Unstable kinetic Alfvén wave in partially ionized plasma

The stability of kinetic Alfven waves is discussed for a partially ionized plasma with a flux of ionizing electrons which balance the plasma particle losses. Accidental electromagnetic perturbations are shown to be unstable due to the energy change of ionizing electrons.     

利用ADS40立体影像建立一体化数字线划图生产体系

为提高数字线划图生产的效率,本文基于ADS40立体影像测图技术,综合利用遥感技术、摄影测量技术、GIS技术及数据库系统,提出了一种一体化数字线划图生产方案。该方案通过嫁接航天远景MapMatrix以及清华山维EPS两个平台,实现针对ADS40相机L1级影像从数据读取、立体模型构建、立体采集、DLG处理以及最终形成GIS入库数据的整个处理流程。实验证明,本文提出的工作方案是利用遥感技术提升城市大比例尺地形图生产、缩短更新周期的有效方案。     

Field Trips as Valuable Learning Experiences in Geography Courses

Abstract

Field trips have been acknowledged as valuable learning experiences in geography. This article uses Kolb’s (1984) experiential learning model to discuss how students learn and how field trips can help enhance learning. Using Kolb’s experiential learning theory as a guide in the design of field trips helps ensure that field trips contribute to internalizing relevant geographical theory and concepts. Three types of field trips are presented: an informal survey of a neighborhood, a more formal scavenger hunt, and a virtual field trip using Google Earth.

Learning is the process whereby knowledge is created through the transformation of experience.

—Kolb (1984)     

基于ADS 40数据的现状图测绘

新疆伊犁河谷土地开发整理现状图测绘由于其作业范围广,精度要求高,采用了ADS 40数字航空摄影数据。本文主要阐述了基于ADS 40数据进行航测外业和内业完成伊犁河谷4 000 km2的现状图测绘的生产过程。     

The Antarctic oscillation-East Asian summer monsoon connections in NCEP-1 and ERA-40

Connections between the spring Antarctic Oscillation(AAO)and the East Asian summer monsoon (EASM)in two reanalysis datasets—NCEP-1(NCEP/NCAR Reanalysis 1)and ERA-40(ECMWF 40- year Reanalysis)—are investigated in this study.Both show significant correlation between AAO and EASM rainfall over the Yangtze River valley,especially after about 1985.Though ERA-40 shows weaker anomalous signals connecting AAO and EASM over southern high latitudes than NCEP-1,both datasets reveal similar connecting patterns between ...     

New magnetic field measurements of β Cephei stars and slowly pulsating B stars

We present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B‐type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B‐type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three β Cephei stars and two stars suspected to be β Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3σ has been diagnosed in two normal B‐type stars, the nitrogen‐rich early B‐type star HD 52089 and in the B5 IV star HD 153716. Roughly one third of β Cephei stars have detected magnetic fields: Out of 13 β Cephei stars studied to date with FORS 1, four stars possess weak magnetic fields, and out of the sample of six suspected β Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: Roughly half of the 34 SPB stars have been found to be magnetic and among the 16 candidate SPBs eight stars possess magnetic fields. In an attempt to understand why only a fraction of pulsating stars exhibit magnetic fields, we studied the position of magnetic and non‐magnetic pulsating stars in the H‐R diagram. We find that their domains in the H‐R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. It is possible that stronger fields tend to be found in stars with lower pulsating frequencies and smaller pulsating amplitudes. A somewhat similar trend is found if we consider a correlation between the field strength and the v sin i ‐values, i.e. stronger magnetic fields tend to be found in more slowly rotating stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

What is the closest black hole to the Sun?

