Effects of petrophysical parameters on attenuation and dispersion of seismic waves in the simplified poroelastic theory: Comparison between the Biot's theory and viscosity‐extended theory     

Haixia Zhao  Bangyu Wu  Jinghuai Gao 《Geophysical Prospecting》2021,69(1):204-219

The simplified macro‐equations of porous elastic media are presented based on Hickey's theory upon ignoring effects of thermomechanical coupling and fluctuations of porosity and density induced by passing waves. The macro‐equations with definite physical parameters predict two types of compressional waves (P wave) and two types of shear waves (S wave). The first types of P and S waves, similar to the fast P wave and S wave in Biot's theory, propagate with fast velocity and have relatively weak dispersion and attenuation, while the second types of waves behave as diffusive modes due to their distinct dispersion and strong attenuation. The second S wave resulting from the bulk and shear viscous loss within pore fluid is slower than the second P wave but with strong attenuation at lower frequencies. Based on the simplified porous elastic equations, the effects of petrophysical parameters (permeability, porosity, coupling density and fluid viscosity) on the velocity dispersion and attenuation of P and S waves are studied in brine‐saturated sandstone compared with the results of Biot's theory. The results show that the dispersion and attenuation of P waves in simplified theory are stronger than those of Biot's theory and appear at slightly lower frequencies because of the existence of bulk and shear viscous loss within pore fluid. The properties of the first S wave are almost consistent with the S wave in Biot's theory, while the second S wave not included in Biot's theory even dies off around its source due to its extremely strong attenuation. The permeability and porosity have an obvious impact on the velocity dispersion and attenuation of both P and S waves. Higher permeabilities make the peaks of attenuation shift towards lower frequencies. Higher porosities correspond to higher dispersion and attenuation. Moreover, the inertial coupling between fluid and solid induces weak velocity dispersion and attenuation of both P and S waves at higher frequencies, whereas the fluid viscosity dominates the dispersion and attenuation in a macroscopic porous medium. Besides, the heavy oil sand is used to investigate the influence of high viscous fluid on the dispersion and attenuation of both P and S waves. The dispersion and attenuation in heavy oil sand are stronger than those in brine‐saturated sandstone due to the considerable shear viscosity of heavy oil. Seismic properties are strongly influenced by the fluid viscosity; thus, viscosity should be included in fluid properties to explain solid–fluid combination behaviour properly.  相似文献   

Optical properties of dust from Jupiter family comets     

E. Hadamcik 《Planetary and Space Science》2009,57(10):1118-1132

To try to define specific physical properties of the dust of Jupiter-family comets (JFCs), we compare the light scattered by them. Amongst the more than 1000 JFCs, less than 200 are numbered, 40 of them being rather bright. In the present work we use data from the latter. In situ observations of three nuclei show low albedo surfaces. The albedo of the dust particles in the coma is low, with generally a red colour. The A(α)fρ product is a measure of cometary activity and secular changes. Images of different regions (jets and fans) give indications on the nucleus rotation and position of the emitting areas, as compared to the position of the rotation axis. Differences in physical properties between the particles in different regions are pointed out by differences in the linear polarization of the scattered light and by spectral variations in brightness and polarization. Jupiter family comets are considered as dust-poor comets. Tails and trails’ studies give an estimation of the size distribution of the particles. However the dust production rates depend on the largest particles (up to centimetre size), which are mainly observed in the trails where large dark compact particles are found. These dark particles are also responsible for the high polarization in the inner most coma of some comets. The meaning, in terms of physical properties, of the linear polarization is discussed through different examples such as 2P/Encke, 9P/Tempel 1 or the fragments of 73P/Schwassmann-Wachmann 3. Cometary outbursts and splitting events show that the properties of the dust ejected from the interior of the nucleus are similar to the ones of more active comets (new or with larger semi-major axis).  相似文献   

