Compressible turbulence in galaxy clusters: physics and stochastic particle re-acceleration     

G. Brunetti  A. Lazarian 《Monthly notices of the Royal Astronomical Society》2007,378(1):245-275

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Particle distributions and X-ray spectra in single or multiple solar current sheets     

C. Gontikakis  A. Anastasiadis  C. Efthymiopoulos 《Monthly notices of the Royal Astronomical Society》2007,378(3):1019-1030

The acceleration of charged particles in a site of magnetic reconnection is analysed by detailed numerical simulations. Single or multiple encounters of the particles with Harris-type reconnecting current sheets (RCSs) are modelled as an overall stochastic process taking place within an active region. RCS physical parameters are selected in a parameter space relevant to solar flares. Initially, the charged particles form a thermal (Maxwellian) distribution corresponding to coronal temperature  ≃2 × 10⁶ K  . Our main goal is to investigate how the acceleration process changes the shape of the particles' kinetic energy distribution. The evolution of the kinetic energy distribution, calculated numerically after one encounter of the particles with a single RCS, is found to be in good agreement with our previously published analytical formulae. In the case of consecutive encounters, we find that the kinetic distribution tends to converge to a practically invariant form after a relatively small number of encounters. We construct a discrete stochastic process that reproduces the numerical distributions and we provide a theoretical interpretation of the asymptotic convergence of the energy distribution. We finally compute the theoretical X-ray spectra that would be emitted by the simulated particles in a thick target model of radiation.  相似文献   

Diffusive synchrotron radiation from pulsar wind nebulae     

G. D. Fleishman  M. F. Bietenholz 《Monthly notices of the Royal Astronomical Society》2007,376(2):625-633

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沉积物捕获器在海岸与陆架沉积动力研究中的应用:以罗源湾和台湾海峡为例     

王爱军  叶翔  陈坚  黄财宾 《海洋学报》2015,37(1):125-136

运用时间序列的沉积物捕获器对海岸与陆架海域沉降颗粒物进行采集,估算沉降通量,并运用多学科综合研究手段分析沉降颗粒物的来源、组成、时空变化及控制因素,可以为海岸与陆架沉积动力过程的研究提供新的研究手段。福建罗源湾的实验表明,夏季罗源湾潮下带小潮至中潮期间的沉降通量为133.20~256.18g/(m2·t);由中潮向大潮变化期间单个潮周期的沉降通量明显增大,台风过后的大潮期间的沉降通量为373.99~590.51g/(m2·t);台风显著影响期间的沉降通量为746.34g/(m2·t);粒度分析及水动力观测结果显示,观测期间罗源湾潮下带沉降颗粒物主要来源于海底沉积物的再悬浮。台湾海峡西北部内陆架海域的实验研究表明,该海域近底部悬浮颗粒物沉降通量最大值为13.34g/(m2·d),由小潮向中潮沉降通量逐渐增大,这主要是由于近底部温盐跃层层位上移,近底部垂向混合作用增强,致使底部再悬浮沉积物向上扩散,并最终被沉积物捕获器捕获。沉积物捕获器可以接收到再悬浮沉积物,结合底部边界层过程的观测研究,可以深入认识海底沉积物的侵蚀、沉降及埋藏过程,在研究海岸与陆架区沉积动力学、泥质区沉积记录的形成过程与保存潜力中扮演着十分重要的角色。  相似文献   

Primordial black holes     

Maxim Yu.Khlopov 《中国天文和天体物理学报》2010,10(6)

Primordial black holes (PBHs) are a profound signature of primordial cos-mological structures and provide a theoretical tool to study nontrivial physics of the early Universe. The mechanisms of PBH formation are discussed and observational constraints on the PBH spectrum, or effects of PBH evaporation, are shown to re-strict a wide range of particle physics models, predicting an enhancement of the ul-traviolet part of the spectrum of density perturbations, early dust-like stages, first or-der phase transitions and stages of superheavy metastable particle dominance in the early Universe. The mechanism of closed wall contraction can lead, in the inflation-ary Universe, to a new approach to galaxy formation, involving primordial clouds of massive BHs created around the intermediate mass or supermassive BH and playing the role of galactic seeds.  相似文献   

