锆石SHRIMP年龄的测定流程

北京离子探针中心是科技部、国土资源部和中国科学院以共建共享方式建立的国家大型科学仪器中心,主要从事地质年代学和宇宙年代学的研究,其核心仪器是全世界第九台、中国引进的第一台高灵敏度高分辨率SHRIMPⅡ二次离子探针质谱仪。     

雏议山东境内陨石

1有关陨石的记载 陨石亦称陨星、流星。陨者,落也。陨石泛指宇宙天体在运行中撞击陨落进入地球引力范围,穿过大气层未被完全烧毁而降落到地面的残块或整块的太空物。陨石是不可多得的天体标本,带来许多宇宙空间的珍贵信息,为人类探索宇宙奥秘,研究天体演化和生命起源提供重要的科学情报。航天、军工、科研、博物馆等单位都逐步开展了对陨石的普查、收集、研究、陈列展示及科学普及工作,并取得了一定成果。     

喜马拉雅山佩枯岗日冰川地貌的年代学、平衡线高度和气候研究

喜马拉雅山珠穆朗玛峰-希夏邦马峰地区是青藏高原南部现代冰川集中发育区之一,古冰川遗迹亦十分丰富,是研究第四纪青藏高原冰川形成和演化的关键区,一直备受地貌和第四纪环境研究者的关注.应用原地宇宙核素10Be暴露年龄测试技术,对采自希夏邦马峰西北佩枯岗日拉曲谷地冰碛垄上的冰川漂砾进行年代学研究;结合冰川地貌分析方法,对古冰川...     

DWT Power Spectrum of the Two-Degree Field Galaxy Redshift Survey

The power spectrum of the two-degree Field Galaxy Redshift Survey (2dFGRS) sample is estimated with the discrete wavelet transform (DWT) method. The DWT power spectra within 0.035 < k < 2.2 h Mpc-1 are measured for three volume-limited samples de-fined in consecutive absolute magnitude bins -19 ～-18, -20～ -19 and -21～-20. We show that the DWT power spectrum can effectively distinguish ACDM models of σs = 0.84 and σ8 = 0.74. We adopt maximum likelihood method to perform three-parameter fitting of the bias parameter b, pairwise velocity dispersion σpv and redshift distortion parame-ter β = Ω0.6m/b to the measured DWT power spectrum. The fitting results state that in a σ8= 0.84 universe the best-fit values of σm given by the three samples are mutually consis-tent within the range 0.28 ～ 0.36, and the best fitted values of σpv are 398 35-27475 37-29 and 550 ± 20km s-1 for the three samples, respectively. In the model of σ8 = 0.74, our three samples give very different values of Ωm. We repeated the fitting using the empirical formula of redshift distortion. The result of the model of low σ8 is still poor, especially, one of the best-fit values of σpv is as large as 103 km s-1. We also repeated our fitting by incorporating a scale-dependent galaxy bias. This gave a slightly lower value of Ωm. Differences between the models of σ8 = 0.84 and σ8 = 0.74 still exist in the fitting results. The power spectrum of 2dFGRS seems to disfavor models with low amplitude of density fluctuations if the bias parameter is assumed to be scale independent. For the fitting value of Ωm to be consistent with that given by WMAP3, strong scale dependence of the bias parameters is needed.     

天体螺旋开放轨道及地球波动膨胀

狄拉克曾预言,引力常数G可能以每年ΔG<10~(-11)速率衰减。当代大百科全书和天体物理学资料为ΔG<2×10~(-11)/年和ΔG<10~(-10)/年。本文据激光精密测距计算得ΔG=1.01×10~(-10)/年。在微观世界,普朗克常数h