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The rotation of the surface layer of the Sun is found to have been accelerated secularly from the sunspot data of 1943 to 1986. To represent the overall state of rotation of the differentially rotating Sun, we define an indexM, by integrating the angular momentum density over the whole surface of the Sun, and call it the angular momentum layer density. The indexM increased monotonically or secularly from 1943 to 1986. This period corresponds to solar cycles 18, 19, 20, and 21. The monotonic increase ofM indicates that a net angular momentum must have steadily been coming from the layer down below the surface. The differential rotation latitudinal dependence profile did not change much from cycle 18 to cycle 20, but at cycle 21 the degree of equatorial acceleration dropped. This aspect is discussed in the context of the 55-year grand cycle. Cycle 21 is the start of grand cycle VI. The latitudinal dependence is less steep at cycle 21. The time scale of secular change of the indexM reflects the time scale of change of linkage of the surface and the deep layer in form of the angular momentum transfer, and that the time scale of the profile change of the differential rotation reflects the time scale of the angular momentum transfer within the surface layer. 相似文献
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Muhammad Mukhlisin Nurul Aini Binti Abd Aziz 《Journal of the Geological Society of India》2016,87(4):483-490
Slope failure usually occurs when soil particles are unable to build a strong bond with each other and become loose because of the presence of water. Water pressure weakens the ties between the particles and they tend to slip. Therefore, this study focused on the use of horizontal drains to reduce water entry and control the ground water level as a method of slope stabilization. Several previous studies have shown that the use of horizontal drains to lower the water level in soil is one of the fastest and cheapest slope stabilization methods. The main objective of this study is to analyze the effect of horizontal drains on slope stability. Information on slope condition during the landslides which happened at Precinct 9, Putrajaya, Malaysia was used for analytical simulation. Seep/W and Slope/W analyses were carried out with GeoStudio version 2007 software. Slopes with and without horizontal drains were then compared in terms of groundwater level and factor of safety (FOS) values. Scenarios were created for seven types of soil namely: residual, clay, silt, loam, sandy loam, sandy clay loam, and silt clay loam for a case wise analysis. The effect of daily steady rainfall and realcondition rainfall was studied. These cases were studied to find the effectiveness of horizontal drains as a slope stabilization tool. The results revealed that when a drain was installed on a slope, the groundwater level dropped immediately and the safety factor of the slope increased. Sandy loam (sL) soil was identified as the best candidate for a horizontal drain. Its highly saturated hydraulic conductivity Ks facilitated groundwater drain through the horizontal drain effectively. Silt clay loam (scL) soil was identified as the least effective candidate. 相似文献
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钾盐作为战略资源,在农业、工业等领域具有重要的使用价值。世界大多数固态钾资源发现于大规模的石油勘探过程中,充分利用各种油气地质、地球物理资料开展钾盐勘探对于国家发展尤为重要。位于哈萨克斯坦的南图尔盖盆地地质构造简单、资源勘探潜力较大。文中以南图尔盖盆地Aryskum坳陷为研究区块,基于其沉积地质特点,结合多口井的常规测井资料及前人研究成果,综合分析自然伽马、自然电位、三孔隙度等测井曲线的响应特征,含钾层段具体表现为自然伽马异常高值,并通过无铀伽马曲线等排除铀、钍元素影响,扩径使得中子值偏高,自然电位异常幅度由砂岩层的负异常变化为正异常,电阻率值偏高,密度值介于2.25~2.45 g/cm3,声波时差在270~350 μs/m范围内。基于含钾层测井曲线特点,利用测井曲线综合识别法、重叠法、交会图法进行研究区钾盐识别。在研究区30余口井中发现有可溶性钾盐层分布,分布在M-Ⅱ-3、M-Ⅱ-2小层底部,其中M-Ⅱ-3层底部为主要钾盐层段,并对各井含钾层段累计厚度进行统计分析。最后,借助地层对比分析含钾层段在横向和纵向上的展布情况,通过等厚图的绘制开展了找钾有利区分析,拓展了测井资料在南图尔盖盆地钾盐勘查中的应用,进而为今后研究区钾盐找矿提供重点方向。 相似文献
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Understanding nesting ecology and behaviour of green marine turtles at Setiu,Terengganu, Malaysia 
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下载免费PDF全文 Aini Hasanah Abd Mutalib Nik Fadzly Amirrudin Ahmad Nurolhuda Nasir 《Marine Ecology》2015,36(4):1003-1012
In this paper, we emphasize the importance of understanding the nesting ecology and nesting behaviour of green marine turtles (Chelonia mydas). Data were collected from 2007 until 2012 from nesting beaches at Setiu Terengganu, Malaysia. We focused on one of the beaches, Telaga Papan, based on data collected in 2012. We recorded the distribution of nesting areas, the emergence hour and the correlation between successful nesting attempts and false crawls. Telaga Papan had a significantly higher distribution of green marine turtle nesting compared with the other five beaches (ANOVA, F5,42 = 8.874, P < 0.01, mean = 36.750 ± 3.727). The highest number of successful nesting attempts was recorded in 2012 (mean = 28.714). A majority of the species landed between 22:00 and 23:59 h (25%). There was a strong correlation between successful nesting attempts and false crawls (rs = 0.883, P = 0.02). Based on these findings on the nesting ecology and nesting behaviour of green marine turtles, we suggest that scientific research, strict monitoring, awareness programs and policy implementation should be carried out proactively. Such activities are necessary to reduce the anthropogenic pressures at the nesting beaches as well as to ensure more successful nesting attempts of green marine turtles in Setiu. 相似文献
