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901.
Susanta Kumar Samanta 《Journal of Earth System Science》2001,110(3):191-203
Petrographic studies of samples of the Rajmahal basalt reveal a variety of microscopic joints within phenocrysts, which seem
to have developed under the influence of thermal stresses during cooling. The theoretical analysis shows that:
In order to understand the effects of cooling rate on the mode of jointing, analogue model experiments were performed by quenching
melt films of organic, crystalline materials under varying cooling conditions. In experiments, non-branching linear joints
developed at relatively lower rates of cooling by a process of sub-critical crack propagation. On the other hand, at higher
rates of cooling the mechanism of crack propagation was essentially supercritical leading to the development of branching
joints. 相似文献
– | •thermal stresses develop in a system only under unsteady state of cooling, |
– | •the stresses responsible for the development of joints are tensile in nature, and |
– | •the magnitude of stresses increases with increasing rates of cooling. |
902.
Kumar Brajesh Jain Rajmal Tripathy S.C. Vats Hari Om Deshpande M.R. 《Solar physics》2000,191(2):293-307
A time series of GONG Dopplergrams for the period 10–14 May 1997 from Udaipur and Big Bear sites has been used to measure the velocity fluctuations in a sunspot (NOAA active region 8038) and quiet photosphere simultaneously. We observe that the power of pre-dominant p mode is reduced in the sunspot as compared to quiet photosphere by 39–52% depending on the location of the sunspot region on the solar disk. We also observe a relative peak frequency deviation of p modes in the sunspot, of the order of 80–310 Hz, which shows a linear dependence on the magnetic field gradient in the active region. The maximum frequency deviation of 310 Hz on 12 May appears to be an influence of a long-duration solar flare that occurred in this active region. We interpret this relative peak frequency deviation as either due to power re-distribution of p modes in the sunspot or a consequence of frequency modulation of these modes along the magnetic flux tubes due to rapidly varying magnetic field structure. 相似文献
903.
The air-sea exchange is one of the main mechanisms maintaining the abundances of trace gases in the atmosphere. Some of these,
such as carbon dioxide and dimethyl sulphide (DMS), will have a bearing on the atmospheric heat budget. While the former facilitates
the trapping of radiation (greenhouse effect) the latter works in the opposite direction through reflectance of radiation
back into space by sulphate aerosols that form from oxidation of DMS in atmosphere. Here we report on the first measurements
made on DMS in the Bay of Bengal and the factors regulating its abundance in seawater. Phytoplankton alone does not seem to
control the extent of DMS concentrations. We find that changes in salinity could effectively regulate the extent of DMSP production
by marine phytoplankton. In addition, we provide the first ever evidence to the occurrence of DMS precursor, DMSP, in marine
aerosols collected in the boundary layer. This suggests that the marine aerosol transport of DMSP will supplement DMS gaseous
evasion in maintaining the atmospheric non-sea salt sulphur budget. 相似文献
904.
A comparative study of Pleistocene phosphorites from the continental slope off western India 总被引:1,自引:0,他引:1
V. Purnachandra Rao S. W. A. Naqvi M. Dileep Kumar D. Cardinal A. Michard D. V. Borole E. Jacobs & R. Natarajan 《Sedimentology》2000,47(5):945-960
Two types of phosphorite recovered from the continental slope off western India are described. The first type, phosphorite 1, comprises a hard, grey nodule composed of carbonate fluorapatite (CFA) and calcite as major minerals. The phosphorite consists of light‐brown microcrystalline apatite containing a few skeletal fragments and planktonic foraminifera. Scanning electron microscope (SEM) studies show evidence of dissolution of skeletal calcite and filling of the resulting cavities by phosphate composed of ovoid to rod‐shaped apatite microparticles. Apatite also occurs as coatings on these particles. The P2O5 content of the phosphorite is 29%, and the CO2 content of the CFA is about 4·5%. The rare‐earth element (REE) abundance (ΣREE=2·02 μg g–1) is lower than in other modern phosphorites. The 87Sr/86Sr ratio and ?Nd value of this sample are 0·70921 and –9·9 respectively. The 14C age found through accelerator mass spectrometry (AMS) dating (18 720 ± 120 years BP) is much younger than that determined by the U‐series method (100 ka). The second type, phosphorite 2, comprises a friable, light‐brown nodule consisting of CFA as the only major mineral, with a CO2 content of the CFA of 4·5%. In thin section, the phosphate is light brown and homogeneous, and a few bone fragments are present. The P2O5 content is 33%, and REE contents (ΣREE = 0·18 μg g–1) are lower than in phosphorite 1. The age of phosphorite 2 is >300 ka. Phosphorite 1 appears to have formed during the late Pleistocene through replacement of carbonate by phosphate; phosphorite 2 is also of Pleistocene age but is much older than phosphorite 1. The initial substrate for phosphorite 2 was a fish coprolite, which was subsequently phosphatized during slow sedimentation under low‐energy conditions. Microbial mediation is evident in both phosphorites. The colour, density and P2O5 content of the phosphorites are found to be dependent on the nature of the initial substrates and physico‐chemical conditions during phosphatization. The CO2 content of the CFA is not related to the precursor carbonate phase. The nature of sediments, rates of sedimentation and the time spent undergoing phosphogenesis at the sediment–water interface may control REE concentrations in phosphorites. 相似文献
905.
906.
In this paper, we have investigated some tilted Bianchi Type I models with heat conduction filled with disordered radiation
of perfect fluid. To get a determinate solution, we have assumed a condition A =(BC)
n between metric potentials. Alternatively we have discussed the case A=(BC)
1/3 for which tilted nature of the model is preserved. The various and geometrical features with singularities in the models
are also discussed.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
907.
G. Handler T. Arentoft R. R. Shobbrook M. A. Wood L. A. Crause P. Crake F. Podmore A. Habanyama T. Oswalt P. V. Birch G. Lowe C. Sterken P. Meintjes J. Brink C. F. Claver R. Medupe J. A. Guzik T. E. Beach P. Martinez E. M. Leibowitz P. A. Ibbetson T. Smith B. N. Ashoka N. E. Raj D. W. Kurtz L. A. Balona D. O'donoghue J. E. S. Costa § M. Breger 《Monthly notices of the Royal Astronomical Society》2000,318(2):511-525
908.
Nine different types of cross‐stratified packages from the coal‐bearing, deltaic succession of the Barakar Formation (Permian) of the Satpura Gondwana Basin, central India, are described. The deposits are characterized by periodic mudstone drapes, reactivation surfaces including all other features suggestive of deposition from periodically unsteady, tidally‐influenced flows. The inferred flow patterns varied from purely bidirectional to pulsating unidirectional. The different types of cross‐stratified packages are interpreted to have resulted from superimposition of ebb‐oriented, steady, unidirectional fluvial currents of variable strength on the tidal flow in a deltaic setting. The study helps to distinguish cross‐strata that may develop in settings where fluvial and tidal currents interact. Copyright © 2004 John Wiley & Sons, Ltd. 相似文献
909.
910.