1956年1月9日至14日在中国的北京和匈牙利的索坡倫两处同时观测大地电流的结果

在不久以前關於大地電流場的研究曾受到了一番鼓舞。C.和M.斯郎波澤曾指出大地電流是一個新的地球物理勘探法的基礎,因此人們已經注意研究這些電流的本質和它們與地磁及天電的關係。闕於這一方面的基本文獻是M.斯郎波澤和G.孔湼茲的論文,在此論文里也包含着關於大地電流的振盪的研究。這篇論文是根據在     

中国大陆科学钻探工程主孔3000～3500 m花岗质片麻岩地球化学性质及其成因机制

中国大陆科学钻探工程主孔(CCSD-MH)3000~3500m深度范围内的岩心揭示的主要岩石类型以正、副片麻岩为主,夹少量的榴辉岩、片岩及斜长角闪岩等。正片麻岩可进一步划分为钾长花岗质片麻岩和二长花岗质片麻岩。地球化学研究表明,花岗质片麻岩的SiO2含量普遍高,为73.56%~79.01%,Al2O3含量为10.49%~13.75%;TiO2、Fe2O3、FeO、MnO和MgO的含量明显偏低,其中Fe2O3为0.26%~2.56%,FeO为0.09%~1.13%,MgO为0.01%~0.63%;岩石明显富含Na2O、K2O,强烈贫钙,Na2O K2O的含量为6.20%~9.15%,K2O的含量为1.26%~5.67%,CaO的含量为0.08%~1.59%。花岗质片麻岩在洋脊玄武岩标准化蛛网图上都表现出强烈富集大离子亲石元素(K、Rb、Th)的特点,高场强元素Ti、Ta和Nb表现为明显的负异常,而Hf和Zr则为明显正异常。3000~3500m花岗质片麻岩的原岩具A型花岗岩的特征,形成于大陆裂谷环境,记录了Rodinia超大陆裂解时苏鲁地区的花岗岩浆事件,表明新元古代晚期扬子板块北缘的构造属性为大陆裂谷环境。     

Volatiles,vesicles, and vugs: Unraveling the magmatic and eruptive histories of Steno crater basalts

In 1972, Apollo 17 astronauts returned 170.4 kg of lunar material. Within 1 month of their return, a subset of those samples was specially curated with the forethought that future analytical techniques would offer new insight into the formation and evolution of the Moon. Of interest in this work is sample 71036, a basalt collected from the rim of Steno crater in the Taurus–Littrow Valley, which was stored frozen and was processed and released for study 50 years later. We report, for the first time, the detailed mineralogy and petrology of 71036 and its companion samples 71035, 71037, and 71055 using a novel combination of 2-D and 3-D methods. We investigate lunar volatiles through in situ measurements of apatite and 3-D measurements of vesicles to understand the degassing histories of the Steno crater basalts. Our coupled 2-D petrography and 3-D tomography data sets support a model of the Steno crater basalts crystallizing in the upper crust of a mare lava flow. Apatite F and OH chemistry and the late-stage deformation of voids and formation of smaller vesicles provide evidence supporting coeval degassing of volatiles and crystallization of mesostasis apatite in Apollo 17 basalts. This work helps to close knowledge gaps surrounding the origin, magmatic evolution, emplacement, and crystallization history of high-titanium basalts.     

AsteroFLAG: First results from hare‐and‐hounds Exercise #1

We report on initial results from the first phase of Exercise #1 of the asteroFLAG hare and hounds. The asteroFLAG group is helping to prepare for the asteroseismology component of NASA's Kepler mission, and the first phase of Exercise #1 is concerned with testing extraction of estimates of the large and small frequency spacings of the low‐degree p modes from Kepler‐like artificial data. These seismic frequency spacings will provide key input for complementing the exoplanet search data. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)