底栖有孔虫(Florilus decors)壳体微量元素/钙比值的LA-ICP-MS原位微区分析方法及应用——以长江口外海域为例

深海沉积物中有孔虫壳体的微量元素、同位素测试技术已较为成熟,而河口近海沉积物中有孔虫壳体元素微区测试却鲜有报道。本文报道了一种利用激光剥蚀电感耦合等离子体质谱（LA-ICP-MS）分析法测试取自长江口外沉积物中的有孔虫壳体元素/钙比值的技术,研究了氦气载气流量、能量密度、束斑大小、激光剥蚀频率等参数对测试结果的影响,优化了活体有孔虫原位分析方法。应用确定的测试条件对2016年7月取自长江口外的底栖有孔虫优美花朵虫样品（Florilus decors）进行测试,发现Mg、Sr等元素/钙比值在壳体不同位置上无显著差异,而Mn的数据较为离散,可能与有孔虫生长过程中经历的水环境及其变化有关。     

Three Super Active Regions in the Descending Phase of Solar Cycle 23

We analyze the magnetic configurations of three super active regions, NOAA 10484, 10486 and 10488, observed by the Huairou Multi-Channel Solar Telescope (MCST) from 2003 October 18 to November 4. Many energetic phenomena, such as flares (including a X-28 flare) and coronal mass ejections (CMEs), occurred during this period. We think that strong shear and fast emergence of magnetic flux are the main causes of these events. The question is also of great interest why these dramatic eruptions occurred so close together in the descending phase of the solar cycle.     

Comparative research on karyotype in three species of Arcidae

ＣｏｍｐａｒａｔｉｖｅｒｅｓｅａｒｃｈｏｎｋａｒｙｏｔｙｐｅｉｎｔｈｒｅｅｓｐｅｃｉｅｓｏｆＡｒｃｉｄａｅＺｈｅｎｇＪｉａｓｈｅｎｇ；ＷａｎｇＭｅｉｌｉｎ；ＧｕｏＤａｎｈｏｎｇ；ＸｕＸｉｍｉｎｄａｎｄＧａｏＱｉｎｇｌａｎＡｂｓｔｒａｃｔ：Ｂｙａｉｒ－...     

An algorithm to resolve γ-rays from charged cosmic rays with DAMPE

The DArk Matter Particle Explorer(DAMPE),also known as Wukong in China,which was launched on 2015 December 17,is a new high energy cosmic ray and γ-ray satellite-borne observatory.One of the main scientific goals of DAMPE is to observe Ge V-Te V high energy γ-rays with accurate energy,angular and time resolution,to indirectly search for dark matter particles and for the study of high energy astrophysics. Due to the comparatively higher fluxes of charged cosmic rays with respect to γ-rays,it is challenging to identify γ-rays with sufficiently high efficiency,minimizing the amount of charged cosmic ray contamination. In this work we present a method to identify γ-rays in DAMPE data based on Monte Carlo simulations,using the powerful electromagnetic/hadronic shower discrimination provided by the calorimeter and the veto detection of charged particles provided by the plastic scintillation detector. Monte Carlo simulations show that after this selection the number of electrons and protons that contaminate the selected γ-ray events at～10 Ge V amounts to less than 1% of the selected sample.Finally,we use flight data to verify the effectiveness of the method by highlighting known γ-ray sources in the sky and by reconstructing preliminary light curves of the Geminga pulsar.     

Simultaneous SOHO and Ground-Based Observations of a Large Eruptive Prominence and Coronal Mass Ejection

Coronal mass ejections (CMEs) are frequently associated with erupting prominences near the solar surface. A spectacular eruption of the southern polar crown prominence was observed on 2 June 1998, accompanied by a CME that was well-observed by the LASCO coronagraphs on SOHO. The prominence was observed in its quiescent state and was followed throughout its eruption by the SOHO EIT and later by LASCO as the bright, twisted core of the CME. Ground-based H observations of the prominence were obtained at the Ondejov Observatory in the Czech Republic. A great deal of fine structure was observed within the prominence as it erupted. The prominence motion was found to rotate about its axis as it moved outward. The CME contained a helical structure that is consistent with the ejection of a magnetic flux rope from the Sun. Similar structures have been observed by LASCO in many other CMEs. The relationship of the flux rope to other structures in the CME is often not clear. In this event, the prominence clearly lies near the trailing edge of the structure identified as a flux rope. This structure can be observed from the onset of the CME in the low corona all the way out to the edge of the LASCO field of view. The initiation and evolution of the CME are modeled using a fully self-consistent, 3D axisymmetric, MHD code.     

