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排序方式: 共有195条查询结果,搜索用时 21 毫秒
81.
Sudip Dey Prasamita Sarkar Chandrani Debbarma Sushmita Paul 《Environmental Earth Sciences》2012,66(2):421-431
This paper aims to assess the geophysical signatures like morphology and structure of a fault line, which is situated in a
part of southern Baromura hill of Tripura, northeast India. In this work manual observations and technical applications were
adopted for understanding the morphological and structural characters of the fault line. As tectonic mapping is one of the
main objectives of this study, the remote sensing technique was used to prepare a tectonic map of the study area. Geothermal
range of the area was measured by unsupervised classification of Landsat TM thermal infrared band (band 6). The classified
thermal band was overlaid by another classified shortwave infrared band (band 7 of Landsat TM), which explains the structural
evidences of the study area. In addition, an automated digital elevation model (DEM) was prepared to assess the morphological
characters of the study area particularly near the confluence of R. Maharani and R. Gumti. To analyse the structural condition
of the faulted zone, resistivity characters of the rocks were measured by “vertical electrical sounding” (VES) method. The
electrical resistivity character of this area strongly supports that a displacement occurred in this place. Finally an attempt
was made to explain the character of faulting on the basis of morphological signatures and structural evidences for future
disaster management planning. 相似文献
82.
83.
Joyjit Dey Souvik Sen Surjyendu Bhattacharjee 《Journal of the Geological Society of India》2018,92(1):36-44
North Karanpura coal field is the western most marginal coal bearing segment of east-west trending Damodar valley basin. It consists of middle Permian Barakar Formation with sandstone, siltstone, coal and shale being the dominant lithofacies, deposited in a fluvial meandering environment, giving rise to repetitive fining upwards cycles. Study of geophysical logs, the drilled core holes were used to identify lithofacies, correlate coal seams with splitmerge behavior; which has been used to understand lateral and vertical facies disposition. Geophysical logs have been employed to compute various coal assay parameters–ash, fixed carbon, moisture, volatile content, cleat porosity, vitrinite reflectance seam wise. Study of log based coal assay parameters, calibrated with lab based values depicts lateral coal quality variation, i.e. decreasing ash content, higher fixed carbon from east to west, which can be a great proxy for future development of field or mine planning. 相似文献
84.
Michael A. Dopita Michiel Reuland Wil van Breugel Wim de Vries S. A. Stanford Huub Röttgering George Miley Bram Venemans Hy Spinrad Steve Dawson Arjun Dey Mark Lacy Daniel Stern Andrew Bunker 《Astrophysics and Space Science》2007,311(1-3):305-309
We present results from a Keck optical and near IR spectroscopic study of the giant emission line halos of the z>3 High Redshift Radio Galaxies (HiZRGs) 4C 41.17, 4C 60.07 and B2 0902+34. The outer regions of these halos show quiet kinematics
with typical velocity dispersions of a few hundred km s−1 and velocity shears consistent with rotation. The inner regions contain shocked, clumpy cocoons of gas closely associated
with the radio lobes with disturbed kinematics and expansion velocities and/or velocity dispersions >1000 km s−1. We also find evidence for the ejection of chemically enriched material in 4C 41.17 up to a distance of ∼60 kpc along the
radio-axis. We infer that these HiZRGs are undergoing a final jet-induced phase of star formation with the ejection of most
of their interstellar medium before evolving to become “red and dead” Elliptical galaxies. 相似文献
85.
Giuseppe Lanzafame D. Molteni & Sandip K. Chakrabarti 《Monthly notices of the Royal Astronomical Society》1998,299(3):799-804
Viscous Keplerian discs become sub-Keplerian close to a black hole since they pass through sonic points before entering into it. We study the time evolution of polytropic viscous accretion discs (both in one- and two-dimensional flows) using smoothed particle hydrodynamics. We discover that for a large region of the parameter space spanned by energy, angular momentum and polytropic index, when the flow viscosity parameter is less than a critical value, standing shock waves are formed. If the viscosity is very high then the shock wave disappears. In the intermediate viscosity, the disc oscillates very significantly in the viscous time-scale. Our simulations indicate that these centrifugally supported high density regions close to a black hole play an active role in the flow dynamics, and consequently, the radiation dynamics. 相似文献
86.