We examine the distance of the two galactic microquasars GRO J1655–40 and A 0620–00 which are potentially the two closest black holes to the Sun. We aim to provide a picture as wide and complete as possible of the problem of measuring the distance of microquasars in our Galaxy. The purpose of this work is to fairly and critically review in great detail every distance method used for these two microquasars in order to show that the distances of probably all microquasars in our Galaxy are much more uncertain than currently admitted. Moreover, we show that many confirmations of quantitative results are often entangled and rely on very uncertain measurements. We also present a new determination of the maximum distance of GRO J1655–40 using red clump giant stars, and show that it confirms our earlier result of a distance less than 2 kpc instead of 3.2 kpc. Because, it then becomes more likely that GRO J1655–40 could originate from the stellar cluster NGC 6242, located at 1.0 kpc, we review the distance estimations of A 0620–00, which is so far the closest black hole with an average distance of about 1.0 kpc. We show that the distance methods used for A 0620–00 are also problematic. Finally, we present a new analysis of spectroscopic and astrometric archival data on this microquasar, and apply the maximum distance method of Foellmi et al. [Foellmi, C., Depagne, E., Dall, T.H., Mirabel, I.F., 2006b. A&A 457, 249]. It appears that A 0620–00 could indeed be even closer to the Sun than currently estimated, and consequently would be the closest known black hole to the Sun.     

四川省九龙县黑牛洞富铜矿矿床黑云母40Ar-39Ar测年及其地质意义

四川省九龙县黑牛洞铜矿床为近期新发现的一个规模在中型以上,产于江浪变质核杂岩中的富铜矿床。本文测试了黑牛洞铜矿床中与成矿密切相关的黑云母的40Ar/39Ar年龄为136.43±0.77 Ma,说明黑牛洞矿床形成于燕山中期。结合矿区附近李伍富铜床矿床地质特征及成矿年龄,表明黑牛洞铜矿床与李伍铜矿床为同一时期形成的矿床,两者成矿与松潘－甘孜造山带大规模岩浆热事件有关,这对于重新认识李伍铜矿床外围找矿潜力和进一步指导找矿工作具有重要意义。     

川西北花岗岩的冷却过程及其对区域成矿的制约

川西北地区位于松潘-甘孜造山带北部,产出众多的中生代花岗岩和卡林型金矿,金成矿作用与区域构造运动和岩浆活动有密切的内在联系。本文拟从花岗岩的角度分析这种内在联系,故测定了川西北的羊拱海黑云母二长花岗岩、达盖寨黑云母二长花岗岩和可尔因二云母二长花岗岩的黑云母或白云母Ar-Ar年龄,分别得到坪年龄158.7±1.4Ma、185.2±1.4Ma、和157.6±1.2Ma,并参考积累的川西北花岗岩体的年代学数据,绘制了造山带北部、中部、东缘中部几个主要花岗岩体的冷却轨迹。不同构造位置花岗岩体的冷却轨迹表明,从造山带北部到造山带东缘中部,各花岗岩体的侵位年龄依次变新,冷却速率依次变缓,在区域构造运动相对较弱期间,各花岗岩的冷却速率明显降低。由以上特征,本文推断在中生代陆内造山过程中,构造应力自松潘-甘孜造山带北部向造山带东缘中部传递,各区域先后由造山相对活跃期进入造山相对宁静期。在造山宁静期,构造运动较弱,花岗岩体缓慢冷却,地壳较长时间保持低温状态,利于金的成矿作用。因而,川西北的金矿主要形成于区域花岗岩的缓慢冷却阶段,这可能是金矿与花岗岩时空耦合的原因之一。     

西秦岭北缘新阳—元龙韧性剪切带中花岗质糜棱岩黑云母40Ar 39Ar年龄及地质意义

西秦岭北缘新阳-元龙大型韧性剪切带是分划西秦岭造山带与祁连造山带的区域主构造边界,通过对其物质组成和构造特征的研究,结合两侧不同(洋-陆)构造环境下各类地质体的研究成果,重点对剪切带内花岗质糜棱岩中黑云母单矿物进行了~(40)Ar-~(39)Ar定年研究.在新阳镇和元龙北剪切带中分别获得(347.95±2.17)Ma (MSWD＝1.89)和(351.70±1.72)Ma (MSWD＝0.80)的坪年龄,分析确定其应为黑云母的冷却年龄,表明变形时代应在早石炭世早期之前;反映了最晚在早石炭世早期,该剪切带已横切秦岭与祁连造山带并发生强烈的右行走滑构造拼贴作用.