Magnetic Field Strengths and Structures from Radio Observations of Solar Active Regions

Radio observations of some active regions (ARs) obtained with the Nobeyama radioheliograph at λ=1.76cm are used for estimating the magnetic field strength in the upper chromosphere, based on thermal bremsstrahlung. The results are compared with the magnetic field strength in the photosphere from observations with the Solar Magnetic Field Telescope (SMFT) at Huairou Solar Observing Station of Beijing Astronomical Observatory. The difference in the magnetic field strength between the two layers seems reasonable. The solar radio maps of active regions obtained with the Nobeyama radioheliograph, both in total intensity (I-map) and in circular polarizations (V-map), are compared with the optical magnetograms obtained with the SMFT. The comparison between the radio map in circular polarization and the longitudinal photospheric magnetogram of a plage region suggest that the radio map in circular polarization is a kind of magnetogram of the upper chromosphere. The comparison of the radio map in total intensity with the photospheric vector magnetogram of an AR shows that the radio map in total intensity gives indications of magnetic loops in the corona, thus we have a method of defining the coronal magnetic structure from the radio I-maps at λ=1.76 cm. Analysing the I-maps, we identified three components: (a) a compact bright source; (b) a narrow elongated structure connecting two main magnetic islands of opposite polarities (observed in both the optical and radio magnetograms); (c) a wide, diffuse, weak component that corresponds to a wide structure in the solar active region which shows in most cases an S or a reversed S contour, which is probably due to the differential rotation of the Sun. The last two components suggest coronal loops on different spatial scales above the neutral line of the longitudinal photospheric magnetic field.     

干旱地区自然资源开发和利用国际学术讨论会即将在乌鲁木齐召开

经上级批准,中国科学院新疆分院将于1985年8月7日至13日在乌鲁木齐召开《干旱地区自然资源开发和利用国际学术讨论会》。会议主要内容是:1.水土资源合理开发利用;2.动植物资源保护和利用;3.盐碱土改良和利用;4.沙漠治理和利用;5.环境与生态变化等。     

辽东湾凝析气田超压成因及侧向传递机制初探

位于辽东湾西部低凸起北端的JZ20-2超压凝析气田,离供烃中心较远,压力系数却达到1.56~1.7,这在我国东部裂谷盆地比较少见。经过综合分析,作者认为JZ20-2凝析气田异常高压的形成与其所处的特殊地质背景紧密相关,辽中凹陷沙河街组三段超压凝析油气沿不整合面、砂体输导通道向辽东湾西部低凸起的运移、充注和能量的侧向传递是JZ20-2凝析气田异常高压形成的根本原因,而上覆东营组二段下亚段-东营组三段巨厚的强超压泥岩封盖和辽西3号边界断层侧向遮挡共同构成的优越封闭环境是超压保存的必要条件。本文分析了该气田超压特征及其远距离超压侧向传递的成因机制,不仅有助于揭示辽东湾西部低凸起超压流体运移聚集的规律和成藏作用,而且可能提供了一个超压远距离侧向传递的典型实例。     

渤海新近系浅水三角洲沉积体系与大型油气田勘探

新近纪渤海具有构造稳定、沉降缓慢、湖泊水域范围大、内部无分割、地形平缓、坡度小等特点,广泛发育浅水三角洲,从而形成渤海海域新近系良好的储盖组合和优越的油气成藏条件。浅水三角洲砂岩储层由于受河流作用的控制,砂体具有明显的方向性,存在明显的分叉现象,与曲流河相比,砂体连通性较好,砂体等厚图呈典型的朵叶状。湖相厚层泥岩普遍发育,与浅水三角洲砂体组成多套垂向优质储盖组合。浅水三角洲发育于渤海新近纪至今处于生烃的峰期主力富烃凹陷的有利区带,新构造运动造成新近纪以来凹陷主力源岩生烃峰期与新构造运动的同步耦合,为渤海大型浅水三角洲成因的优质储层油气成藏创造了优越条件,可以形成大型油气田。因此,重视并充分挖掘渤海浅水三角洲储层类型油气藏的勘探潜力将是追求浅层优质油藏、进一步增储上产的方向所在。     

鉴江河口底泥盐度释放规律研究

底泥盐度释放是河口水资源利用的主要限制因子。本文以鉴江为例,基于野外实测与室内实验,系统分析了鉴江河口底泥盐度及水体氯离子的分布特征;通过振荡、换水及静态等实验。定量研究了河口底泥盐度释放规律。结果表明：（1）潮泛河口底泥盐度主要受上溯潮水的影响。有较为明显的梯度性;（2）底泥盐度释放量在初期较大,随着换水周期的累加,则逐步降低;在同一换水周期。底泥盐度释放强度与其本底盐度浓度成正指数关系;（3）静态释放时间越长,上覆水盐度越大。静置30d。三组样品上覆水的浓度分别达2626mg·L-1、932mg·L-1、533mg·L-1。远远超过用水水质的要求。     

桩静载荷试验快速法与慢速法对比研究

通过对54根管桩静载荷试验快速法与慢速法对比试验研究,找出了在各级荷载作用下,快速法与慢速法沉降差异规律及快速法与慢速法分别得出的极限承载力差异规律;得出了将快速法静载试验下的沉降及单桩极限承载力修正成慢速法静载试验的沉降及单桩极限承载力的公式;提出了适应天津地区管桩的快速法静载试验方法。     

莱州市海湾扇贝秋季自然海区半人工采苗初获成功

莱州湾东南岸海湾扇贝每年秋季都自行产卵。笔者在栉孔扇贝半人工采苗取得极大成功的启示下，经过４年探索，终于在１９９２年取得了海湾扇贝秋季自然海区半人工采苗的试验成功，共投放采苗袋１００个，采苗２０×１０４粒左右。１９９２年１１月２８日特邀请中科院海洋研究所张福绥研究员首次到莱州指导工作，经检查每袋采苗量２１００多粒，壳高２～３ｍｍ。目前笔者正进一步研究海湾扇贝秋苗的越冬问题和在生产中的应用价值。莱州市海湾扇贝秋季自然海区半人工采苗初获成功@李学祥@周经济