87.
Bhal Chandra Joshi Prakash Arumugasamy Manjari Bagchi Debades Bandyopadhyay Avishek Basu Neelam Dhanda Batra Suryarao Bethapudi Arpita Choudhary Kishalay De L. Dey A. Gopakumar Y. Gupta M. A. Krishnakumar Yogesh Maan P. K. Manoharan Arun Naidu Rana Nandi Dhruv Pathak Mayuresh Surnis Abhimanyu Susobhanan 《Journal of Astrophysics and Astronomy》2018,39(4):51
Radio pulsars show remarkable clock-like stability, which make them useful astronomy tools in experiments to test equation of state of neutron stars and detecting gravitational waves using pulsar timing techniques. A brief review of relevant astrophysical experiments is provided in this paper highlighting the current state-of-the-art of these experiments. A program to monitor frequently glitching pulsars with Indian radio telescopes using high cadence observations is presented, with illustrations of glitches detected in this program, including the largest ever glitch in PSR B0531+21. An Indian initiative to discover sub-(mu )Hz gravitational waves, called Indian Pulsar Timing Array (InPTA), is also described briefly, where time-of-arrival uncertainties and post-fit residuals of the order of (mu )s are already achievable, comparable to other international pulsar timing array experiments. While timing the glitches and their recoveries are likely to provide constraints on the structure of neutron stars, InPTA will provide upper limits on sub-(mu )Hz gravitational waves apart from auxiliary pulsar science. Future directions for these experiments are outlined. 相似文献
88.
Raka Dona Ray Mandal Monika Sinha † Manjari Bagchi Sushan Konar Mira Dey ‡ Jishnu Dey 《Monthly notices of the Royal Astronomical Society》2006,365(4):1383-1386
It appears that there is a genuine shortage of radio pulsars with surface magnetic fields significantly smaller than ∼108 G. We propose that the pulsars with very low magnetic fields are actually strange stars locked in a state of minimum free energy and therefore at a limiting value of the magnetic field which cannot be lowered by the system spontaneously. 相似文献
89.
The effect of the geomagnetic Lorentz force on the muon component of extensive air shower (EAS) has been studied in a Monte Carlo generated simulated data sample. This geomagnetic field affects the paths of muons in an EAS, causing a local contrast or polar asymmetry in the abundance of positive and negative muons about the shower axis. The asymmetry can be approximately expressed as a function of transverse separation between the positive and negative muons barycentric positions in the EAS through opposite quadrants across the shower core in the shower front plane. In the present study, it is found that the transverse muon barycenter separation and its maximum value obtained from the polar variation of the parameter are higher for iron primaries than protons for highly inclined showers. Hence, in principle, these parameters can be exploited to the measurement of primary cosmic-ray mass composition. Possibility of practical realization of the proposed method in a real experiment is briefly discussed. 相似文献
90.
Raktima Dey Sophie C. Lewis Julie M. Arblaster Nerilie J. Abram 《Wiley Interdisciplinary Reviews: Climate Change》2019,10(3)
There has been much attention given to the spatial and temporal characteristics of changes in mean and extreme rainfall over Australia during the past century. As Australia is the second driest continent on Earth, reliable projections around the trends and variability in future rainfall are crucial for policymakers and water resource management. This article comprehensively reviews the current published literature on trends in Australia's rainfall from pre‐instrumental and instrumental records, the climatic drivers of Australia's rainfall variability, attribution of the long‐term trends, extreme rainfall attribution methods with particular reference to a recent case study (2010–2012 east Australia rainfall event) and projected changes of mean and extreme rainfall over Australia during the 21st century. Notable trends in the observational record of rainfall in Australia are a decrease in mean rainfall in southwest and southeast Australia and an increase in northwest Australia since 1950. The general consensus of research into Australia's future rainfall is that mean rainfall will continue to decrease in southwest Australia in a warming world, while changes over northern and eastern Australia remain uncertain. There are still significant knowledge gaps around the causes of observed trends in rainfall both in the mean and extremes, the ability of climate models to accurately represent rainfall in the Australian region and future rainfall projections. These gaps are identified, and avenues for future research directions are proposed. This article is categorized under:
- Paleoclimates and Current Trends > Modern Climate Change