a series of dilution experiments were used to determine the DMSPp production and consumption rates in relation to increased iron availability. In contrast to previous experiments in the Southern Ocean, DMS concentrations decreased over the course of the 15-d iron-fertilisation experiment, from an integrated volume-specific concentration in the mixed layer on day 0 of 0.78 nM (measured values 0.65-0.91 nM) to 0.46 nM (measured values 0.42-0.47 nM) by day 15, in parallel with the surrounding waters. DMSPp, chlorophyll a and the abundance of photosynthetic picoeukaryotes exhibited indiscernible or only moderate increases in response to the raised iron availability, despite an obvious physiological response by the phytoplankton. High specific growth rates of DMSPp, equivalent to 0.8-1.2 doublings d−1, occurred at the simulated 60% light level of the dilution experiments. Despite the high production rates, DMSPp accumulation was suppressed in part by microzooplankton grazers who consumed between 61% d−1 and 126% d−1 of the DMSPp production. Temporal trends in the rates of production and consumption illustrated a close coupling between the DMSP-producing phytoplankton and their microzooplankton grazers. Similar grazing and production rates were observed for the eukaryotic picophytoplankton that dominated the phytoplankton biomass, partial evidence that picoeukaryotes contributed a substantial proportion of the DMSP synthesis. These rates for DMSPp and picoeukaryotes were considerably higher than for chlorophyll a, indicating higher cycling rates of the DMSP-producing taxa than for the bulk phytoplankton community. When compared to the total phytoplankton community, there was no evidence of selection against the DMSP-containing phytoplankton by the microzooplankton grazers; the opposite appeared to be the case. SAGE demonstrated that increased iron availability in the HNLC waters of the Southern Ocean does not invariably lead to enhanced DMS sea-air flux. The potential suppression of DMSPp accumulation by grazers needs to be taken into account in future attempts to elevate DMS emission through in situ iron fertilisation and in understanding the hypothesised link between levels of Aeolian iron deposition in the Southern Ocean, DMS emission and global albedo.  相似文献   
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