Variation of solar irradiance and mode frequencies during Maunder minimum

Using the sunspot numbers reported during the Maunder minimum and the empirical relations between the mode frequencies and solar activity indices, the variations in the total solar irradiance and 10.7 cm radio flux for the period 1645 to 1715 is estimated. We find that the total solar irradiance and radio flux during the Maunder minimum decreased by 0.19% and 52% respectively, as compared to the values for solar cycle 22. This revised version was published online in July 2006 with corrections to the Cover Date.     

Deepwater Ventilation and Stratification in the Neogene South China Sea

Combined data of physical property, benthic foraminifera, and stable isotopes from ODP Sites 1148, 1146, and 1143 are used to discuss deep water evolution in the South China Sea (SCS) since the Early Miocene. The results indicate that 3 lithostratigraphic units, respectively corresponding to 21-17 Ma, 15-10 Ma, and 10-5 Ma with positive red parameter (a*) marking the red brown sediment color represent 3 periods of deep water ventilation. The first 2 periods show a closer link to contemporary production of the Antarctic Bottom Water (AABW) and Northern Component Water (NCW), indicating a free connection of deep waters between the SCS and the open ocean before 10 Ma. After 10 Ma, red parameter dropped but stayed higher than the modern value (a*=0), the CaCO3 percentage difference between Site 1148 from a lower deepwater setting and Site 1146 from an upper deepwater setting enlarged significantly, and benthic species which prefer oxygen-rich bottom conditions dramatically decreased. Coupled with a major negative excursion of benthic δ13C at ~10 Ma, these parameters may denote a weakening in the control of the SCS deep water by the open ocean. Probably they mark the birth of a local deep water due to shallow waterways or rise of sill depths during the course of sea basin closing from south to east by the west-moving Philippine Arc after the end of SCS seafloor spreading at 16-15 Ma. However, it took another 5 Ma before the dissolved oxygen approached close to the modern level. Although the oxygen level continued to stabilize, several Pacific Bottom Water (PBW) and Pacific Deep Water (PDW) marker species rapidly increased since ~6 Ma, followed by a dramatic escalation in planktonic fragmentation which indicates high dissolution especially after ~5 Ma. The period of 5-3 Ma saw the strongest stratified deepwater in the then SCS, as indicated by up to 40% CaCO3 difference between Sites 1148 and 1146. Apart from a strengthening PDW as a result of global cooling and ice cap buildup on northern high latitudes, a deepening sea basin due to stronger subduction eastward may also have triggered the influx of more corrosive waters from the deep western Pacific. Since 3 Ma, the evolution of the SCS deep water entered a modern phase, as characterized by relative stable 10% CaCO3 difference between the two sites and increase in infaunal benthic species which prefer a low oxygenated environment. Thesubsequent reduction of PBW and PDW marker species at about 1.2 Ma and 0.9 Ma and another significant negative excursion of benthic δ13C to a Neogene minimum at ~0.9 Ma together convey a clear message that the PBW largely disappeared and the PDW considerably weakened in the Mid-Pleistocene SCS. Therefore, the true modern mode SCS deep water started to form only during the "Mid-Pleistocene climatic transition" probably due to the rise of sill depths under the Bashi Strait.     

