太阳系早期的短寿期放射性核素   总被引：2，自引：0，他引：2  

徐伟彪 《天文学报》2003,44(3):231-239

较详细地介绍全新的太阳系起源理论——X-wind模式,天体化学实验发现太阳系早期存在大量的短寿期放射性核素(半衰期小于100Ma),这些核素对太阳系的形成和演化有重要的影响,一种理论认为,这些核素是在恒星内部合成,并由星风注入原太阳分子云,星风产生的激波诱发分子云核的塌缩而形成原太阳,另一种理论认为,这些核素是高能粒子与原太阳分子云或太阳星云中的气体和尘埃相互作用的产物。  相似文献   

Contributions to the Ring Current Energy During Geomagnetic Storms     

Van Zele  María Andrea 《Studia Geophysica et Geodaetica》2002,46(1):33-41

The purpose of this research was to study the complexity of the energization of the ring current during a geomagnetic storm, produced during southern Bz(IMF) by the injection of plasma sheet ions, accelerated by enhanced convective electric fields. This model assumes that the plasma sheet is continuously populated by H⁺ from the sun and the ionosphere, and sporadically by ionospheric O⁺, making the ring current a coupled system whose energy can hardly be expressed analytically. When Bz(IMF) turns north, the ring current becomes uncoupled, and the energy decays exponentially if the storm is weak, or can be expressed as a combination of exponentials during strong storms representing the quick decay of O⁺ and the slower decay of H⁺, as has been shown.  相似文献   

云台太阳光谱仪像质优良的时间分布规律     

钟树华  王琼珍 《天文研究与技术》2000,(2):11

通过对云台水平式太阳光谱仪 1 982年太阳光谱观测中的成像质量情况统计分析 ,初步得到光谱仪一年中成像质量优良的时间在秋夏 9月和 8月份 ;一天内有两次像质优良的时间 ,上、下午各有一次 ,分别在日出后 2～ 3小时和日落前 3～ 4小时各有半小时到 1小时左右的时间。  相似文献   

中纬度地区的洪水与太阳活动关系的研究     

李可军  向福元  李建勇  顾啸马  李秋莎  陈学昆 《天文研究与技术》2000,(2):82

本文试图说明太阳活动与地球天气气候相关联 ,并用韩国江汉大洪水及我国长江大洪水的事例建立中纬度 (2 0°～ 4 0°)地区的洪水与太阳活动的统计规律 :二者呈负相关 ,大洪水常发生在太阳活动相对宁静的年份。由此本文推断未来几年长江发生大洪水的可能性不大。  相似文献   

1997年3月9日漠河日全食外日冕结构及相对强度分布     

李秋莎  张柏荣 《天文研究与技术》2000,(2):11

利用简单的视频图像采集系统 ,对 1 997年 3月 9日用PanasonicNV -S880EN型摄像机拍摄的黑龙江漠河日全食黄光 (加GG1 1滤光片 )和白光日冕观测资料进行计算处理 ,得到大于 1 .5R⊙ 的太阳活动低年外日冕结构及其相对强度分布。  相似文献   

Ionospheric measurements of relative coronal brightness during the total solar eclipses of 11 August, 1999 and 9 July, 1945     

C. J. Davis  M. Lockwood  S. A. Bell  J. A. Smith  E. M. Clarke 《Annales Geophysicae》2000,18(2):182-190

Swept-frequency (1/10 MHz) ionosonde measurements were made at Helston, Cornwall (50°06N, 5°18W) during the total solar eclipse on August 11, 1999. Soundings were made every three minutes. We present a method for estimating the percentage of the ionising solar radiation which remains unobscured at any time during the eclipse by comparing the variation of the ionospheric E-layer with the behaviour of the layer during a control day. Application to the ionosonde date for 11 August, 1999, shows that the flux of solar ionising radiation fell to a minimum of 25±2% of the value before and after the eclipse. For comparison, the same technique was also applied to measurements made during the total solar eclipse of 9 July, 1945, at Sörmjöle (63°68N, 20°20E) and yielded a corresponding minimum of 16 ± 2%. Therefore the method can detect variations in the fraction of solar emissions that originate from the unobscured corona and chromosphere. We discuss the differences between these two eclipses in terms of the nature of the eclipse, short-term fluctuations, the sunspot cycle and the recently-discovered long-term change in the coronal magnetic field.  相似文献   

