A possible method for the determination of the magnitude and inclination of a sunspot magnetic-field     

Jie-hai Jin 《Chinese Astronomy and Astrophysics》1985,9(1):15-19

A method is presented in this paper for the determination of both the H and the γ of a sunspot magnetic field by means of two polarizers with transmission axes inclined at ± 45° to the fast axis of a quarter-wave plate. Previously, this arrangement was used to determine H only.It is shown that the profiles of the Stokes parameters are sensitive to the sunspot atmosphere model used whereas the results given by the present method are not. It is shown, more ever, that the formula for determining H from the wave length shift, Δλ = 4.67 × 10^?5gHλ², cannot be used in many cases.  相似文献   

Cytoplasmic regionalization in starfish oocyte occurrence and localization of cytoplasmic determinants responsible for the formation of archenteron and primary mesenchyme in starfish (asterias amurensis) oocytes     

Zhang Shicui  Wu Xianhan  Zhou Jing  Wang Renxue  Wu Shangqin 《中国海洋湖沼学报》1990,8(3):263-272

Starfish oocytes with intact germinal vesicles (GVs) were cut along desired planes with glass needles or ligated using silk thread loops into two parts and allowed to mature in vitro, and inseminated. The experimental results showed that (1) only the parts with GVs or partial GV contents (PGVCs) cleaved, those without any GV materials did not; but nucleated and non-nucleated fragments cut from mature eggs were able to divide; (2) the development of animal parts of oocytes containing GVs or PGVCs was like that of animal fragments of matured oocytes with female pronuclei; most of them gave rise to permanent blastulae, and just a few formed ectodermal vesicles with a little primary mesenchyme; (3) a large part of vegetal fragments with GVs or PGVCs, and the vegetal parts of mature eggs without female pronuclei developed into small but normal embryos; (4) the fragments containing GVs or PGVCs obtained from the oocytes along a plane parallel to the animal-vegetal (A-V) axis developed as normally as the halves (with or without female pronuclei) severed from mature eggs along the same axis. Based on the data above, it was concluded that (1) the non-chromatin materials in the oocyte GVs are indispensable for successful fertilization and cleavage of starfish eggs; (2) some factor (s) located asymmetrically in the vegetal hemispheres of starfish oocytes is (are) responsible for formation of the archenteron and primary mesenchyme. It is evident from the above findings that the oocyte cytoplasm of the starfish had already regionalized before the GV break-down. Contribution No. 1722 from the Institute of Oceanology, Academia Sinica  相似文献   

The period changes of BW Vulpeculae     

《Chinese Astronomy and Astrophysics》1985,9(3):191-195

The period of the β Cephei variable, BW Vulpeculae, is increasing all the time at a rate of (14.24±0.20) × 10^?10d/d. Also, the residual in the time of light maximum shows a quasi-sinusoidal variation with a period of about 26.3 years and an amplitude of 0.022 – 0.024 days. If this is interpreted as the light-time effect in a binary orbit, then the orbit will have a size a sin i = 1.91 – 2.08 AU and an eccentricity e = 0.52.  相似文献   

Photoelectric photometry of the eclipsing binary WX Cancri     

《Chinese Astronomy and Astrophysics》1985,9(3):206-213

We obtained 672 observed points in yellow and 674 in blue in our photoelectric light curve of the Algol-type binary WX Cnc and we give 2 each of the times of primary and secondary minima. Using the Russell-Merrill method, we derived four mutually consistent sets of orbital elements, and determined the spectral type to be F6V for the combined system, and F5V and F8V for the primary and secondary components, separately. We found WX Cnc to be a detached system of two main sequence stars.  相似文献   

Turbulent diffusion in a shearing oscillatory flow     

Zhang Fagao  Takashi Ichiye 《中国海洋湖沼学报》1986,4(2):127-138

The diffusion in a shearing oscillatory flow from an instantaneous surface point source is considered. An analytical solution is obtained by Fourier transform. The results show that, for three dimensional diffusion in an oscillatory flow with constant shear, the distribution of the contaminant follows the multivariate Gaussian distribution rule. When the frequency is very high, or the time very short, the shear does not influence the diffusion. For moderate values of time, there are fluctuations with longitudinal variance. For large values of time the longitudinal variance increases as t, and the peak concentration decreases as t^−1.5, which are faster than those in a flow without shear, but much slower than those in a steady flow, where the longitudinal variance increases as t³ and the peak concentration decreases as t^−2.5. The contaminant patch is elongated in the longitudinal direction of the shear flow and moves back and forth with the water motion. Contribution No. 1306 from the Institute of Oceanology, Academia Sinica. Received July 12, 1985  相似文献   

