青海纳日贡玛斑岩铜(钼)矿地质地球化学特征及成因探讨

纳日贡玛斑岩铜矿,矿体主要赋存在喜山期花岗斑岩体中.笔者通过野外观察和室内研究,从矿床地质特征,岩石地球化学特征等方面对矿床的成因进行了探讨,初步认为它是一个典型的斑岩型铜(钼)矿床.     

Features of discrete VLF emissions observed at Gulmarg,India during the magnetic storm of 6–7 March, 1986

During the analysis of archived VLF data from Indian low latitude ground stations, some discrete VLF emissions recorded at the low latitude ground station Gulmarg (geomagnetic latitude 24°26′N; geomagnetic longitude 147°09′E, L = 1.28) during moderate magnetic storm activity (Σ K _P ⁻ = 32, K _P index varies from 4 to 6 during the observation period) on 6/7 March, 1986 are presented in this paper. The dynamic spectra of these discrete VLF emissions were observed along with tweeks and its harmonics, which is interesting and complex to explain. In most of the events the harmonic frequency of tweeks correlates with the starting frequency of harmonics of discrete emissions. In order to explain the observed features of discrete VLF emissions, we propose cyclotron resonance interaction between whistler mode wave and energetic electrons of inner radiation belt as possible generation mechanism. An attempt is also made to determine parallel energy, anisotropy and wave growth relevant to the generation process of VLF emissions.     

小城镇街道灰尘中氮磷含量研究

以上海市的枫泾镇(FJ)、松江新城(SJ)和朱家角镇(ZJJ)为例,研究了小城镇街道灰尘中氮磷的含量水平和分布特征,结果表明:小城镇街道灰尘中总无机氮的含量为11.9-1040.6μg/g,平均含量为117.5.μg/g;可溶磷的含量为15.8～65.8μg/g,平均含量为48.7μg/g;各小城镇街道灰尘中的氮磷含量表现为:FJ＞ZJJ＞SJ.各小城镇街道灰尘中氮磷含量的空同分布差异较大,位于城镇中心和风景区内采样点的氮磷含量明显较高,而城镇周边乡村地区含量较低.对各小城镇街道灰尘氮磷含量的季节变化分析表明,秋季小城镇街道灰尘中氮磷的含量明显高于冬季和夏季,温度、降雨量可能是其季节变化的主要影响因子.     

基于景观分区的植被类型信息提取

利用陆地卫星多光谱遥感数据,在研究草被、针叶林、阔叶林、耕地等不同植被类型波谱特征的基础上,引入景观分区信息,进行空间特征与波谱特征相结合的遥感植被类型信息提取,其精度和效果优于单纯依赖植被指数的分类方法,能够适用于研究区植被类型的详细划分。     

On the source of quasi-periodic oscillations of the black hole candidate GRS 1915+105: some new observations and their interpretation

A few classes of the light curve of the black hole candidate GRS 1915+105 have been analysed in detail. We discover that unlike the previous findings, quasi-periodic oscillations (QPOs) occasionally occur even in the so-called 'On' or softer states. Such findings may require a revision of the accretion/wind scenario of the black hole candidates. We conjecture that considerable winds that are produced in 'Off' states cool down as a result of Comptonization and fall back to the disc, creating an excess accretion rate and producing the so-called 'On' state. After the drainage of the excess matter, the disc goes back to the 'Off' state. Our findings strengthen the shock oscillation model for QPOs.     

Two-dimensional electric field measurements in the ionospheric footprint of a flux transfer event

Line-of-sight Doppler velocities from the SuperDARN CUTLASS HF radar pair have been combined to produce the first two-dimensional vector measurements of the convection pattern throughout the ionospheric footprint of a flux transfer event (a pulsed ionospheric flow, or PIF). Very stable and moderate interplanetary magnetic field conditions, along with a preceding prolonged period of northward interplanetary magnetic field, allow a detailed study of the spatial and the temporal evolution of the ionospheric response to magnetic reconnection. The flux tube footprint is tracked for half an hour across six hours of local time in the auroral zone, from magnetic local noon to dusk. The motion of the footprint of the newly reconnected flux tube is compared with the ionospheric convection velocity. Two primary intervals in the PIFs evolution have been determined. For the first half of its lifetime in the radar field of view the phase speed of the PIF is highly variable and the mean speed is nearly twice the ionospheric convection speed. For the final half of its lifetime the phase velocity becomes much less variable and slows down to the ionospheric convection velocity. The evolution of the flux tube in the magnetosphere has been studied using magnetic field, magnetopause and magnetosheath models. The data are consistent with an interval of azimuthally propagating magnetopause reconnection, in a manner consonant with a peeling of magnetic flux from the magnetopause, followed by an interval of anti-sunward convection of reconnected flux tubes.