论浙江安吉矿产资源开发保护规划与区域经济的可持续发展

安吉县矿产资源开发利用与保护规划工作在我省开展比较早 ,规划的组织实施在国发经济建设和社会发展中已发挥出较好的作用。在参与安吉地区农业生态环境地质调查过程中 ,结合资源环境的调查评价 ,在整顿矿业秩序 ,改善和修复矿山生态环境 ,矿山地质灾害调查防治等方面做了些尝试。本文就资源环境的开发保护 ,矿业经济与区域经济可持续发展方面作些探讨 ,对于正在进行或将要进行规划和实施规划的地区具一定借鉴意义     

First Results from SWAN Lyman α solar wind mapper on SOHO

After one year of almost flawless operation on board the SOHO spacecraft poised at L1 Lagrange point, we report the main features of SWAN observations. SWAN is mainly dedicated to the monitoring of the latitude distribution of the solar wind by the Lα method. Maps of sky Lα emissions were recorded througout the year. The region of maximum emission, located in the upwind hemisphere, deviates strongly from the pattern that could be expected from a solar wind constant with latitude. It is divided into two lobes by a depression aligned with the solar equatorial plane called the Lyα groove already noted in 1976 Prognoz data. The north lobe is much brighter than the south lobe. These two characteristics can be explained qualitatively by an enhanced ionization along the neutral sheet where the slow solar wind is concentrated, which results from the higher low-latitude solar wind mass flux as measured by Ulysses. The groove is the direct imprint on the sky of the enhanced carving by the slow solar wind, at this time of solar minimum, when the tilt angle of the neutral sheet is small. The question is still pending to predict what will happen with the ascending phase of the solar cycle. Observations of comets are briefly mentioned, with the ability of SWAN to monitor the H₂O production of many comets. Operations of the instrument are briefly described, including some instrumental problems which could be solved by software modifications sent to the instrument. Supplementary material to this paper is available in electronic form at http://dx.doi.org/10.1023/A:1004979605559     

Magneto-induced Line Broadening of Magneto-sensitive Lines in Solar Magnetized Atmospheres

We analyze the spectral line broadening of those magneto-sensitive lines in solar magnetized atmospheres. The broadening at the line wings is due to the increase of the effective width of energy levels involved in Zeeman splitting, and the broadening at the line core also originated in Zeeman splitting under the condition that the Zeeman components are mixed. Therefore, the magnetoinduced or Zeeman broadening take effects on the whole line. The observed Stokes parameter data in a sunspot and outside it acquired by Solar Stokes Spectrum Telescope (S3T) are analyzed for the demonstration of this mechanism, and the Zeeman broadening rates are calculated for FeI6302.5 under some assumptions. Our result shows that the broadening is increased as the magnetic field strength becomes stronger, but the rate of increase at the line core is decreased as the field strength increases, while the rate at the wing does not show such an obvious regularity. The broadening is more effective in the line core than in the wings.     

宽甸北部早元古宙铅锌矿地质特征及成因讨论

辽宁宽甸北部早元古宙铅锌矿位于辽东青城子—吉林荒沟山—朝鲜检德铅锌矿带上。赋存于辽东优、冒地槽的过渡带,靠近优地槽一侧的碳酸盐岩建造中。矿体受岩相、岩性控制明显,属层控矿床。吕梁构造旋回的变质变形作用对矿带的改造不明显。矿带的同位素特征表明,张家堡子铅锌矿形成于封闭盆地环境,矿质来源于大陆边缘深部液态矿源层;而高丽墓子铅锌矿带则形成于正常海洋环境,表现了明显的原始沉积矿床的特点。     

致密星的X射线辐射时延现象

能谱仅反映了高能天体辐射的部分性质，而高能X射线辐射的时变可以反映致密天体的动态性质。因此，在构造高能辐射的理论模型时，既要考虑X辐射的能谱性质，也要考虑其时变性质。特别对高能天体X辐射的快速光变，一般认为其发生在致密天体附近，致密天体快速光变的研究可以揭示出致密天体附近的物理性质，因此，时变可以对X辐射模型给以很强的限制。X射线源不同能量光子到达观测者的时间差称为X射线辐射的时延。介绍了高能X辐射时变中的时延分析方法及其最新发展，综述了致密双星系统中黑洞侯选林和中子星的时延现象，并简单介绍了为解释这些现象所发展的模型，以及时延对模型的限制。     

Wind tunnel simulation experiment and investigation on the electrification of sandstorms

~~Wind tunnel simulation experiment and investigation on the electrification of sandstorms~~     

Features of clay minerals in the YSDP102 core on the continental shelf of the southeast Yellow Sea

Ninety-eight clay mineral samples from the YSDP102 core were analyzed by x-ray diffractometer to study the four clay minerals: illite, chlorite, kaolinite and smectite. Twenty-eight samples had been analyzed on the laser particle-siz eanalyzer to reveal the particle features of the sediments. Distribution of the clay minerals and the particle characteristics in the YSDP102 core show that the core experienced three different depositional periods and formed three different sedimentary intervals due to different sediment sources and different depositional environments. Features of the clay minerals and the heavy minerals in the YSDP102 core indicate that coarse-grained sediments and fine-grained sediments result from different sources. The Yellow Sea Warm Current has greatly influenced the sedimentary framework of this region since the current‘s formation.     

