Variations of snow temperature and their influence on snow cover physical parameters in the Western Tianshan Mountains, China

This article discussed about snow temperature variations and their impact on snow cover parameters. Automatic temperature recorders were used to sample at 10-minute intervals at the Tianshan Station for Snow-cover and Avalanche Research, Chinese Academy of Sciences. 10-layer snow temperature and the snow cover parameters were measured by the snow property analyzer (Snow Fork) in its Stable period, Interim period and Snow melting period. Results indicate that the amplitude of the diurnal fluctuation in the temperature during Snow melting period is 1.62 times greater than that during Stable period. Time up to the peak temperature at the snow surface lags behind the peak solar radiation by more than 2.5 hours, and lags behind the peak atmospheric temperature by more than 0.2 hours during all three periods. The optimal fitted function of snow temperature profile becomes more complicated from Stable period to Snow melting period. 22 h temperature profiles in Stable period are the optimal fitted by cubic polynomial equation. In Interim period and Snow melting period, temperature profiles are optimal fitted by exponential equation between sunset and sunrise, and by Fourier function when solar radiation is strong. The vertical gradient in the snow temperature reaches its maximum value at the snow surface for three periods. The peak of this maximum value occurs during Stable period, and is 4.46 times greater than during Interim period. The absolute value of temperature gradient is lower than 0.1°C cm⁻¹ for 30 cm beneath snow surface. Snow temperature and temperature gradient in Stable period∼Interim period indirectly cause increase (decrease) of snow density mainly by increasing (decreasing) permittivity. While it dramatically increases its water content to change its permittivity and snow density in Snow melting period.     

The research of sea-land breeze (SLB) on the west coast of Bohai Bay based on field observation

Four automatic meteorological stations were set up in a line from beach to inland perpendicular to the west coast of Bohai Bay. Wind direction and velocity at altitudes of 2 m, 4 m and 12 m were surveyed with 10 minute intervals. On "Sea-Land Breeze" (SLB) days, the transition from sea breeze to land breeze was very evident in the study area. Direction of sea breeze was basically perpendicular to the coast and mainly from the ENE and E. Duration of sea breeze varied by the stations’ distance to the coastline, and the near-coast wind velocity was larger than that of the inland and decreases as it reaches inland. There was increased development of SLB on sunny days than on overcast days. The term "Climatic Coastal Zone" can be defined for the area influenced by SLB, which reaches more than 74 km inland on a typical SLB day but less than 10 km on a non-typical SLB day.     

极移的地震激发研究

本文采用Harvard目录中1977－1994年间的地震有关参数，及Dahlen计算的地震引起地球惯量矩的变化有关公式，得到由地震引起的极移要比观测值小2个量级．单个地震引起的极漂移呈现随机特性，但它的累积效应却表现出长期的变化，地震引起激发极的运动方向趋向于130—150°E，它与观测极漂移的方向相反．本文这一分析结果将随着观测技术的不断改进及观测精度的提高而得到证实．当考虑地球液核效应时，地震也可能对地球液核自由章动产生影响．我们的分析表明，大地震的这一影响与VLBI检测出的结果相比较，它在观测精度以下．     

浅谈河北省太行山区家庭养兔规模

本文对河北省太行山区家庭养兔规模进行了抽样调查,分析了家庭养兔规模的制约因素和规模大小之利弊。根据当地实际,提出了家庭养兔的适宜规模、经营方式和生产方向,对同类地区发展家庭养兔业具有一定的指导意义。     

