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Study of S-wave ray elastic impedance for identifying lithology and fluid
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作者 龚雪萍 张峰 +1 位作者 李向阳 陈双全 《Applied Geophysics》 SCIE CSCD 2013年第2期145-156,235,共13页
In this paper, we derive an approximation of the SS-wave reflection coefficient and the expression of S-wave ray elastic impedance (SREI) in terms of the ray parameter. The SREI can be expressed by the S-wave incide... In this paper, we derive an approximation of the SS-wave reflection coefficient and the expression of S-wave ray elastic impedance (SREI) in terms of the ray parameter. The SREI can be expressed by the S-wave incidence angle or P-wave reflection angle, referred to as SREIS and SREIP, respectively. Our study using elastic models derived from real log measurements shows that SREIP has better capability for lithology and fluid discrimination than SREIS and conventional S-wave elastic impedance (SEI). We evaluate the SREIP feasibility using 25 groups of samples from Castagna and Smith (1994). Each sample group is constructed by using shale, brine-sand, and gas-sand. Theoretical evaluation also indicates that SRE1P at large incident angles is more sensitive to fluid than conventional fluid indicators. Real seismic data application also shows that SRE1P at large angles calculated using P-wave and S-wave impedance can efficiently characterize tight gas-sand. 展开更多
关键词 S-WAVE IMPEDANCE ray parameter lithology identification fluid indicator
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Cosmological constraints on the DGP braneworld model with gamma-ray bursts
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作者 NanLiang Zong-HongZhu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2011年第5期497-506,共10页
We investigate observational constraints on the Dvali, Gabadadze and Porrati (DGP) model with Gamma-ray bursts (GRBs) at high redshift obtained directly from the Union2 Type Ia supernovae data set. With cosmology-... We investigate observational constraints on the Dvali, Gabadadze and Porrati (DGP) model with Gamma-ray bursts (GRBs) at high redshift obtained directly from the Union2 Type Ia supernovae data set. With cosmology-independent GRBs, the Union2 set, as well as the cosmic microwave background observation from the WMAP7 result, the baryon acoustic oscillation, the baryon mass fraction in clus- ters and the observed H(z) data, we obtain that the best-fit values of the DGP model are {ΩM0,Ωrc} = {0.235^+0.015-0.14, 0.138^+0.o51-0.048}, which favor a flat universe, and the transition redshift of the DGP model is ZT=0.67^+0.03-0.04.These results lead to more stringent constraints than the previous results for the DGP model. 展开更多
关键词 Gamma rays: bursts-cosmology: cosmological parameters
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Estimation of boundary parameters and prediction of transmission loss based upon ray acoustics 被引量:1
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作者 GUO Yuhong FAN Minyi HUI Junying (Harbin Engineering University Harbin 150001) 《Chinese Journal of Acoustics》 2000年第4期371-376,共6页
Estimation of boundary parameters and prediction of transmission loss using a coherent channel model based upon ray acoustics and sound propagation data collected in field experiments are presented. Comparison betwee... Estimation of boundary parameters and prediction of transmission loss using a coherent channel model based upon ray acoustics and sound propagation data collected in field experiments are presented. Comparison between the prediction results and the experiment data indicates that the adopted sound propagation model is valuable, both selection and estimation methods on boundary parameters are reasonable, and the prediction performance of transmission loss is favorable. 展开更多
关键词 Estimation of boundary parameters and prediction of transmission loss based upon ray acoustics
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The Dimension Paradox in Parameter Space of Cosine Family 被引量:1
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作者 Xiaojie HUANG Weiyuan QIU 《Chinese Annals of Mathematics,Series B》 SCIE CSCD 2020年第4期645-656,共12页
It is proved in this paper that the union of escaping parameter rays without endpoints for the cosine family Sκ(z)=eκ(ez+e-z),whereκ∈C is a parameter,has Hausdorff dimension 1,which implies that the ray endpoints ... It is proved in this paper that the union of escaping parameter rays without endpoints for the cosine family Sκ(z)=eκ(ez+e-z),whereκ∈C is a parameter,has Hausdorff dimension 1,which implies that the ray endpoints alone have Hausdorff dimension 2.This shows that Karpińska’s dimension paradox occurs also in the parameter plane of the cosine family. 展开更多
关键词 Dimension paradox Hausdorff dimension Parameter rays Dynamic rays
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