用于海洋探测的多参数拖曳荧光计系统   总被引：4，自引：1，他引：3  

夏达英王振先  朱儒弟袁毅之 《海洋工程》1999,(1):15

本文论述了作者研制成功的拖曳荧光计系统。该系统的荧光传感器采用了光源调制和信号同步解调技术,同时在受光器上采用了专用遮光导水暗盒及弯曲导水管,确保荧光传感器在探测体积内水体及时交换,并能有效地消除海中太阳光的影响。系统能在任一日光强度下从海表层至８０ｍ水深任一深度,走航拖曳速度在２～１０ｋｎ内平稳地水平工作。该拖曳体内安装有荧光传感器、温度传感器、深度传感器和多路传输电子线路装置。通过一根直径为１４ｍｍ的电源／信号传输七蕊铠装电缆将拖曳体与手摇绞车及船上控制器、数据采集、记录显示器连接在一起,可以同时测量光学和水文参数,这些数据为０～５Ｖ模拟电压量输出。该系统进行了多次水池和海上现场实验及应用,达到了预期设计目标。并且借助于荧光示踪染料完成了多处海区的水体混合扩散测量实验任务,建立了实验观测方法。本文还介绍了该系统的构造、现场测量实验数据和应用  相似文献   

The effect of a poloidal magnetic field on the linear and adiabatic oscillations of a polytropen=3     

M. Goossens 《Astrophysics and Space Science》1977,52(1):3-10

The frequencies of the linear and adiabatic oscillations of a gaseous polytrope with a poloidal magnetic field are determined with the aid of a perturbation method. The influence of the poloidal magnetic field on the different types of spheroidal oscillation modes is discussed. The poloidal magnetic field generally strengthens the stability of the oscillation modes and this effect is the largest in the case of the non-radialp-modes.  相似文献   

GONG p-Mode Parameters Through Two Solar Cycles     

René Kiefer  Rudi Komm  Frank Hill  Anne-Marie Broomhall  Markus Roth 《Solar physics》2018,293(11):151

We investigate the parameters of global solar p-mode oscillations, namely damping width \(\Gamma\), amplitude \(A\), mean squared velocity \(\langle v^{2}\rangle\), energy \(E\), and energy supply rate \(\mathrm{d}E/\mathrm{d}t\), derived from two solar cycles’ worth (1996?–?2018) of Global Oscillation Network Group (GONG) time series for harmonic degrees \(l=0\,\mbox{--}\,150\). We correct for the effect of fill factor, apparent solar radius, and spurious jumps in the mode amplitudes. We find that the amplitude of the activity-related changes of \(\Gamma\) and \(A\) depends on both frequency and harmonic degree of the modes, with the largest variations of \(\Gamma\) for modes with \(2400~\upmu\mbox{Hz}\le\nu\le3300~\upmu\mbox{Hz}\) and \(31\le l \le60\) with a minimum-to-maximum variation of \(26.6\pm0.3\%\) and of \(A\) for modes with \(2400~\upmu\mbox{Hz}\le\nu\le 3300~\upmu\mbox{Hz}\) and \(61\le l \le100\) with a minimum-to-maximum variation of \(27.4\pm0.4\%\). The level of correlation between the solar radio flux \(F_{10.7}\) and mode parameters also depends on mode frequency and harmonic degree. As a function of mode frequency, the mode amplitudes are found to follow an asymmetric Voigt profile with \(\nu_{\text{max}}=3073.59\pm0.18~\upmu\mbox{Hz}\). From the mode parameters, we calculate physical mode quantities and average them over specific mode frequency ranges. In this way, we find that the mean squared velocities \(\langle v^{2}\rangle\) and energies \(E\) of p modes are anticorrelated with the level of activity, varying by \(14.7\pm0.3\%\) and \(18.4\pm0.3\%\), respectively, and that the mode energy supply rates show no significant correlation with activity. With this study we expand previously published results on the temporal variation of solar p-mode parameters. Our results will be helpful to future studies of the excitation and damping of p modes, i.e., the interplay between convection, magnetic field, and resonant acoustic oscillations.  相似文献   

The German Bight (North Sea) is a nursery area for both locally and externally produced sprat juveniles     

Hannes Baumann  Arne M. Malzahn  Rudi Voss  Axel Temming 《Journal of Sea Research》2009,61(4):234-243

To better understand the role of the German Bight (GB) as a nursery area for juvenile North Sea sprat Sprattus sprattus we sought to determine whether the area may receive only locally or also externally produced offspring. We sampled juveniles during 3 trawl surveys in the GB in August, September, and October 2004 and applied otolith microstructure analysis in order to reconstruct their distributions of the day-of-first-increment-formation (dif). These were contrasted with spatial and seasonal patterns of sprat egg abundance in the GB and its adjacent areas, observed during 6 monthly plankton surveys. It was found that the majority of juveniles originated mainly from April/May 2004, coinciding with high spawning activity west of the GB, whereas spawning and larval production inside the GB peaked notably later, in May/June. This indicated that a large proportion of juveniles was produced outside the GB and transported subsequently into it through passive and/or active migration. Shifts to later mean difs from one survey to the next and length distributions indicative of the simultaneous presence of multiple cohorts, supported the notion that the GB is a complex retention and nursery area for sprat offspring from different North Sea spawning grounds and times. Later born juveniles had significantly faster initial growth rates than earlier born conspecifics, which was likely temperature-mediated, given the strong correlation between back-calculated growth histories and sea surface temperature as a proxy for thermal histories of juveniles (r² = 0.52).  相似文献