Investigating dynamic mechanisms of geological phenomena using methodology of computational geosciences: An example of equal-distant mineralization in a fault

This paper presents a research methodology associated with approximately a decade old computa- tional geosciences. To demonstrate how it can be used to investigate the dynamic mechanisms of geological phenomenon, we use as an example the equal-distant distribution of gold deposits in a three-dimensional permeable fault within the Yilgarn Craton, Western Australia. The related numerical results demonstrate that: (1) convective pore-fluid flow in fluid-saturated porous media is the control- ling dynamic mechanism leading to the equal-distant distribution of gold deposits along the fault; (2) the main characteristic of the new methodology is to change the traditionally used empirical, descrip- tive and qualitative methodology into the fundamentally scientific principles based predictive and quantitative methodology. Thus, this new methodology provides a modern scientific research tool for investigating the dynamic mechanisms associated with observed geological phenomena in nature.     

Inversion of focal mechanism and events identification using an improved relative amplitude method

The relative amplitude method(RAM) is more suitable for source inversion of low magnitude earthquakes because it avoids the modeling of short-period waveforms.We introduced an improved relative amplitude method(IRAM) which is more robust in practical cases.The IRAM uses a certain function to quantify the fitness between the observed and the predicted relative amplitudes among direct P wave,surface reflected pP and sP waves for a given focal mechanism.Using the IRAM,we got the fault-plane solutions of two ea...     

长重力波形成机制研究进展

简要介绍了长重力波的概念和它在近岸过程的重要性,概述和评析了长重力波形成的Munk与Tucker模式,BLW,Unoki和非线性作用模式,BFLW模式以及BLW和BFLW联合作用等6种模式,展望了长重力波综合研究的内容和必要性.     

论龙眼、荔枝生产的若干农业气象问题及对策

通过对龙眼、荔枝长期观察结果的分析,认为树体和花序受寒（冻）害、冬季连阴雨寡照致使成花率低,花期低温阴雨或高温干旱天气,使果树不能正常开花座果或果实败育等,是广西龙眼、荔枝生产上的主要农业气象问题。并就这些问题的发生机理及对策进行探讨。     

Tectonics of the Laptev Sea – Moma `Rift' Region: Investigation with Seismologic Broadband Data

Based on teleseismic broadband data, mainly recorded from stationsof the Incorporated Research Institute for Seismology (IRIS) and theGräfenberg (GRF) array in Germany, the focal mechanism and thefocal depth of the largest earthquakes in northeastern Siberia in thetime interval 1976–1996 were determined. For 9 events the relativeanelastic attenuation of the shear wave with respect to the compressionalwave along the travel paths could be calculated. Using the slip vectorsfrom the best constrained focal mechanisms and additional slip vectorsfrom Jemsek et al. (1986) and Parfenov et al. (1988), we obtained the North American–Eurasian pole of rotation west of the Cherskii mountainsat 67.1^° N, 132.3^° E.The investigation shows that the extension of the Arctic Mid-Ocean Ridgeinto the continental shelf acts as a continental graben structure.Actually, the crustal extension is concentrated on the eastern LaptevSea area and the seismicity of the western part of the Laptev Sea canbe explained by the assumption of a separate microplate. In the continentsoutheast of the Laptev Sea a series of northwest trending depressions,known as the Moma `Rift', are observed. Although in this region elevatedheat flow, recent volcanism and a low crustal thickness were found (i.e.Duchkov and Sokolova, 1985; Devyatkin, 1985), there is only a poorcorrelation between the seismicity and the rift valleys. So the Momastructures seem to be related to an aborted rift structure.     

Comparative ecophysiology of active zoobenthic filter feeding, essence of current knowledge

The present contribution gives an overview of current knowledge of a comprehensive and steadily growing research field. The first section deals with water pumping and particle retention mechanisms in ciliary and muscular filter feeders. The second section examines the biological filter pumps in order to assess adaptation to the environment. Filter-feeding benthic invertebrates have evolved filter pumps to solve common basic problems. This has led to a large degree of similarity between otherwise distant standing species, which makes comparative studies interesting and important. The present review of zoobenthic filter feeding aims at accentuating such recognition.     

Asymmetry of compton scattering by relativistic electrons with an isotropic velocity distribution: Astrophysical implications

The angular distribution of low-frequency radiation after a single scattering by relativistic electrons with an isotropic velocity distribution differs markedly from the Rayleigh angular function. In particular, the scattering by an ensemble of ultrarelativistic electrons is described by the law p=1?cosα, where α is the scattering angle. Thus, photons are mostly scattered backward. We discuss some consequences of this fact for astrophysical problems. We show that a hot atmosphere of scattering electrons is more reflective than a cold one: the fraction of incident photons reflected after a single scattering can be larger than that in the former case by up to 50%. This must affect the photon exchange between cold accretion disks and hot coronae (or advective flows) near relativistic compact objects, as well as the rate of cooling (through multiple inverse-Compton scattering of the photons supplied from outside) of optically thick clouds of relativistic electrons in compact radio sources. Scattering asymmetry also causes the spatial diffusion of photons to proceed more slowly in a hot plasma than in a cold one, which affects the shapes of Comptonization spectra and the time delay in the detection of soft and hard radiation from variable X-ray sources.     

The precession of eccentric discs in close binaries

If the emission of gamma-ray bursts were as a result of the synchrotron process in the standard internal shock scenario, then the typical observed spectrum should have a slope F _ν ∝ ν ^−1/2, which strongly conflicts with the much harder spectra observed. This directly follows from the cooling time being much shorter than the dynamical time. Particle re-acceleration, deviations from equipartition, quickly changing magnetic fields and adiabatic losses are found to be inadequate to account for this discrepancy. We also find that in the internal shock scenario the relativistic inverse Compton scattering is always as important as the synchrotron process, and faces the same problems. This indicates that the burst emission is not produced by relativistic electrons emitting synchrotron and inverse Compton radiation.     

Extended X-ray emission in the radio-loud galaxy 3C 382

ROSAT /HRI observations of the powerful radio-loud galaxy 3C 382 reveal extended X-ray emission associated with the source. On the basis of this new spatial component, a previous ROSAT /PSPC spectral analysis of the source is revised. Allowing for the presence of an additional thermal component in the PSPC spectrum, the non-thermal component is found to be compatible with the extrapolation of the well-defined 3C 382, 2–10 keV, power-law spectrum into the soft X-ray region. The thermal – extended – component would then account for the soft excess emission previously reported for this source. The origin of this thermal component is not clear. Its luminosity compares with that of rich Abell clusters; yet, the galaxy environment in 3C 382 appears of moderate optical richness. An alternative is that it is the result of a massive extended gaseous atmosphere sustained by the deep gravitational potential well of 3C 382.