色球耀斑Hα谱线轮廓不对称性研究

Hα谱线轮廓的不对称性是色球耀斑光谱观测中的重要特征,也是耀斑动力学过程的重要观测事实之一．以紫金山天文台太阳光谱仪的观测资料为依据,给出Hα谱线不对称性的典型轮廓．在考虑氢原子非热激发、电离的作用下,经验性地计算了不同大气模型下谱线的不对称性特征,并在此基础上,对观测谱线进行半经验的研究．结果表明, 色球区的向下运动能够产生Hα谱线的红、蓝不对称性,并可以再生具体耀斑的谱线不对称性特征．此外,不仅非热粒子的能流、谱指数大小以及速度场所处的高度对谱线轮廓有影响,耀斑大气的背景模型对谱线的轮廓也有一定的影响．     

On the Geometry of Broad-Line Regions in BL Lac Objects

The geometry of broad-line regions (BLRs) in active galactic nuclei (AGNs) is still controversial. We use a sample of BL Lac objects, of which the black hole masses Mbh are estimated from their host galaxy absolute magnitude at R-band, MR, by using the empirical relation between MR and black hole mass Mbh. The sizes of the broad-line regions for Mgn are derived from the widths of Mgn lines and the black hole masses. Compared with the empirical relation between BLR size RBLR and MgII line luminosity LMgII, it is found the BLR sizes in the BL Lac objects derived in this paper are 2-3 orders of magnitude higher. If the BLR geometry of these sources is disklike, then the viewing angle between the axis and the line of sight is in the range of ~ 2°-15°, which is consistent with the unification scheme.     

谱线分析法测定ζAur型系统的 红巨星星风物质损失

用双星技术（Binary-technique）的谱线分析方法来测定双星系统中的红巨星或红超巨星的星风物质损失率是目前最为精确的。扼要介绍了此类方法的一般原理以及在ζAur/VVCep双星系统的物质损失测量中的应用。同时介绍了该方法的最新进展,并展开与此有关的一些简要讨论。     

An X-Ray Study of Lobe-Dominated Radio-Loud Quasars with XMM-Newton

We report on our results of X-ray spectral analysis for a sample of radio-loud quasars covering a wide range of the radio core-dominance parameter, R, from core-dominated to lobe-dominated objects, using data obtained mostly with the XMM-Newton Observatory. We find that the spectral shape of the underlying power-law continuum is flat even for the lobe-dominated objects (average photon index ～ 1.5), indistinguishable from that of core-dominated quasars. For lobe-dominated objects, contribution of X-rays from the jets is expected to be very small based on previous unification schemes, more than one order of magnitude lower than the observed X-ray luminosities. Assuming that radio-loud quasars follow the same X-ray-UV/optical luminosity relation for the disk-corona emission as found for radio-quiet quasars, we estimate the X-ray flux contributed by the disk-corona component from the optical/UV continuum. We find that neither the luminosity, nor the spectral shape, of the disk-corona X-ray emission can account for the bulk of the observed X-ray properties. Thus in lobe-dominated quasars, either the disk-corona X-ray emission is much enhanced in strength and flatter in spectral shape (photon index～1.5) compared to normal radio-quiet quasars, or their jet X-ray emission is much enhanced compared to their weak radio core-jet emission. If the latter is the case, our result may imply that the jet emission in X-rays is less Doppler beamed than that in the radio. As a demonstrating example, we test this hypothesis by using a specific model in which the X-ray jet has a larger opening angle than the radio jet.     

用MonteCarlo法模拟Lyα谱线轮廓

该文介绍了一种用Monte Carlo法模拟Lyα谱线轮廓的代码.该代码以Verbamme的思想与方法为基础,结合了其它的模拟方法,通过几种模型,模拟出了多种情况下的Lyα谱线轮廓.文中详细说明了该代码的模拟方法并讨论了模拟出的结果.     

在太阳磁场大气中FeIλ 5324.19(?)谱线的形成深度

本文在用Unno-Beckers方程计算光球和黑子本影磁场内FeIλ5324.19谱线形成过程中,计算了该谱线Stokes参数随5000连续谱光学深度分布的贡献函数及形成深度随波长的变化。计算结果表明:磁光效应的存在给该线横向磁场定标参数Q、U的形成深度的确定带来一定的复杂性,对I和V的形成深度的确定没有明显的影响。结合北京天文台太阳磁场望远镜半宽0.15的双折射滤光器,确定所观测磁场信息的形成深度。当对日面中心观测,在滤光器调至线心时,I形成在光球层及黑子高度100公里左右,在偏离线心0.15时V分量形成高度亦如此,Q、U分量的情况较复杂。     

1982年12月2日耀斑随时间变化的半经验模型

我们利用南京大学太阳塔中的多波段光谱仪,在H_α、H_β和CaⅡ H、K三个波段同时拍到了1982年12月2日日面S15W11处的一个SB级耀斑的光谱。本文给出其中七个时刻的谱线轮廓及有关参数的序列。在非局部热动平衡条件下计算了耀斑随时间变化的半经验模型,结果显示了色球耀斑的演化过程。利用模型得到了一些色球物质蒸发参数,结果同根据SMM的X射线观测所作的估计相一致。     

基于共轭地表曲面的山脊线和山谷线提取方法的研究

从数字化地形资料中自动提取山脊线和山谷线的技术,在测绘、工程设计等方面有着重要的意义。本文对地形流水模拟法提取山脊线和山谷线的方法进行深入研究后,提出利用共轭地表曲面的概念实现自动提取算法山谷线和山脊线的方法,并设计出了基于共轭地表曲面的地形流水模拟法自动提取算法山谷线和山脊线的算法。文后通过实验验证了该方法的有效性,它所提取的山脊线和山谷线与实际地形相符合。     

类星体QSO2000-330的重元素吸收线系统的证认

本文利用文[1]和文[2]所给出的高红移类星体吸收系统的证认方法,对目前最大红移类星体QS02000-330(z_e=3.78)的吸收光谱进行了吸收线红移系统的证认,并得到了六个重元素的吸收线系统:z_a=3.1881,3.1913,3.3335,3.5519以及z_a=1.3441,3.3459。前四个系统和Hunstead等人(1986)所得到的A、B、C、D系统(红移值分别是z_a=3.1881,3.1914,3.3332,3.5519)相符合;后两个是我们新发现的吸收系统。     

磷对过铝质岩浆液相线温度影响的实验研究

以宜春414岩体中的钠长花岗岩作为实验初始物,利用RQV-快速内冷淬火高温高压装置实验研究了100MPa压力、含5%H2O条件下,P对过铝质花岗岩液相线温度的影响.实验结果表明,碱性长石是最早结晶的矿物;随着体系中P2O5含量从0.27%增加到7.71%,液相线温度从最初的810℃降低到740℃,表明P有效地降低了过铝质岩浆体系的液相线温度.在过铝质岩浆体系中,P5+与Al3+的结合形成AlPO4,降低了熔体中碱性长石组分的活度,很可能是液相线温度降低的机制.