Exceptional Fireball Activity of Orionids in 2006     

Pavel Spurný  Lukáš Shrbený 《Earth, Moon, and Planets》2008,102(1-4):141-150

We report exceptional fireball activity of the Orionid meteor shower in 2006. During four nights in October 2006 the autonomous fireball observatories of the Czech part of the European Fireball Network (EN) recorded 48 fireballs belonging to the Orionids. This is significantly more than the total number of Orionids recorded during about five decades long continuous operation of the EN. Based on precise multi-station photographic and radiometric data we present accurate atmospheric trajectories, heliocentric orbits, light curves and basic physical properties of 10 Orionid fireballs with atmospheric trajectories that were long enough and, with one exception, were observed from at least three stations. Seven were recorded in within a 2-h interval in the night of 20/21 October. Their basic parameters such as radiant positions and heliocentric orbits are very similar. This high fireball activity originated from a very compact geocentric radiant defined by α = 95.10° ± 0.10° and δ = 15.50° ± 0.06°. These fireballs most likely belonged to a distinct filament of larger meteoroids trapped in 1:5 resonance with Jupiter. From detailed light curves and basic fireball classification we found that these meteoroids appertain to the weakest component of interplanetary matter.  相似文献   

First arrival cycle-based calculation methods of in situ sound speed and attenuation in sediments     

Dapeng Zou  Wei Luo  Hongbo Zheng 《Marine Georesources & Geotechnology》2017,35(1):98-103

The acoustic properties of seafloor sediments are of great importance in geoacoustic modeling, detecting, and oceanic engineering. The methods based on the first arrival cycle are investigated to calculate sound speed and attenuation of sediment more precisely in in situ measurements. The comparison of different data analysis methods based on the first arrival cycle approach for in situ measurement results in the following conclusions: (1) the calculated methods can help find the effective cycles and reduce the errors in calculating sound speed and attenuation; (2) using this approach, the point judgment method-based data analysis has the same effectiveness as the cross-correlation method-based data analysis in calculating group sound speed and has the same effectiveness in calculating attenuation in the time domain as the spectrum analysis method-based data analysis has in calculating attenuation in frequency domain; and (3) measurement in water can help not only calibrate the transmitting distance but also can calculate the time delay for the sound speed and the attenuation loss in the transmitting process. Finally, theoretical calculation was used to calculate the measured results, indicating a good agreement, which supports that first arrival cycle-based calculated methods can be used to analyze the measured data and the effective density fluid model can be used to analyze more acoustic properties and invert several physical properties in this experiment.  相似文献   

GEO空间碎片光度测量标定方法的研究   总被引：1，自引：0，他引：1  

庄诚  隋成华  唐轶峻 《天文研究与技术》2011,(4):343-346

基于GEO卫星、太阳和观测站的空间几何关系,建立了消除太阳赤纬角对地球同步轨道( Geostationary Orbit,GEO)卫星光学特性的影响的方法.以三轴稳定GEO盒状卫星缩比模型为研究样本,在不同太阳赤纬角下进行仿真实验光度测量,研究太阳赤纬角和相位角的空间几何关系,得出消除太阳赤纬角对其辐亮度值以及以相位角...  相似文献   

环境因子对三种常见微藻细胞中二甲基硫丙酸含量影响的初步研究   总被引：2，自引：0，他引：2  

李炜  焦念志 《海洋与湖沼》1999,30(6):635-639

以3种常见的海洋浮游藻类──扁藻、杜氏藻和牟氏角刺藻作为实验材料,采用正交方法设计实验条件,研究盐度、温度和光强的变化对藻类细胞内二甲基硫丙酸（DMSP）含量的影响。结果表明,3种藻类细胞DMP含量相差很大。扁藻DMSP含量最高,其次为杜氏藻,牟氏角刺藻含量最低。种间差别的影响明显高于环境条件的变化对藻细胞DMSP含量的影响。3种环境因子对藻细胞DMSP含量的影响效果不同,盐度变化引起藻细胞DMP含量的变化最为显著,其次为温度和光强。随着盐度的增加,扁藻、杜氏藻和牟氏角刺藻细胞内DMSP含量均呈上升趋势。  相似文献   

中肋骨条藻和新月菱形藻对营养盐的吸收速率及环境因素影响的研究   总被引：19，自引：4，他引：15  

李铁  史致丽  仇赤斌  王巧玲 《海洋与湖沼》1999,30(6):640-645

于１９９５年３月－－１９９６年１月,通过实验室模拟培养,研究了中肋骨条菏和新月菱形藻对磷酸盐和硝酸盐的吸收速率,以及温度、光照等环境因素对新月菱形藻吸收磷酸盐的影响。结果表明,用Ｍｉｃｈａｅｌｉｓ－Ｍｅｎｔｏｎ方程处理,求得中肋骨条藻和新月菱形藻吸收磷酸盐的半饱和常数分别为０．６１μｍｏｌ／Ｌ和０．４８μｍｏｌ／Ｌ,吸收硝酸半饱和常数分别为７．８μｍｏｌ／Ｌ和６．０μｍｏｌ／Ｌ,新月菱形藻对磷酸盐  相似文献   

