基于Van Allen Probes EMFISIS波动仪器观测的内磁层上频带哨声合声波全球分布的统计分析

基于Van Allen Probes近三年的EMFISIS仪器波动观测数据,针对内磁层上频带哨声模合声波幅度的全球分布特性对地磁活动水平的依赖性进行了详细的统计分析,着重研究上频带合声波平均场强幅度随磁壳值(L)、磁地方时(MLT)、地磁纬度(MLAT)的分布特征及不同强度区间的合声波的发生概率.结果表明,上频带合声波的平均场强幅度与地磁活动条件密切相关,在强磁扰期,平均幅度可达到40 pT以上.在外辐射带中心区域(L=4~6),上频带合声波的幅度最强;在L~3的区域,上频带磁层合声波没有分布.在夜侧至晨侧(22—09MLT),上频带合声波幅度最强;在下午侧至昏侧(15-19MLT),上频带合声波幅度最弱;日侧(10-14MLT)上频带合声波在不同地磁活动条件下都存在,幅度偏小.上频带合声波主要分布在|MLAT|10°,其中21-09MLT范围内、磁纬位于|MLAT丨5°的平均场强幅度最强,磁扰期间可达约100 pT.另外,统计而言,中等幅度(10~30 pT)的上频带合声波在夜侧至晨侧(23-09MLT)靠近磁赤道区域的发生率最高,可达15%左右.强幅度(30 pT)的上频带合声波普遍分布在夜侧(01-05MLT),发生率最小.本文建立的上频带哨声模合声波的全球分布模型结合已经建立的下频带合声波的全球分布模型,将有助于进一步深入理解该重要磁层等离子体波动对地球等离子体片、辐射带、环电流动力学过程的定量贡献.     

Optimal subreflector position determination of shaped dual-reflector antennas based on the parameters iteration approach

A new method based on the parameters iteration technique has been developed to determine the optimal subreflector position for shaped Cassegrain antennas, that are distorted by gravity, to improve their electromagnetic(EM) performance. Both the features of shaped surface and the relationship between optical path difference(OPD) and far field beam pattern are employed. By describing the shaped dualreflector surface as a standard discrete parabola set, we can utilize the optical features of the standard Cassegrain system in the classical OPD relationship. Then, the actual far field beam pattern is expressed as the synthesis of ideal beam and error beam by decomposing subreflector adjustment parameters using a mechanical-electromagnetic-field-coupling-model(MEFCM). Furthermore, a numerical method for determining optimal subreflector position is presented. The proposed method is based on the iteration technique of subreflector adjustment parameters, and the optimal far field pattern is used for the iteration. The numerical solution of optimal adjustment parameters can be obtained rapidly. Results for a 25 m shaped Cassegrain antenna demonstrate that the adjustment of the subreflector to the optimal position as determined by the proposed method can improve the EM performance effectively.     

A low-latency pipeline for GRB light curve and spectrum using Fermi/GBM near real-time data

Rapid response and short time latency are very important for Time Domain Astronomy, such as the observations of Gamma-ray Bursts(GRBs) and electromagnetic(EM) counterparts of gravitational waves(GWs). Based on near real-time Fermi/GBM data, we developed a low-latency pipeline to automatically calculate the temporal and spectral properties of GRBs. With this pipeline, some important parameters can be obtained, such as T_(90) and fluence, within ～ 20 min after the GRB trigger.For ～ 90% of GRBs, T_(90) and fluence are consistent with the GBM catalog results within 2σ errors.This pipeline has been used by the Gamma-ray Bursts Polarimeter(POLAR) and the Insight Hard Xray Modulation Telescope(Insight-HXMT) to follow up the bursts of interest. For GRB 170817 A, the first EM counterpart of GW events detected by Fermi/GBM and INTEGRAL/SPI-ACS, the pipeline gave T_(90) and spectral information 21 min after the GBM trigger, providing important information for POLAR and Insight-HXMT observations.     

Generation of GHZ state and cluster state with atomic ensembles via the dipole—blockade mechanism

This paper proposes scalable schemes to generate the Greenberger--Horne--Zeilinger (GHZ) state and the cluster state with atomic ensembles via the dipole blockade mechanism on an atom chip, where the qubit is not carried by a single atom but an atomic ensemble. In the protocols, multiqubit entangled states are determinately prepared. Needlessness for single-photon source further decreases the complexity of the experiment. Based on the present laboratory technique, the schemes may be realized. The achieved results reveal a prospect for large-scale quantum communication and quantum computation.     

