土星磁层等离子体径向输运的数值模拟   总被引：2，自引：2，他引：0       下载免费PDF全文

王翼  陈出新 《地球物理学报》2008,51(3):635-642

本文建立了一个包含离心力效应的自洽稳态土星磁层模型,并且用等离子体细丝模型对土星磁层等离子体径向输运进行了数值模拟.模拟结果表明,Dione（土卫四）附近的等离子体可能因为发生离心交换不稳定性（Centrifugal Interchange Instability）而被输运到离土星更远的地方.这种输运现象的发生是由离心力主导的,等离子体的黏滞效应和能量转移对输运过程的影响非常小（几乎可以忽略不计）,但土星电离层电导率对输运过程有重要影响,电导率越低,径向输运过程越快,反之,高电导率在一定程度上会阻碍输运的进行.在土星电离层电导率σ=2 S时,Dione（距离土星6.3R_S, R_S为土星半径）附近的等离子体在5.52个小时中被输运到距离土星10R_S的地方.本文的模拟结果还表明,密度受到扰动的等离子体是不稳定的,如果洛仑兹力和等离子体热压强梯度不能与离心力平衡,径向输运就会发生.密度大的等离子体在向外输运过程中会绝热膨胀而温度降低,密度小的等离子体则在注入磁层过程中因为绝热压缩而温度升高.  相似文献   

Intergalactic radio absorption and the cobe data     

Eric J. Lerner 《Astrophysics and Space Science》1995,227(1-2):61-81

The COBE data on cosmic Background radiation (CBR) isotropy and spectrum are generally considered to be explicable only in the context of the Big Bang theory and to be confirmation of that theory. However, this data can also be explained by an alternative, non-Big Bang model which hypothesizes an intergalactic radio-absorbing and scattering medium. A simple, inhomogenous model of such an absorbing medium can reproduce both the isotropy and spectrum of the CBR within the limits observed by COBE, and in fact gives a better to fit to the spectrum observations than does a pure blackbody. Such a model does not contradict any other observations, such as the existence of distant radio sources.  相似文献   

A window on the plasma universe: the very large array     

Kevin R. Healy 《Astrophysics and Space Science》1995,227(1-2):83-91

For nearly two decades, the aperature synthesis telescope known as the Very Large Array (VLA) has been providing a wealth of data on all types of astronomical objects. This telescope fills the need for more powerful and more sensitive instruments to gather data on a vast range of plasma phenomena in astrophysical settings. Currently the VLA is capable of observing at eight radio frequency bands (four corresponding to important spectral lines) with sensitivities on the order of 10^–29 Wm ^–2 Hz ^–1, or 10^–3 Jansky (1 mJy), and noise levels ten times lower. This paper describes the VLA and its capabilities, and describes how researchers interested in plasma astrophysics can use the instrument.  相似文献   

Magnetic polarimetric refraction in the solar corona     

Y. N. Gnedin  E. D. Lopez 《Solar physics》1996,164(1-2):97-102

We present expressions which describe the angular displacement of radio sources due to refraction in a magnetized plasma. The main objective of the present paper is to take into account the combined effect of gradients of the electron density and the magnetic field. We use the geometrical optics approximation for the determination of the angular broadening of the radiation. The expressions obtained are applied to the case of the solar corona.  相似文献   

Shock waves propagation in the turbulent interplanetary plasma     

I. V. Chashei  V. I. Shishov 《Astrophysics and Space Science》1996,243(1):23-28

Effect of turbulence on interplanetary shock waves propagation is considered. It is shown that background turbulence results in the additional shock wave deceleration which may be comparable with the deceleration due to plasma sweeping. The turbulent deceleration is connected with the energy losses due to the strong turbulence amplification behind the moving shock front.  相似文献   

Using VLBI fringe-phase information from geodetic experiments for short-period ionospheric studies     

Thomas Hobiger  Tetsuro Kondo  Yasuhiro Koyama  Kazuhiro Takashima  Harald Schuh 《Journal of Geodesy》2007,81(6-8):389-401