碳酸盐岩早期差异成储路径及其对储集性能的影响:以滨里海盆地N油田石炭系KT-Ⅰ与KT-Ⅱ层系为例*

以滨里海盆地N油田石炭系KT-Ⅰ与KT-Ⅱ层系碳酸盐岩储集层为例,综合岩心、薄片、扫描电镜、高压压汞、常规物性分析以及各类测试资料,对碳酸盐岩储集层特征以及早期成储路径展开系统研究,并进一步探讨成储路径与储集层孔喉结构和质量的关系。结果表明,KT-Ⅰ层系以云岩类储集层为主,颗粒灰岩次之,其中云岩类储集层以晶间(溶)孔、小型溶洞为主,孔喉连通性好,为高孔—高渗的孔洞型储集层, 而颗粒灰岩类储集层以粒内溶孔、铸模孔及生物体腔孔发育为特征,孔喉连通性差,属中孔—低渗的孔隙型储集层。KT-Ⅱ层系以粒间(溶)孔和生物体腔孔发育的颗粒灰岩为特征,为中高孔—高渗的孔隙型储集层。进一步分析表明,KT-Ⅰ层系云岩与灰岩储集层单旋回厚度小,皆受高频海平面升降变化驱动的早成岩期岩溶的控制, 而KT-Ⅱ层系单旋回厚度大,颗粒滩未经历早期岩溶的改造。 3类储集层的成储路径分别为: (1)KT-Ⅰ云岩类储集层,准同生期白云石化作用导致矿物相转变并使得部分矿物更易遭受溶蚀→早成岩期岩溶作用控制储集层的形成→云岩抗压溶岩石骨架有利于储集层的保护; (2)KT-Ⅰ颗粒灰岩储集层,早成岩期岩溶作用优化储集层→初期压实控制胶结流体通道进而控制胶结作用—粒间孔与粒内孔差异胶结控制储集层的保护; (3)KT-Ⅱ颗粒灰岩储集层,原始沉积环境控制储集层的形成→初期压实与早期胶结作用控制储集层的保护。成储路径差异控制了不同的孔渗特征与孔喉结构,而孔喉结构进一步控制了早期岩溶型云岩、早期岩溶型颗粒灰岩、原生孔保存型颗粒灰岩3种储集层的质量。研究结果将为具类似特征的碳酸盐岩储集层成因分析提供参考,也因发现了云岩较灰岩更易早期溶蚀的现象而具有较为重要的岩溶地质学意义。     

辽宁金杖子地区水系沉积物地球化学特征

金杖子地区位于冀东-辽西金成矿带,区内矿产资源丰富,成矿地质条件优越。本文在1∶25000水系沉积物测量工作的基础上,结合该区地质特征和成矿地质条件,对该地区10种元素的地球化学特征、离散程度及综合异常特征进行研究,圈定综合异常3处,为进一步的地质勘查工作提供了依据。     

云南滇西地区早古生代增生杂岩的厘定及其洋壳俯冲消减作用——基于1∶5万文东幅地质调查的新认识

【研究目的】 澜沧岩群一直存在较大争议,查明澜沧岩群的物质组成、构造属性、时代及变质变形特征具有重要的意义,为进一步重建特提斯的时空格架提供重要的基础资料。【研究方法】 在1∶5万详细野外调查的基础上,系统开展LA-MC-ICP-MS锆石U-Pb年代学等综合研究。【研究结果】 查明了澜沧岩群的物质组成及变质变形特征,具有基质+块体的构造混杂岩特征,经历了3期变质变形,整体表现为逆冲推覆-增生造山的构造变形样式。通过碎屑锆石、变酸性岩锆石U-Pb年代学研究,结合已有的研究资料,厘定其形成时代为早古生代。澜沧岩群中高压变质岩的原岩具有岩浆弧、OIB和E-MORB的特征,说明澜沧岩群经历了深俯冲、增生造山作用过程。【结论】 结合区域已有的研究资料及本文研究成果,认为澜沧岩群不是基底岩系,而是昌宁—孟连原-古特提斯洋俯冲消减形成的早古生代增生杂岩。     

A Full-Sun Magnetic Index from Helioseismology Inferences

Solar magnetic indices are used to model the solar irradiance and ultimately to forecast it. However, the observation of such indices is generally limited to the Earth-facing hemisphere of the Sun. Seismic maps of the far side of the Sun have proven their capability to locate and track medium–large active regions at the non-visible hemisphere. We present here the possibility of using the average signal from these seismic far-side maps, combined with similarly calculated near-side maps, as a proxy to the full-Sun magnetic activity.     

Evolution of the optical spectrum of SN 1987a in the large magellanic cloud

The evolution of the spectrum of SN1987a is traced from 1987 February 26 to March 31. Based on the low-resolution spectroscopic data we identify the lines of H, He I, Na I, Fe II, Sc II, Ca II which are known to be present in Type II Supernovae, and also present evidence for the existence of lines of Mg I, Ca_I, O I, and N I. We discuss the evolution of the Hα profile, and draw attention to its complex structure around March 30. Close to the rest wavelength of Ha a double-peaked structure appeared in the profile with a peak-to-peak separation of ∼ 1400 km s⁻¹, suggestive of an expanding shell or disc of gas. Using the available broadband photometric information, we also trace the evolution of the photosphere of SN1987a assuming that it radiates like a supergiant.