Conceptual problems with remote element synthesis     

O. K. Manuel 《Journal of Earth System Science》2000,109(1):195-203

The notion of remote element synthesis has recently been modified to explain the presence of nucleogenetic isotopic anomalies and decay products of short-lived nuclides by injection of a small amount ofexotic nucleogenetic material. Even with this modification, remote element synthesis seems inconsistent with the following observations:

–	Evidence of coupled variations in the chemical and isotopic compositions of the source material for meteorites.
–	Residual coupling of chemical and isotopic heterogeneities across planetary distances in the solar system today.
–	The mass-fractionation relationship seen across isotopes of elements in the planetary system, in the solar wind, and in solar flares.
–	Linkage of short-lived radioactivities with isotopic anomalies and with physical properties of their host grains, as expected for early condensate of fresh stellar debris.
–	Temporal and spatial distributions of short-live nuclides and their decay products.
–	Mirror-image (+ and −) isotopic anomalies in meteorite grains that sum to “normal” isotopic ratios, as expected of unmixed products of the same nuclear reactions that produced our bulk elements.
–	The lac supporting evidence for “presolar” grains or nearby stars that injectedexotic material into the early solar nebula.

  相似文献   

含部分晶须的钛酸锂的制备及其性能表征     

邓昭平  倪师军  李思平  夏新蕊  王鹏威 《矿物岩石》2006,26(4):98-100

L i4T i5O12是一种循环性能好、有很好的充放电平台、理论比容量较大、不与电解液反应的新型负极材料,研究探索以偏钛酸和碳酸锂为主要原料制备含部分晶须的尖晶石型晶型L i4T i5O12的一种方法。通过此工艺在1 000℃煅烧8 h后在样品中约20%的晶须出现,晶须的直径≤0.5μm,晶须的长度约为7μm。  相似文献   

雅鲁藏布江蛇绿岩中超高压矿物硅尖晶石的研究   总被引：3，自引：1，他引：3       下载免费PDF全文

白文吉杨经绥  方青松任玉峰 戎 合施倪承  李国武马喆生 《中国地质》2006,33(6):1379-1385

从西藏雅鲁藏布江蛇绿岩带的罗布莎蛇绿岩的铬铁矿中，发现一个由70-80种奇异矿物组成的地幔矿物群，其中包括一种成分特殊的尖晶石类矿物。该种尖晶石呈包裹体分布在毒砂中，28粒该矿物的平均化学成分：Na2O 1.58％，MgO7．52％，Al2O3 36．59％，SiO2 44．45％，FeO 8．72％，并含少量CaO和TiO2。经激光拉曼谱仪测试，一部分颗粒具有Franclinite（锌铁尖晶石ZnFe2O4）拉曼谱。根据尖晶石结构和化学成分，可以得出两种分子式：（Mg0．52Na0．14Fe0.32Al0.74）1.72（Si2.00Al1.20）3.20O8和（Mg0.52Na0.14Fe0.32Si0.50）1.48相（Si1.50Al1.94）3．44O8。两种分子式都表明阳离子Si呈六配位占据尖晶石八面体晶格位置。Si离子呈六配位的硅酸盐。实验证明具有超高压性质，来自相当于过渡带400-670km的深部。表明西藏雅鲁藏布江蛇绿岩（古大洋岩石圈）的岩浆活动达到过渡带。可能是地幔柱活动将硅尖晶石类等超高压矿物搬运到上地幔浅部的。  相似文献   

电感耦合等离子体发射光谱法测定键合用硅铝丝中硅铁铜     

宋小年  冯天培 《岩矿测试》2006,25(2):189-190196

采用电感耦合等离子体发射光谱法测定硅铝丝（Al—1％Si）中Si及杂质元素Fe和Cu。确定了最少取样量和样品溶解方法，优化了元素分析谱线和仪器的测量条件。实验表明，方法的加标回收率为99％～1叭％，相对标准偏差（n=6）低于1．4％，Si、Fe、Cu的检出限分别为8．5、1．0和0．4μg／L。该方法应用于快速测定键合硅铝丝中的各种元素，结果满意。  相似文献