The usage of Very Long Baseline Interferometry (VLBI) fringe-phase information in geodetic VLBI is a new field of research, which can be used for the detection of short-period (i.e., several minutes) variations (scintillations) of the ionosphere. This paper presents a method for the extraction of such disturbances and discusses how dispersive influences can be separated from intra-scan delay variations. A proper functional and stochastic model for the separation of the different effects is presented and the algorithms are applied to real measurements. In an example, it is shown that a traveling ionospheric disturbance in Antarctica can be detected very precisely. A possible physical origin and the propagation properties of the disturbance are presented and the results are compared with GPS measurements. The benefit of this method for other applications is also discussed.  相似文献   

电化学氢化物发生技术在原子光谱分析领域的应用进展     

祖文川  汪雨  武彦文  陈舜琮 《岩矿测试》2014,33(2):168-177

电化学氢化物发生法（EcHG）是原子光谱仪发展的一种实用气态进样技术。该技术通过采用电化学发生池内的电极反应代替传统化学还原的方法来生成氢化物和汞蒸气。与传统的化学法硼氢化钾（钠）-酸氢化物发生体系相比,EcHG技术仅需要支持电解质,氢化物（汞蒸气）在阴极室内发生后直接导入原子光谱仪的原子化器,在降低分析成本和溶液配制时间的同时,分析过程引入的空白值也大大降低,更加绿色环保。近年来,EcHG原子光谱分析已经从单一的元素总量测定发展到元素形态分析,从微量元素分析发展到痕量超痕量元素分析,发生元素涵盖了砷、硒、铅、镉、锡、锑、锗和汞,应用范围涉及食品、环境、烟草、饲料等实际样品。EcHG技术应用于原子荧光光谱分析,特征元素检出限能够达到0.1 μg/L级（汞为ng/L级）;应用于原子吸收光谱与等离子体发射光谱分析,适用元素检出限能够达到μg/L级,相对标准偏差均小于10%,回收率在90%~110%之间。EcHG技术相关的机理研究也已经起步,这为该技术在原子光谱分析领域的应用提供了理论基础。但是,EcHG技术的分析范围目前仅限于部分元素的无机态,对元素的有机形态分析是本领域发展的难点之一。本文提出,关于电化学氢化物发生的机理研究、电化学流通池结构的优化、形态分析范围的拓展等将成为该技术的重要发展方向。  相似文献   

软海绵属海绵Halichondria sp.甾体类化学成分研究   总被引：1，自引：0，他引：1       下载免费PDF全文

孙见凡  李云秋  杨斌  胡静  董光  刘永宏 《热带海洋学报》2013,(1):55-59

为了系统研究中国南海软海绵属海绵 Halichondria sp.的化学成分,文章采用多种色谱方法分离纯化,从其氯仿萃取部位中分离得到了9个甾体类化合物,依据理化性质、波谱数据和文献对照的方法鉴定其结构.其结构分别鉴定为:1)3β-羟基-5,8,22-麦角甾三烯-7-酮;2)3β,5α-二羟基-7,22-麦角甾二烯-6-酮;3)3β,5α,6β-胆甾三醇;4)3β,5α,9α-三羟基-7,22-胆甾二烯-6-酮;5)3β-羟基-5-胆甾烯-6-酮;6)5α,8α-环二氧-6,22-麦角甾二烯-3β-醇;7)5α,8α-环二氧-6-胆甾烯-3β-醇;8)7,22-麦角甾二烯-3β,5α,3β-三醇;9)胆甾醇.本研究结果不仅丰富了软海绵属海绵的化学成分研究,而且将为软海绵属海绵的化学分类及甾体类化合物的进一步研究提供有利的理论依据.  相似文献   

Gravitational weak lensing of hairy black hole in presence of plasma     

《New Astronomy》2024

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Weak gravitational lensing of black hole from T-duality in plasma     

《New Astronomy》2024

In this study, we investigate the impact of a plasma environment on gravitational weak lensing around a black hole from the perspective of T-duality. Our results demonstrate that the deflection angle of light rays around the black hole is notably affected by the parameter $l_0$, with an increase leading to a decrease in the deflection angle, while the effect of plasma on the deflection angle is the opposite. We also consider different types of plasma distributions, including uniform ${\omega }_e=const$, Singular Isothermal Sphere medium, and Non-Singular Isothermal gas sphere plasma. We have analyzed the total magnification of the image source due to gravitational weak lensing, taking into account the effect of parameter $l_0$ related to T-duality in the presence of plasma around the black hole.  相似文献