ELECTROCHEMICAL CORROSION BEHAVIOR OF STEEL IN THE JUNCTURE AREA OF SEA CLAY AND SAND     

张经磊  侯保荣  郭公玉  杨芳英  谢肖勃 《中国海洋湖沼学报》1993,11(2):171-175

Corrosion behavior of steel in the juncture area of sea clay and sand was studied. The results show that galvanic corrosion occurred between steel samples buried in sea clay and sand, and that the polarity of the galvanic cell reversed after some testing later. The cause of reversing of polarity is discussed.  相似文献   

One zone modeling of irregular variability of stellar convective envelope     

W. Unno  D. -R. Xiong 《Astrophysics and Space Science》1993,210(1-2):77-81

One zone modeling of the irregular variability of red super-giants is intended with regard to the nonlinear coupling of finite amplitude pulsation with convection. The nonlocal mixing length is employed for the evaluation of the convective flux, the turbulent pressure and the turbulent power of temperature fluctuations. The radial pulsation and the Boussinesq convection are assumed for simplicity. The one zone is defined as the layer having the entropy maximum and the minimum at the bottom and at the top, respectively. The quasi-adiabatic approximation is consistent with this definition in fixing the zone to the same mass range. The spatial derivatives are evaluated under the assumption of homologous changes with the equilibrium homologous parameters. Then, a set of 6 simultaneous first order nonlinear ordinary differential equations are obtained as the one zone representation of the irregular variability of the convective envelope.  相似文献   

Morphological characters of the two-ribbon flare of 1981 May 13 and their explanation     

Zu-yan Zhu  Hong-ao Wu  Tian-jun Cao 《Chinese Astronomy and Astrophysics》1985,9(2):119-123

We give a summary of the morphology of the two-ribbon flare of 1981 May 13. One striking feature is that the Ha flare began at about 0338' UT and the double-ribbon structure was formed about 0346, $\text{before}$ the impulsive phase of the radio 3 cm burst at 04 11 UT. The 3 cm radio burst flux beginning at 03 33 UT showed only slow, stepwise increases lasting half an hour until the impulsive phase and this type of increase is usually regarded to be a typical thermal process. Each step in the radio flux corresponded to a variation in the Ha flare, showing that the radio and Hα emissions during this period came from the same thermal source. In this paper, we explain this behaviour in terms of Hyder's model: we think that the magnetic trough supporting the solar prominence rose for some reason, causing the prominence matter (the dark filaments) to fall along the magnetic lines and to hit the chromosphere and trigger off the flare. We give rough estimates of the energy density, the height of prominence and the infall matter at the different radio increments. We also give a qualitative explanation for the appearances of the single-peak structure in the radio burst at 0411 and the covering of the sunspot shortly after at 04 13 and propose several possible mechanisms.  相似文献   

The apparent copper complexing capacity of seawater and the interaction of copper with humic matter     

Mingyi  Sun 《中国海洋湖沼学报》1985,3(2):224-234

The anodic stripping voltammetry with physically-coating mercury film electrode was used to investigate the complexing action of trace heavy metals in seawater with organic ligands. The apparent copper complexing capacity of seawater was determined by titrating the organic ligands in natural seawater with standard ionic copper solution. The complexing actions of copper in seawater with humic acid (HA) or fulvic acid (FA) were investigated by titrating copper in seawater with HA or FA solution. The equilibrium time, electrodeposition potential, and effect of pH etc. were investigated respectively. The results show that the interaction of copper in seawater with organic matter is a fast process. At natural pH, HA or FA tend to act with copper in seawater to form nonlabile complexes. During experimental electrode process, these complexes did not significantly dissociate. The experimental results were calculated according to 1∶1 complex formation.  相似文献   

On the microwave millisecond spike emission and its associated phenomena during the impulsive phase of large solar flare     

Chun-sheng Li  Qi-jun Fu  Yu-hua Yan  Shu-ying Jiang  Hong-wei Li 《Chinese Astronomy and Astrophysics》1985,9(2):128-133

We propose a model of two acceleration regions, which can explain, on the basis of microwave maser caused by a “hollow-beam” distribution of electrons, the presence of millisecond spikes in the event of 1981 May 16 and their absence in the event of 1981 October 12, and the enhanced continuous emission in the latter. We have also uncovered relations among the features, e.g. the Type III_G, Type IV_DCIM and hard x-ray bursts, that accompany the microwave millisecond spikes during the impulsive phase of a large flare.  相似文献