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Sunspot drawings obtained at the National Astronomical Observatory of Japan during the years 1954–1986 were used to determine meridional motions of the Sun. A meridional flow of a few ms–1 was found, which is equatorward in the latitude range from -20° to +15° and is poleward at higher latitudes in both hemispheres. A northward flow of 0.01° day–1 or 1.4 ms–1 at mid-latitudes (between 10° and 20°) was also detected. From our limited data-set of three solar cycles, an indication of solar-cycle dependence of meridional motions was found. 相似文献
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准噶尔盆地吉木萨尔页岩油是中国典型的陆相页岩油。通过场发射扫描电镜、激光共聚焦、纳米CT、核磁共振等实验技术联合对微纳米孔隙中页岩油赋存特征进行研究,结果表明甜点储层具有纳米—亚微米—微米全尺度含油特征。在微纳米尺度,油、水赋存特征表现为重质组分油附着于2~5 μm以上孔隙的孔壁及充填于2~5 μm以下的孔隙中,中质组分油赋存于2~5 μm以上孔隙的中央,孔隙水含量较少,呈孤立状赋存于2~5 μm以上孔隙的中央,并被中质组分油包裹。页岩油在微纳米孔隙中的赋存不仅受生烃超压充注控制,还受吸附作用及多期次成藏影响。孔隙表面润湿性由亲水润湿反转为亲油润湿是烃类发生吸附的主要原因,多期次成藏造成微纳米孔隙中油质差异及高的含油饱和度。早期生烃超压充注进储层的重质组分油在孔隙表面亲油润湿下吸附于孔隙表面,随着吸附层变厚,纳米级孔隙逐渐被充满,孔隙水被驱替到较大的孔隙中间;后期成熟的中质组分油以此方式进一步充注和调整。研究认为埋深较大的凹陷西部是有利勘探方向。微纳米孔隙中的重质组分油是未来页岩油提高采收率的方向。吉木萨尔页岩油微观赋存特征及成因机制可能具有普遍性,对于中国陆相页岩油的深入研究具有借鉴意义。 相似文献
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We devised a new method, which we call the running-segment method, to achieve high-resolution time series of indices of solar rotation for determining the latitude dependence of the differential rotation by a least-squares fitting of the daily translation of positions of sunspot groups during a fixed time segment of 11 years. The segment is moved by an amount of one year to determine the differential profile of the next point of time. Time of the determined rotation data is defined by an arithmetic mean of the beginning and ending years of the segment. The rotation underwent an acceleration from 1948 to 1974 and a deceleration from 1974 to 1987. We found that the time profile of the indexM, the angular momentum surface layer density defined by integration of the angular momentum volume density over the whole surface, follows almost exactly the time profile of the 11-year running mean of the yearly mean of the sunspot relative number with a delay time of about 20 years. The acceleration (deceleration) phase corresponds to the ascending (descending) phase of amplitude of the 11-year solar cycle of cycle 16 (19) to cycle 19 (20) with a delay time of about 20 years. The cycles 15–20 correspond to the 55-year grand cycle V of the 11-year cycle. The delay time of about 20 years agrees well with the delay time predicted by a nonlinear dynamo theory of the solar cycle for driving the 55-year modulation of the 11-year solar cycle. The agreement suggests that the Lorentz force of the magnetic field of the solar cycle during grand cycle V drives the solar rotation modulation from 1948 to 1987 and that the force needed about 20 years to modify the rotation during 1943–1992. 相似文献
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Sunspot drawings obtained at National Astronomical Observatory of Japan during the years 1954–1986 were used to determine the differential rotation of the Sun. From the limited data set of three solar cycles it was found that three factors (the level of cycle activity, the cycle phase, and sunspot type) affect the solar rotation rate. The differential rotation varies from cycle to cycle in such a way that the rotation velocity in the low activity cycle (cycle 20) is higher than in the high-activity cycle (cycle 19). The equatorial rotation rate shows a systematic variation within each cycle. The rate is higher at the beginning of the cycle and decreases subsequently. Although quite small, the variation of solar differential rotation with respect to Zürich sunspot type was found. The H and J types show the slowest rotation among all the sunspot types. 相似文献
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A periodic long-term modulation of the solar surface rotation with a time scale on the order of 100 years is found in the sunspot data from 1874 to 1992 obtained by combinig the Greenwich Photoheliographic Results from cycle 11 to cycle 20 analysed by Balthasar, Vázquez, and Wöhl and the Mitaka sunspot sketch data from cycle 18 to 22 of the National Astronomical Observatory of Japan which was the Tokyo Astronomical Observatory of the University of Tokyo until 1988. A new index of the solar rotation M defined by integrating the angular momentum density over the whole surface, which we call the angular momentum surface layer density, reached a maximum at solar cycle 14, decreased to a minimum at cycle 17, and then increased to reach another maximum at cycle 21. The increase of M means acceleration of the surface layer as a whole by transport of angular momentum from the deeper layer. This implies an decrease (increase) of the radial gradient of the differential rotation if the basic radial gradient of the differential rotation increases (decreaes) inward. The decrease of M means deceleration of the surface layer and implies an increase (decrease) of the radial gradient. The degree of the equatorial acceleration of the surface differential rotation is also found to have undergone the same 100 year periodic modulation during the same interval, reaching a minimum at cycle 14, a maximum at cycle 17, and a minimum at cycle 21 in antiphase with the modulation of M. Thus both radial and latitudinal gradients of the differential rotation increased and decreased in phase (in anti-phase) if the basic radial gradient increases (decreases) inward. 相似文献
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