Notes on laboratory rearing of juvenile spiny lobsters,jasus edwardsii (hutton) (crustacea: Decapoda: Palinuridae)     

Craig B. Kensler 《新西兰海洋与淡水研究杂志》2013,47(1):71-75

Post‐puerulus specimens of Jasus edwardsii (Hutton) have been successfully reared in the laboratory from the puerulus stage for periods of up to 12 months. The spiny lobsters were reared in concrete‐asbestos tanks measuring 2.4m × 37cm × 23cm. The tanks were supplied with a continuous flow of sea water and provided with constant aeration. Empty shells of paua (Haliotis iris Martyn) and rocks from the intertidal zone provided cover within the tanks.

Fresh mussel (Mytilus sp.) was preferred to all other foods tried in feeding experiments. The animals were fed every second day on opened mussels, and occasionally on fresh fish. The juveniles “grazed” actively on the calcareous algae (Corallina officinalis L.) present on the rocks.

The animals were extremely sensitive to pollution. To reduce pollution risks all sediments were removed from each tank, as the interstices between them were found to harbour uneaten food particles. Any uneaten foods were siphoned out every second day and each tank was thoroughly cleaned every six to eight weeks.

From a total of over 3,300 animals collected since November 1965, over 800 are presently being reared in the laboratory and various aspects of their ecology studied. The first step in raising larger adult sizes from juvenile stages in the laboratory is clearly possible.  相似文献   

Light hydrocarbons geochemistry of surface sediment from petroliferous region of the Mehsana block,North Cambay Basin     

T. Madhavi  T. Satish Kumar  M. A. Rasheed  G. Kalpana  D. J. Patil  A. M. Dayal 《Journal of the Geological Society of India》2009,74(1):7-15

A study was carried out to test the usefulness of surface geochemical methods as regional evaluation tools in petroliferous region of the Mehsana block, North Cambay Basin. A suite of 135 soil samples collected from the depth of 2.5 m, were analyzed for adsorbed light gaseous hydrocarbons and carbon isotopes (δ¹³C_methane and δ¹³C_ethane). The light gaseous hydrocarbon analysis show that the concentration ranges 402 ppb, 135 ppb, 70 ppb, 9 ppb and 18 ppb of C₁, C₂, C₃, iC₄ and nC₄, respectively. The value of carbon isotopic ranges of methane −29.5 to −43.0‰ (PDB) and ethane −19.1 to −20.9‰ (PDB). This data, when mapped, indicates patterns coinciding with major known oil and/or gas field of Sobhasan/Linch in this study area. The existence of un-altered petroliferous microseeps of catagenetic origin is observed in the study area. A regional study, such as the one described here, can provide important exploration facts concerning the regional hydrocarbon potential in a block. This method has been confirmed and can be applied successfully in frontier basins.  相似文献   

含孔隙、裂隙地层随钻多极子声波测井理论   总被引：4，自引：4，他引：0       下载免费PDF全文

许松  苏远大  陈雪莲  唐晓明 《地球物理学报》2014,57(6):1999-2012

储层岩石中普遍存在孔隙与裂隙,对钻井中的测井声波产生重要影响.基于孔、裂隙介质弹性波理论,导出了随钻声波测井的井孔声场表达式.据此考察了地层裂隙密度与含气饱和度的变化时井孔内随钻多极子模式波（斯通利波、弯曲波和螺旋波）的速度、衰减与灵敏度以及地层纵、横波的响应特征.裂隙密度与含气饱和度对模式波的速度频散与衰减都有影响,且两参数的值越大,影响越大.具体来说,速度对裂隙密度更敏感,而衰减对含气饱和度更敏感.具有"艾里相"特征的随钻偶极和四极子波在地层含气时产生强烈衰减,可以作为判断地层含气的一个明显指示.理论模拟与实际测井数据分析结果符合较好.  相似文献