河北春季一次飞机人工增雪的综合分析   总被引：1，自引：0，他引：1  

李宝东  孙玉稳  孙霞  刘伟  韩洋  蒋元华 《干旱气象》2014,(5):819-829

2013年4月19日,河北省人工影响天气办公室在河北中南部地区根据云系特点首次采用多层次水平催化和垂直验证的方式对层状云进行人工催化和探测。本文利用机载仪器所取得的飞机探测资料,结合实时天气、卫星、雷达、探空和雨量观测资料,分析了河北春季层状云增雪作业的技术指标,探讨了航测微物理参量和卫星、雷达、探空等资料在作业中的应用。结果表明：云在发展期雷达回波由15 dBZ逐步上升到25-35 dBZ,卫星反演的云顶高度、云顶温度、有效粒子半径、光学厚度等都有增加;云在中后期有效粒子半径、光学厚度、液水路径迅速下降,雷达回波同时减弱。在高度3 177-5 723 m之间过冷云滴达100-700个/cm^3,含水量在0.01 g·m^-3左右,最大0.081 g·m^-3,云粒子主要在此增长,形成降水粒子,该区间适宜催化。作业后,影响区内云体发展,雷达回波增强,出现35 dBZ强回波,且强回波中心扩大;卫星反演的云顶高度、光学厚度等比对比区有明显增加。  相似文献   

光衰减系数与悬浮颗粒物浓度的关系     

王鲁宁  魏皓  赵亮 《中国海洋大学学报(自然科学版)》2014,44(4):8-14

海水中光合作用有效光强(PAR)的变化受多种因素影响,其中分布在海水中的悬浮颗粒物是造成PAR在水中衰减的重要因素之一,尤其是在风与潮混合作用较强的近海。已有的研究表明:PAR在水中是呈指数衰减的,并且在悬浮物颗粒物分布比较稳定时,光衰减系数k与悬浮物体积浓度线性相关。在生态模型中,往往需要利用k获得水下光强,而衰减系数k很难直接通过观测得到,因此本文目的就是建立衰减系数与悬浮颗粒物体积浓度的关系,后者可通过观测得到。经过对2个航次与2个定点观测数据的处理,得到了PAR衰减系数分别与所有粒径悬浮物颗粒物总体积浓度以及3种粒级(黏土、粉砂、细砂)悬浮物体积浓度之间的线性关系式,并且发现相对于细砂,较小粒径的黏土、粉砂的浓度能更好的表征PAR的衰减特性。  相似文献   

Regular and chaotic dynamics in 3D reconnecting current sheets     

C. Gontikakis  C. Efthymiopoulos  A. Anastasiadis 《Monthly notices of the Royal Astronomical Society》2006,368(1):293-304

We consider the possibility of particles being injected at the interior of a reconnecting current sheet (RCS), and study their orbits by dynamical systems methods. As an example we consider orbits in a 3D Harris type RCS. We find that, despite the presence of a strong electric field, a 'mirror' trapping effect persists, to a certain extent, for orbits with appropriate initial conditions within the sheet. The mirror effect is stronger for electrons than for protons. In summary, three types of orbits are distinguished: (i) chaotic orbits leading to escape by stochastic acceleration, (ii) regular orbits leading to escape along the field lines of the reconnecting magnetic component, and (iii) mirror-type regular orbits that are trapped in the sheet, making mirror oscillations. Dynamically, the latter orbits lie on a set of invariant KAM tori that occupy a considerable amount of the phase space of the motion of the particles. We also observe the phenomenon of 'stickiness', namely chaotic orbits that remain trapped in the sheet for a considerable time. A trapping domain, related to the boundary of mirror motions in velocity space, is calculated analytically. Analytical formulae are derived for the kinetic energy gain in regular or chaotic escaping orbits. The analytical results are compared with numerical simulations.  相似文献   

11颗行星际尘粒中的锂,硼同位素丰度分析     

谢萍 《紫金山天文台台刊》1997,16(2):77-81

我们首次测量了4颗行星际尘粒(IDPs)中的~6Li/~7Li,~(10)B/~(11)B。它们的平均值分别是(8.40±0.37)×10~(-2)和(2.40±0.18)×10~(-2),随后又精确测量了7颗IDPs~6Li/Li的同位素丰度。  相似文献   

The Photon Mean Free Path Sphere, The Minimum Energy, and the Masses of the Main Elementary Particles     

A. Dinculescu 《Astrophysics and Space Science》2006,301(1-4):153-155

The photon mean free path sphere has several properties that strongly correlate with characteristics of the observable universe. This apparent connection led to a set of equations that were recently used to derive the values of the main cosmological parameters. It also leads, via an expression for the minimum energy, to an equation relating the mass of the proton to the mass of the electron.  相似文献