辨析“气候变暖”

近年来人们对＂气候变暖＂及其机制的争论达到了前所未有的程度,这可能是因为气候变化不再是单纯研究大气变化规律的科学,而变成一门与＂减排方案＂和＂征收碳税＂有关的政治与经济问题相联系,与国家经济利益有关的崭新课题.＂气候变暖＂既与利益有关,就会难免偏离公正,偏离纯理论科学.本研究对国内外＂气候变暖＂最新动态进行回顾分析,得出以下认识和结论.1）过去百年城市发展,极大地影响了器测温度数据,如果没有对＂热岛效应＂进行矫正,无疑高估了过去百年全球升温的幅度;2）过去百年全球有所变暖是事实,但不同学者增温估算不一致.不仅升温幅度不确定,而且人类和自然因素对升温贡献各占多少也不确定;如果考虑到城市发展对增温估算的影响,过去百年增温应当比0.4℃更低,远没有达到历史上次级波动的变化范围.3）尽管过去百年地球有所变暖,但在万年轨道尺度上,现在地球处于变冷的大趋势过程中.对现在气候变暖更合理解释,是属于变冷大趋势中的次级变暖波动;4）不论过去还是现在,大气CO2浓度变化总是落后于温度变化,即总是温度驱动着CO2变化,而不是CO2浓度驱动地球增温.     

Why does the Antarctic Peninsula Warm in climate simulations?

The Antarctic Peninsula has warmed significantly since the 1950s. This pronounced and isolated warming trend is collectively captured by 29 twentieth-century climate hindcasts participating in the version 3 Coupled Model Intercomparison Project. To understand the factors driving warming trends in the hindcasts, we examine trends in Peninsula region’s atmospheric heat budget in every simulation. We find that atmospheric latent heat release increases in nearly all hindcasts. These increases are generally anthropogenic in origin, and account for about 60% of the ensemble-mean warming trend in the Peninsula. They are driven primarily by well-understood features of the anthropogenic intensification of global hydrological cycle. As sea surface temperature increases, moisture contained in atmospheric flows increases. When such flows are forced to ascend the Peninsula’s topography, enhanced local latent heat release results. The mechanism driving the warming of the Antarctic Peninsula is therefore clear in the models. Evidence for a similar mechanism operating in the real world is seen in the increasing snow accumulation rates inferred from ice cores drilled in the Peninsula. However, the relative importance of this mechanism and other processes previously identified as potentially causing the observed warming, such as the recent sea ice retreat in the Bellingshausen Sea, is difficult to assess. Thus the relevance of the simulated warming mechanism to the observed warming is unclear, in spite of its robustness in the models.     

全边界层选用相似理论对O3、NOx浓度及沉降的影响

将广泛应用于东亚地区的LLA(Lurmann Lloyd Atkinson)化学机制耦合到欧拉型区域空气质量模式(RAQM),并考虑区域污染物长期模拟研究中降水随时间变化的非均匀性,讨论了湍流参数化过程中相似理论在近地层和全边界层的应用对湍流垂直扩散系数(Kz)与干沉降速度(V),O3与NOx浓度的影响。结果表明,全边界层应用相似理论明显低估了Kz值,近地层50m处Kz值被低估20%以上,750m处其值被低估约70%;O3、NOx的干沉降速度在日本东部与南部海域被低估了10%以上,在朝鲜半岛东部和西部海域模拟值普遍偏高。Kz和干沉降速度的不同直接影响污染物的浓度和沉降量分布。Kz值的被低估对NOx浓度有明显影响,在近地层50m处NOx浓度最大可增加约30%,整个边界层中NOx平均浓度除台湾省东北海域外普遍增加5%~20%。O3浓度则受干沉降作用的影响较大。虽然近地层、全边界层分别应用相似理论都较好地模拟了O3与NOx峰值浓度出现的时间,但相似理论应用于全边界层会引起较大的误差。即使是大区域、长期空气质量模拟研究,也建议相似理论仅应用于近地层,且模式第一层高度应设置在常通量层内。