太阳光谱望远镜的Stokes光谱测量

中国科学院云南天文台"太阳Stokes光谱观测与理论研究”团组自进入国家天文观测中心以来,经过一年多的努力,对50cm太阳光谱望远镜原偏振测量部分进行了彻底改造,由原来的D.C.调制改为A.C.调制,且增加了偏振测量校正系统.其机械,电控设计和加工于2000年2月完成,3月完成了光学调试,4月上旬完成了偏振解调和图像处理的软件编制.自2000年4月下旬以来,对23周峰年出现的部分活动区进行了较为成功的斯托克斯光谱测量,其偏振测量精度可达2×10-3,已接近国际水平,为该团组开展的课题研究打下了良好的基础.以此望远镜与怀柔观测基地太阳磁场望远镜相配合,将使我国太阳矢量磁场和速度场的研究更上一个台阶.给出了偏振测量的具体方法和部分测量结果.尽管取得了以上的成绩,但在近期内将对该偏振测量方式作进一步改进,用双光束分析代替单光束分析,使偏振测量精度提高到5×10-4,从而使之不仅能在活动区而且也能在宁静区得到矢量磁场的信息,不仅如此,还可对太阳第二光谱进行测量,提高我们依托该望远镜进行研究的广度和深度.     

A relation between solar activity and the Earth's rotation

In this paper, applying Vondrák band filter to both series of (l.o.d.) and sunspot relative number (R), we obtain variations of amplitude of 11 yr term during 1800–1985. The results show that solar cyclic signal in (l.o.d.) series is weak and unstable. The amplitude of 11 yr term in R series has long-periodic variation. The paper has briefly discussed some results about effects of solar activity on the Earth's rotation through the atmospheric motion. From the variation of (l.o.d.) obtained by band filter, we find that maxima of amplitude of annual term in (l.o.d.) occur at the same time with those of sunspot number. It implies that the angular momentum imbalance between the circulations in Southern Hemisphere and Northern Hemisphere is controlled in some way by solar activity.     

Nuclear Starburst Activity in the Seyfert 2 Galaxy NGC 2273

We present spectrophotometric results of the Seyfert 2 galaxy NGC 2273. The presence of high-order Balmer absorption lines (H8, H9, H10) and weak equivalent widths of Call K A3933, CN A4200, G-band A4300 and MgIb 5173 clearly indicate recent star-forming activity in the nuclear region. Using a simple stellar population synthesis model, we find that for the best fit, the contributions of a power-law featureless continuum, an intermediate-age (~ 108 yr) and an old (> 109yr) stellar population to the total light at the reference normalization wavelength are 10.0%, 33.4% and 56.6%, respectively. The existence of recent starburst activity is also consistent with its high far-infrared luminosity (log LFIR/L = 9.9), its infrared color indexes [a(25,60) = -1.81 and a(60,100) = -0.79, typical values for Seyfert galaxies with circumnuclear starburst], and its q-value (2.23, ratio of infrared to radio flux, very similar to that of normal spirals and starburst galaxies). Byrd et al. have suggested that NGC 2273 mig     

THE EVALUATION AND ANALYSIS OF THE TOURISM RESOURCES IN JILIN PROVINCE

This paper comprehensively evaluates and analyzes the tourism resources in Jilin Province,China.And it consists of three parts.The first two parts are on the resources evaluation and analysis.Based on the results of evaluation about the structural and spatial distribution of the tourism resources,it is found that ,the natural resources play fundamen-tal roles in Jilin,while the human and cultural resources are important complementary parts as well .In the spatial distribu-tion analysis,the resources show the characteristic of “six clusters“and “three belts “spatial relations.Four clusters are centered on the cities,which are Changchum,Jilin,Baicheng,Tonghua and Jiˊan;one cluster is around the Changbai Moutains and one cluster nears the frontier at Tumen between China,Russia and P.D.R.Korea.And the three belts are;1)The west belt.It contains Xianghai and Momoge natural protection region.The evident of this zone is its ecologi-cal and ethical tourism resources.2)The middle belt characterized by urban traveling and recreation,including Jilin and Changchum,together with their nearby Nongˊan and Siping.3)The last belt is also the most important one,which is the east zone.It covers the Changbai Mountains,the golden triangles of Tonghua and the Tumen River.This zone is remark-able for its abundant natural landscapes and unique folk-customs.In the last part the concept planning is briefly construct-ed for the tourism resources in Jilin Province according to the above evaluation and analysis.