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1.
Corrado Massa 《Astrophysics and Space Science》2006,305(4):377-384
Quantum theory in Robertson – Walker spacetime suggests the existence of a minimal energy ε of the order of 10−45 erg. Reasonable forms for ε give the expansion factor R=R(t)(t= the cosmic time) with no need of gravitational field equations.Einstein's theory should be modified in gravitational fields of strength less than ε c/ħ ∼ 10−8 cm/s2 where c is the speed of light and ħ is the reduced Planck constant. The cosmological term λ is expected to decrease as the universe expands.In the Appendix, ε is derived from a big bang – big crunch Newtonian cosmology. 相似文献
2.
Longitudinal and transverse dispersion in estuaries may be determined in principle by measuring the change in time of the concentration field of a water soluble dye. In practice, measurements may take the form of several sampling runs crossing the dye patch. The coefficients of dispersion are usually estimated from the second moments of the concentration field; the use of second moments, in particular, introduces errors because measurements at long times or distance are unduly emphasized.A self-consistent method, free of the disadvantages inherent in the use of higher moments, is described in which the distribution of concentration in space is related to the zeroth spatial moment of concentration. In this formulation, based upon sampling runs across the dye patch, the concentration field in the estuary may be directly and simply related to the dispersion coefficients in both the intercept and gradient of a linear graph.The methods are illustrated by the characterization of a series of experiments in the Inner Estuary of Milford Haven. 相似文献
3.
A. Bhatnagar R. M. Jain J. T. Burkepile I. M. Chertok A. Magun H. Urbarz P. Zlobec 《Astrophysics and Space Science》1996,243(1):209-213
The powerful cosmic ray flare of Sept. 29, 1989 occurred behind the limb and was observed over a wide spectral range. The analysis of optical, radio, and other relevant data suggest two phases of energy release. After an impulsive phase a prolonged post eruption energy release occurred in an extended region of the corona following the eruption of a large coronal mass ejection (CME). This phase is responsible for numerous coronal and interplanetary phenomena including the ground-level increase of cosmic rays. 相似文献
4.
Wave propagation in anisotropic linear viscoelastic media: theory and simulated wavefields 总被引:6,自引:0,他引:6
J. M. Carcione 《Geophysical Journal International》1990,101(3):739-750
5.
Randall D. Campbell 《Experimental Astronomy》2002,14(1):57-60
Keck's Long Wavelength Spectrometer (LWS), is the facility instrument used for imaging and spectroscopy in the wavelength
range of 3–28 μm at the Keck Observatory. LWS uses an 128 × 128 Si:As blocked impurity band (BIB) array manufactured by the
Boeing Corporation. This paper discusses the method used for optimizing the detector's operating parameters at a temperature
of 8.5 K and bias voltage of 1.2 V. A process for characterizing detective quantum efficiency of BIB detectors is also presented.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
6.
In this study, we investigate two internal wave generation methods in numerical modeling of time-dependent equations for water wave propagation, i.e., delta source function method and source term addition method, the latter of which has been called the line source method in literatures. We derive delta source functions for the Boussinesq-type equations and extended mild-slope equations. By applying the fractional step splitting method, we show that the delta source function method is equivalent to the source term addition method employing the energy velocity. This suggests that the energy velocity should be used rather than the phase velocity for the transport of incident wave energy in the source term addition method. Finally, the performance of the delta source function method is verified by accurately generating nonlinear cnoidal waves as well as linear waves for horizontally one-dimensional cases. 相似文献
7.
In this paper, we analyse the ability of the nonlinear shallow-water (NSW) equations to predict wave distortion and energy dissipation of periodic broken waves in the inner surf zone. This analysis is based on the weak-solution theory for conservative equations. We derive a new one-way model, which applies to the transformation of non-reflective periodic broken waves on gently sloping beaches. This model can be useful to develop breaking-wave parameterizations (in particular broken-wave celerity expression) in both time-averaged wave models and time-dependent Boussinesq-type models. We also derive a new wave set-up equation which provides a simple and explicit relation between wave set-up and energy dissipation. Finally, we compare numerical simulations of both, the NSW model and the simplified one-way model, with spilling wave breaking experiments and we find a good agreement. 相似文献
8.
9.
于2001年10月—2002年3月在深圳职业技术学院海洋生物技术实验室进行摄食-生长实验(实验周期为56天)。实验在水温30℃的条件下进行,设饥饿、1%、2%和饱食4个摄食水平,研究了中华鳖(Trionyxsinensis)幼鳖(296.60—396.09g)的生长和能量收支。结果表明,中华鳖幼鳖的特定生长率随摄食水平的增加,其湿重、干物质、蛋白质和能量的特定生长率均呈二次曲线增加,其中干物质的特定生长率(SGRdr)与摄食率(Rl)的关系式为SGRdr=-0.3621+0.8809Rl-0.1352Rl2(r2=0.896,n=26,P<0.01);除湿重的转化效率外,干物质、蛋白质和能量的转化效率在2%组均达到最大,分别为27.47%、31.48%和25.01%;摄食水平对中华鳖氨氮排泄率和尿素氮排泄率以及氨氮占总氮排泄率的比例均有显著影响(P<0.01),总氮排泄率、氨态氮排泄率和尿素氮排泄率均随摄食水平的增加而升高,从饥饿组到饱食组的变动范围分别是4.71%—38.70%、3.50%—24.64%和1.21%—6.48%,而氨氮占总氮比例的变化规律与上述指的标略有不同,饥饿组的比例略高于1%组,摄食组的比例随摄食水平的增加而增加,该比例的变动范围是71.92%—83.20%,回归分析表明,幼鳖的总氮排泄率[μmol/(g·d)](GN)、氨氮排泄率[μmol/(g·d)](NH3N)及尿素氮排泄率[μmol/(g·d)](UN)与其蛋自质摄入率(%体重 相似文献
10.
摄食水平和性别对稀有鮈鲫生长和能量收支的影响 总被引:7,自引:0,他引:7
于1995年10月采集本所自繁有ju鲫(约1.03g/ind),在30℃水温下进行摄食-生长实验,研究了从饥饿到饱食5个摄食水平对不同性别稀有ju鲫的生长和能量收支的影响,结果表明,鱼体干物和能量含量不受摄食率和性别的影响,随着摄食率的增加,雌鱼的湿重,干重和能量特定生长率均呈双对数增加,雄鱼湿重特定生长率呈双对数增加,而干物质和能量特定生长率呈指增加,雄鱼生长速度及摄食率低于雌鱼,随着摄食率的增加,食物能损失于粪便中的比例均呈上升趋势,损失于排泄物中的比例变化不大,呈下降趋势,用于代谢的比例呈下降趋势,用于生长的比例呈上升趋势,除饥饿组外,在各个摄食水平,雌鱼食物能用于代谢的比例较雄鱼低,而用于生长的比例较雄鱼高。 相似文献