经济海藻羊栖菜(Sargassum fusiforme)受精卵生物活性物质及矿质元素成分分析

为了综合评价经济海藻羊栖菜(Sargassum fusiforme)受精卵的营养价值及开发利用前景,本文检测了羊栖菜受精卵碳水化合物、膳食纤维、氨基酸、脂肪酸等生物活性物质与矿质元素成分,并与文献报道的孢子体相应成分进行了比较。结果发现:羊栖菜受精卵富含碳水化合物、蛋白质、氨基酸及膳食纤维,其含量分别为(20.4±0.07)、(22.7±0.03)、(16.7±0.04)和(39.2±0.03)g/100g DW;谷氨酸、维生素E和β-类胡萝卜素含量尤其高,分别达到(9.82±0.05)g/100g DW、(11.8±0.01)mg/100g DW和(3.0×103±7.07)μg/100gDW;而脂肪含量偏低,只有1.03%。矿质元素中微量元素铁、钙和镁的含量较高,分别为(4.54×103±49.50)、(1.83×103±7.78)和(1.40×103±28.28)mg/100g DW。通过与文献报道的羊栖菜孢子体生化成分相比较,羊栖菜受精卵中蛋白质、氨基酸、β-类胡萝卜素、钾、钠、磷、铁、钙、锌、锰及铜元素的含量均高于羊栖菜孢子体。说明羊栖菜受精卵具有更高的天然产物提取、开发和利用价值。     

地震低频信息缺失特征分析及拓频方法研究（英文）

地震低频信息能够提高分辨率与成像精度,改善反演质量,甚至直接进行油气检测,需要对其进行有效保护与拓展。对于子波而言,缺失低频信息会导致主瓣幅度降低、第一旁瓣幅度增加,并出现次级旁瓣呈周期震荡衰减的现象;从合成地震记录和典型地质模型来看,低频缺失会产生假同相轴,造成分辨率提高的假象,且模型不同位置的特征存在一定差异;对缺失低频的模型数据进行波阻抗反演,会造成构造失真、岩性改变的假象,特别是高陡构造和薄互层。针对缺失低频的地震资料,本文还研究了基于压缩感知与稀疏约束的拓频方法,开发了相应的模块,并对实际CIP道集进行处理,取得了较好的应用效果。     

X-Ray Afterglows of GRBs 050318 and 060124 and their External Shock Origin

The observations with Swift X-ray telescope (XRT) challenge the conventional gamma-ray burst model in many aspects. The XRT light curves are generally composed of four consecutive segments, i.e., a steep decay segment, a shallow decay segment, a normal decay segment, a jet-like steep decay segment, and sometimes erratic flares as well. The phys-ical origin of the X-ray emission is highly debatable. We focus here on the physical origin of the X-ray emissions of GRBs 050318 and 060124. We present the XRT light curves and spectra of the two bursts. The light curve decay slopes of the two bursts are normal, and their relations to the spectral indices are consistent with the prediction of the standard forward shock model. The multi-wavelength light curves at 0.5keV, 1.0keV, 2.0keV and 4.0keV can be reproduced by this model with an isotropic kinetic energy Ek = 2.2×1052 erg, e = 0.04, B = 0.01 for GRB 050318 and Ek = 4.2×1053 erg, e = 0.05, B = 0.01 for GRB 060124. These facts suggest that the normal decay phases of the X-rays for the two bursts are of the forward shock origin.     

基于形态学和16S rRNA基因序列的轮螺科面盘幼虫物种鉴定

轮螺科(Architectonicidae)是一类成体螺壳右旋而面盘幼虫螺壳左旋的腹足类,其面盘幼虫在国内一直被误定为强卷螺属(Agadina)种类,归在螔螺科(Limacinidae)中。本文基于线粒体16SrRNA基因序列和胚壳的形态特征,对轮螺科面盘幼虫进行了物种鉴定。结果表明,根据胚壳壳顶和脐孔的形态特征,面盘幼虫可大致分为2种明显不同的形态类型:形态类型I的个体壳扁,壳顶凹陷,脐孔形状规则,圆而深;形态类型II的个体壳顶突出,脐孔形状不规则,浅或深,肛区龙骨有或无。GMYC(GeneralizedMixedYuleCoalescent)和ABGD(AutomaticBarcodingGapDiscovery)分析显示,轮螺科面盘幼虫16S rRNA基因的50种单倍型形成19个分子可操作分类单元(molecular operationaltaxonomic units,MOTUs),同一MOTU的幼虫具有相同的胚壳形态。其中,11个MOTUs中的幼虫属于形态类型I,8个MOTUs中的幼虫属于形态类型II。此外,不同MOTUs的面盘幼虫,其软体部黑色幼体器官(Black Larval Organ)的位置和大小也不同。根据研究结果推测,轮螺面盘幼虫的形态具有种或属特异性。轮螺科面盘幼虫单倍型形成的MOTU数量明显多于国内目前已记录的物种数,其种类多样性可能被低估。基于16SrRNA序列能直接鉴定到种的仅Psilaxisradiatus和配景轮螺(Architectonica perspectiva)2种。本文也从分子水平订正了国内长期以来的分类错误。     