水脉泽寄主活动星系核的吸积率(英文)

水超脉泽辐射( 各向同性光度超过 10 个太阳光度) 通常在星系中心最内部的核区( 小于几个秒差距) 被发现,因而活动星系核被认为是其唯一的能量源。同其它没有检测到水脉泽辐射的活动星系核相比,水脉泽寄主活动星系核可能隐含着某种或某些特殊性质。基于此我们调研了已经公开发表的所有水脉泽源的 X 射线观测情况,得到了一个有 X 射线观测研究结果的子样本( 39 个源) 。由它们的 X 射线光度以及估算的黑洞质量,导出了它们的无量纲吸积率( logL2-10keV /LEdd,其中 L2-10keV和 LEdd分别是 2 - 10keV 的固有光度和爱丁顿光度) ; 与距离范围相当的、没有检测到水脉泽的活动星系核样本相比,发现脉泽寄主活动星系核有较高的吸积率。进一步分析比较这两个活动星系核样本的质量吸积率,也发现类似的趋势。此外,为了探索吸积率和水脉泽辐射间可能的内在联系,我们对它们的脉泽光度和吸积率进行了统计分析,然而结果显示二者之间没有明显的相关性。     

鲍高效养殖模式的研究

本研究采取苗种强化培育、坑道培育大规格苗种、湖间带鲍参混养等相结合,并配套适当技术措施,促进鲍快速生长,缩短养殖周期一年左右,提高成活率15％以上,增加经济效益200％左右,形成鲍高效养殖的较理想模式。     

太平洋牡蛎人工培育群体的基因型及杂合度研究

实验运用淀粉凝胶电泳的方法检测了１龄养殖太平洋牡蛎Ｃｒａｓｏｓｔｒｅａｇｉｇａｓ５个基因座位上的基因型和杂合度。根据孟德尔自由分离规律,从子代的基因型推断出亲代可能的基因。杂合度的分析表明,人工培育的１龄太平洋牡蛎在Ａａｔ２、Ａｈ１、Ａｈ２、Ｉｄｈ１和Ｌａｐ５个多态位点上的杂合度符合Ｈ－Ｗ平衡规律,未发现明显的杂合子缺失现象。     

四川盆地构造沉降特征及成因机制分析

盆地的沉降过程能够反映盆地的演化历史及成盆机制。为深入分析四川盆地构造沉降特征,本文基于最新钻井资料和地震数据,通过回剥反演方法,进行去压实、沉积负载、古水深和海平面变化校正,重建了四川盆地不同构造单元的构造沉降史。同时根据瞬时均匀伸展模型和裂后热坳陷模型进行正演模拟,对盆地成因进行分析。构造沉降史的恢复揭示了四川盆地具有典型的克拉通盆地沉降特征。四川盆地的形成演化可划分为震旦纪—早古生代、石炭纪—三叠纪、侏罗纪—白垩纪3个构造沉降旋回,盆地经历了晚震旦世—早寒武世、早志留世、晚二叠世—早三叠世以及中晚侏罗世4幕快速沉降,第一幕和第三幕快速沉降期为岩石圈伸展减薄引起,另外两幕为前陆盆地发育过程中所引起的快速沉降。构造沉降正演结果表明四川盆地在寒武纪—奥陶纪和晚二叠世—三叠纪经历了两期“快速沉降—缓慢沉降”过程,快速沉降受控于岩石圈的伸展作用,缓慢沉降为岩石圈热冷却作用所主导。盆地在热冷却沉降阶段后进入前陆挠曲沉降,出现不同规模的剩余沉降。

     

华熊地块中生代岩浆作用的物质继承性

中生代是华熊地块最重要的岩浆作用时期。通过对其中主要地体中燕山期改造型花岗岩和同熔型花岗岩的同位素研究,结合其形成物质背景和地质特征,认为它们的物质特征主要取决于它们继承各自不同的地体物质(特别是基底物质)和同一地体物质的多少程度。地体及其中生代岩浆作用的构造环境是解释这一继承机理的主要因素。