中子星自洽的有限磁层大气模型

本文讨论的是中子星自洽的有限磁层大气模型,先用试探解方法得到一个解析解,它给出有限磁层大气的分布轮廓,然后用能量最小原理讨论了其特性,取得了有意义的结果。同时,通过对其等离子体与真空交界面的研究,得出其交界面也是稳定的。最后,我们对模型的发展作了展望,指出赤道区的超共转,可能与子脉冲漂移有关,从这个模型出发,我们将可能最终建立一个自洽的有辐射的模型。     

Secular influence of change in the heliocentric gravitation constant <Emphasis Type="Italic">GM</Emphasis><Subscript>⊙</Subscript> on evolution of orbits of Meteor Streams

The Secular influence of the change in the heliocentric gravitational constant on the evolution of orbits of Meteor Streams is examined by using the method of celestial mechanics with variable mass and variable gravitational constant. The change in the heliocentric gravitational constant includes the combined changes in the sun’s mass and gravitational constant obtained from the modern observation of planets and spacecraft. The perturbation equations are solved by expanding series with mean anomaly. The solutions of the secular and periodic variation of orbital elements are derived. The theoretical results for the secular variables of the semi-major axes, solar distances at perihelion and orbital periods are given for three Meteor Streams: Dracorids, Quadrantids, and Ursids. The numerical results are shown in Table 2. The discussion and conclusion are drawn.     

The “Same Side – Opposite Side Effect” of the Heliospheric Current Sheet in Ionospheric Negative Storms

Using 141 CME-interplanetary shock (CME-IPS) events and foF2 from eight ionosonde stations from January 2000 to September 2005, from the statistical results we find that there is a “same side?–?opposite side effect” in ionospheric negative storms, i.e., a large portion of ionospheric negative disturbances are induced by the same-side events (referring to the CMEs whose source located on the same side of the heliospheric current sheet (HCS) as the Earth), while only a small portion is associated with the opposite-side events (the CMEs source located on the opposite side of the HCS as the Earth); the ratio is 128 vs. 46, and it reaches 41 vs. 14 for the intense ionospheric negative storms. In addition, the ionospheric negative storms associated with the same-side events are often more intense. A comparison of the same-side event (4 April 2000) and the opposite-side event (2 April 2001) shows that the intensity of the ionospheric negative storm caused by the same-side event is higher than that by the opposite-side event, although their initial conditions are quite similar. Our preliminary results show that the HCS has an “impeding” effect to CME-IPS, which results in a shortage of energy injection in the auroral zone and restraining the development of ionospheric negative perturbations.     

Revisiting vertical structure of neutrino-dominated accretion disks: Bernoulli parameter, neutrino trapping and other distributions

We revisit the vertical structure of neutrino-dominated accretion flows (NDAFs) in spherical coordinates with a new boundary condition based on the mechanical equilibrium. The solutions show that NDAF is significantly thick. The Bernoulli parameter and neutrino trapping are determined by the mass accretion rate and the viscosity parameter. According to the distribution of the Bernoulli parameter, the possible outflow may appear in the outer region of the disk. The neutrino trapping can essentially affect the neutrino radiation luminosity. The vertical structure of NDAF is like a “sandwich”, and the multilayer accretion may account for the flares in gamma-ray bursts.     

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.     

A model of fast radio bursts: collisions between episodic magnetic blobs

Fast radio bursts(FRBs) are bright radio pulses from the sky with millisecond durations and Jansky-level flux densities. Their origins are still largely uncertain. Here we suggest a new model for FRBs. We argue that the collision of a white dwarf with a black hole can generate a transient accretion disk, from which powerful episodic magnetic blobs will be launched. The collision between two consecutive magnetic blobs can result in a catastrophic magnetic reconnection, which releases a large amount of free magnetic energy and forms a forward shock. The shock propagates through the cold magnetized plasma within the blob in the collision region, radiating through the synchrotron maser mechanism,which is responsible for a non-repeating FRB signal. Our calculations show that the theoretical energetics, radiation frequency, duration timescale and event rate can be very consistent with the observational characteristics of FRBs.     

苡茨河泥石流地质灾害及防治

据统计,1992~2013年苡茨河曾多次发生泥石流地质灾害,并造成村民生命财产巨大损失。2013年7月24日再次爆发泥石流,破坏农田71280m2(108亩)。因此在对苡茨河泥石流形成条件、活动特征分析基础上,分析其泥石流的形成机制及其造成巨大危害的原因,预测其发展趋势,在已有治理措施的基础上,提出两种防治对策进行对比,得出一个较为合理的防治方案。     

江西萍乡杨家湾2号洞哺乳动物化石及其时代探讨

2015年11月和2016年10月先后对杨家湾2号洞化石点进行发掘。目前已出土哺乳动物化石1000多件,主要为单个牙齿化石,骨骼较少且较为破碎。初步鉴定出31个哺乳动物属种,其中偶蹄类数量最为丰富,野猪所占比例最大;灵长类和食肉类较为丰富;啮齿类、长鼻类及奇蹄类较少;尚未发现食虫类和翼手类。大部分属种为现生类群,少量灭绝属种如巴氏大熊猫、东方剑齿象及华南巨貘等。从动物群组成来看,该动物群与杨家湾1号洞、湖南道县福岩洞等动物群较为相似,属于我国南方典型的晚更新世大熊猫-剑齿象动物群,但是其所包含的动物属种相对后两个化石点都较少,尤其是小哺乳动物属种单调。杨家湾2号洞的堆积物颗粒比1号洞的较粗,且含较多角砾,缺少红色粘土;据初步判断,该洞的堆积物是由洞口进入。动物群组合指示该地区晚更新世气候较为温暖湿润。

     

广西田阳县那赖旧石器遗址发现的石制品和玻璃陨石

对广西田阳县那赖旧石器遗址进行实地调查,在百色盆地右江第Ⅳ级阶地的网纹红土中发现了一件玻璃陨石和大量的旧石器（包括12件手斧）。玻璃陨石的特征表明其为原地埋藏,未经后期流水作用搬运。玻璃陨石和石器之间的关系进一步证实,百色盆地第Ⅳ级阶地中保存的玻璃陨石可以代表手斧的埋藏年代。那赖遗址的石制品组合与百色盆地其他遗址的类似。通过与世界上其他阿舍利手斧在形态上和技艺上对比表明,该遗址手斧代表了早中更新世之交东亚的阿舍利技术特点。

     

柴达木盆地晚中新世河湖相沉积物粒度组成及其古环境意义

本文应用沉积物粒度端元分析模型对柴达木盆地怀头他拉剖面开放湖相沉积物进行分离,得到4个具有现实环境意义的端元组分,分别代表 4种动力过程。端元1为河流沉积,端元2、3都为湖相沉积,端元4为三角洲沉积。这些成分含量在晚中新世的变化趋势不明显但变化幅度相对较大,表明柴达木盆地这套地层记录了沉积环境或气候的快速变化。尽管怀头他拉粒度变化趋势总体不明显,然而平均粒径在约8.3~7.0Ma期间有所降低,指示当时亚洲季风可能发生了增强,导致柴达木古湖面积扩大,到达研究站点沉积物的粒度变细。东亚和南亚地区古气候数据合成支持这一推论,由此我们推断亚洲大陆在约8.3~7.0Ma期间气候相对较湿润,是青藏高原隆升的一个直接反应;而7Ma以后气候变干可能反映了大气CO₂含量下降的驱动。轨道尺度研究表明柴达木盆地气候在约8.3~7.0Ma期间发生了较大幅度的变化,支持青藏高原隆升是气候变化放大器的观点。