第23太阳活动周期太阳风参数及地磁指数的统计分析

日冕物质抛射(Coronal Mass Ejection,简称CME)和共转相互作用区(Corotating Interaction Region,简称CIR)是造成日地空间行星际扰动和地磁扰动的两个主要原因,提供了地球磁暴的主要驱动力,进而显著影响地球空间环境.为深入研究太阳风活动及受其主导影响的地磁活动的时间分布特征,本文对大量太阳风参数及地磁活动指数的数据进行了详细分析.首先,采用由NASA OMNIWeb提供的太阳风参数及地磁活动指数的公开数据,通过自主编写matlab程序对第23太阳活动周期(1996-01-01—2008-12-31)的数据包括行星际磁场Bz分量、太阳风速度、太阳风质子密度、太阳风动压等重要太阳风参数及Dst指数、AE指数、Kp指数等主要的地磁指数进行统计分析,建立了包括269个CME事件和456个CIR事件列表的数据库.采用事例分析法和时间序列叠加法分别对两类太阳活动的四个重要太阳风参数(IMF Bz、太阳风速度、太阳风质子密度、太阳风动压)和三个主要地磁指数(Dst、AE、Kp)进行统计分析,并研究了其统计特征.其次,根据Dst指数最小值确定了第23太阳活动周期内的355个孤立地磁暴事件,并以Dst指数最小值为标准将这些磁暴进一步分类为145个弱磁暴、123个中等磁暴、70个强磁暴、12个剧烈磁暴和5个巨大磁暴.最后,采用时间序列叠加法对不同强度磁暴的太阳风参数和地磁指数进行统计分析.统计分析表明,对于CME事件,Nsw/Pdyn(Nsw表示太阳风质子密度,Pdyn表示太阳风动压)线性拟合斜率一般为正;对于CIR事件,Nsw/Pdyn线性拟合斜率一般为负,这可作为辨别CME和CIR事件的一种有效方法.从平均意义上讲,相较于CIR事件,CME事件有更大的南向IMF Bz分量、太阳风动压Pdyn、AE指数、Kp指数以及更小的Dstmin.一般情况下,CME事件有更大的可能性驱动极强地磁暴.总体而言,对于不同强度的地磁暴,Dst指数的变化呈现出一定的相似性,但随着地磁暴强度的增强,Dst指数衰减的速度变快.CME和CIR事件以及其各自驱动的地磁暴事件有着很多不同,因此,需要将CME事件驱动的磁暴及CIR事件驱动的磁暴分开研究.建立CME、CIR事件及地磁暴的数据库以及获取的统计分析结果,将为深入研究地球磁层等离子体片、辐射带及环电流对太阳活动的响应特征提供有利的帮助.     

岩石塑性变形条件下的Mohr-Coulomb屈服准则

传统的Mohr-Coulomb强度准则仅描述了峰值强度状态下正应力和剪应力之间的关系,作为岩石破坏的判据.本文拓展概念,提出Mohr-Coulomb屈服准则表述岩石发生塑性变形后不同应力状态下屈服面的应力应变关系.在总结实验研究的基础上建立了使用三轴压缩试验数据确定塑性参数c和φ随内变量κ变化的实验技术方法,给出了评价各向同性模型精度的参量表达以及某些测试结果.采用具有各向同性强(软)化规律的Mohr-Coulomb屈服准则,利用岩石的初始屈服、峰值屈服和残余屈服三组参数可以将全过程应力应变曲线简化表征为四直线模型,它比三线性模型有更广泛的适用性.本文的结果为工程地质数值模拟提供了理论和实验基础,具有指导意义.