Soil characterization based on land cover heterogeneity over a tropical landscape: an integrated approach using earth observation data-sets     

Diwakar Paudel  Jay Krishna Thakur  Sudhir Kumar Singh  Prashant K. Srivastava 《国际地球制图》2015,30(2):218-241

Soil is a vital part of the natural environment and is always responding to changes in environmental factors, along with the influences of anthropogenic factors and land use changes. The long-term change in soil properties will result in change in soil health and fertility, and hence the soil productivity. Hence, the main aim of this paper focuses on the analysis of land use/land cover (LULC) change pattern in spatial and temporal perspective and to present its impact on soil properties in the Merawu catchment over the period of 18?years. Post classification change detection was performed to quantify the decadal changes in historical LULC over the periods of 1991, 2001 and 2009. The pixel to pixel comparison method was used to detect the LULC of the area. The key LULC types were selected for investigation of soil properties. Soil samples were analysed in situ to measure the physicochemical soil properties. The results of this study show remarkable changes in LULC in the period of 18?years. The effect of land cover change on soil properties, soil compaction and soil strength was found to be significant at a level of <0.05.  相似文献   

Panel discussion     

N. Mukunda  H. C. Arp  Geoffrey Burbidge  Ramnath Cowsik  T. Padmanabhan  J. V. Narlikar  Geoff Burbidge  Arati Chokshi  J. C. Pecker  Tarun Souradeep  Pasupathy  Rohini Godbole  Gopal Krishna  D. F. Roscoe 《Journal of Astrophysics and Astronomy》1997,18(4):465-475

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Thermal convection instability of liquid metals in magneto-hydrodynamics     

Rama Singhal  Krishna M. Srivastava 《Astrophysics and Space Science》1983,89(1):33-51

The problem of thermal convection instability of a horizontal layer of magnetized fluid has been studied to occur crystal growing under the effect of horizontal temperature gradient. In the study, the problem has been reduced to an eigen-value problem for a stream function. The dispersion relations for low viscosity fluid and high viscosity fluid respectively have been discussed analytically and some numerical results have been obtained. It is shown that the critical Rayleigh number and other its related constants for low viscosity fluid (i.e., mercury) are much differ than the high viscosity fluid (i.e., glycerol).  相似文献   

Nonlinear electrostatic drift Kelvin-Helmholtz instability     

Avadhesh C. Sharma  Krishna M. Srivastava 《Astrophysics and Space Science》1993,200(1):107-116

Nonlinear analysis of electrostatic drift Kelvin-Helmholtz instability is performed. It is shown that the analysis leads to the propagation of the weakly nonlinear dispersive waves and the nonlinear behaviour is governed by the nonlinear Burger's equation.  相似文献   

Equivalent width of interstellar molecular lines     

K. S. Krishna Swamy  S. P. Tarafdar 《Astrophysics and Space Science》1974,26(1):179-182

We have made an analysis of the observed equivalent widths of the lines of Lyman and Werner bands by Smith. The H₂ column densities of 3×10¹⁹ to 10²⁰ and the excitation temperature of 80 to 150 K satisfy the observations. This temperature refers to the kinetic temperature. We have also discussed the importance of getting the excitation temperature from lines of H₂ and other heteronuclear diatomic molecules for the same star and from different regions of space.  相似文献   

A cocoon model for thermal X-ray sources and ‘Oscillars’     

Krishna M. V. Apparao 《Astrophysics and Space Science》1972,18(2):334-336

A gas cocoon surrounding a neutron star can be heated to a high temperature by the low frequency radiation emitted by the neutron star whose rotation axis is inclined to its magnetic axis. This heated gas can emit X-rays and may be identified with thermal X-ray sources. If the neutron star emission shows periodicities larger than the cooling time of the gas, these will be reflected in the emission of X-ray; the recently observed X-ray sources which show oscillations and quasiperiodicities (Oscillars) may be such sources.  相似文献   

Unsteady flow of a non-Newtonian visco-elastic fluid between two coaxial circular cylinders     

Krishna Raj Choubey 《Astrophysics and Space Science》1984,105(2):301-305

In this paper, the flow of a visco-elastic liquid between two coaxial circular cylinders has been studied when inner cylinder is moving from rest for a certain period with linearly growing speed and then stops suddenly. The Laplace transform technique has been employed to solve the basic differential equations. The expression for the velocity field is obtained.  相似文献   

Errata     

B.V. Krishna MurthyK. Sen Gupta 《Planetary and Space Science》1972

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Analysis of the hyades giant stars ε and γ Tau     

K. S. Krishna Swamy 《Astrophysics and Space Science》1970,8(1):86-89

Two hyades giant stars, and Tau, have been studied from an analysis of strong line profiles. We get for Tau,T _e =4750K and logg=2.7, and for Tau,T _e =4700K and logg=2.8. Hydrogen-to-metal ratio for the two stars is nearly the same as that of solar value.  相似文献   

Aerosol optical depths at Mohal-Kullu in the northwestern Indian Himalayan high altitude station during ICARB     

Jagdish C. Kuniyal  Alpana Thakur  Harinder K. Thakur  Sanjeev Sharma  P. Pant  Pan S. Rawat  K. Krishna Moorthy 《Journal of Earth System Science》2009,118(1):41-48

First time observations of spectral aerosol optical depths (AODs) at Mohal (31.9°N, 77.11°E; altitude 1154 m amsl) in the Kullu valley, located in the northwestern Indian Himalayan region, have been carried out during Integrated Campaign for Aerosols, gases and Radiation Budget (ICARB), as a part of the Indian Space Research Organisation-Geosphere Biosphere Program (ISRO-GBP). AODs at six wavelengths are obtained using Microtops-II Sunphotometer and Ozonometer. The monthly mean values of AOD at 500 nm are found to be 0.27 ± 0.04 and 0.24 ± 0.02 during March and April, 2006 respectively. However, their monthly mean values are 0.33 ± 0.04 at 380 nm and 0.20 ± 0.03 nm at 870 nm during March 2006 and 0.31 ± 0.3 at 380 nm and 0.17 ± 0.2 at 870 nm during April 2006, showing a gradual decrease in AOD with wavelength. The Ångstrom wavelength exponent ‘α’ had a mean value of 0.72 ± 0.05, implying reduced dominance of fine particles. Further, the afternoon AOD values are higher as compared to forenoon values by ～ 33.0% during March and by ～ 9.0% during April 2006 and are attributed to the pollutant lifted up from the valley by the evolving boundary layer. Besides the long-range transportation of aerosol particles by airmass from the Great Sahara and the Thar Desert regions to the observing site, the high values of AODs have also been influenced by biomass burning and frequent incidents of forest fire at local levels.  相似文献