Landscape ecology, inter alia, addresses the question as to how altered landscape patterns affect the distribution, persistence, and abundance of a species.
Landscape ecology plays an important role in integrating the different scales of biodiversity from habitat patch to biome
level. Satellite remote sensing technology with multi-sensor capabilities offers multi-scale information on landscape composition
and configuration. Advances in geospatial analytical tools and spatial statistics have improved the capability to quantify
spatial heterogeneity. Globally, landscape level characterization of biodiversity has become an important discipline of science.
Considering the vast extent, heterogeneity, and ecological and economic importance of forest landscapes, significant efforts
have been made in India during the past decade to strengthen landscape level biodiversity characterization. The generic frame
work of studies comprises preparation of national databases providing information on composition and configuration of different
landscapes using multi-scale remote sensing techniques, understanding the landscape patterns using geospatial models to elicit
disturbance and diversity patterns and application of this information for bioprospecting and conservation purposes. Studies
on hierarchical linkage of multi-scale information to study the processes of change, landscape function, dynamics of habitat
fragmentation, invasion, development of network of conservation areas based on the understanding of multi-species responses
to landscape mosaics, macro-ecological studies to understand environment and species richness, habitat and species transitions
and losses, landscape level solutions to adaptation and mitigation strategies to climate change are a few of the future challenges.
The paper presents the current experiences and, analyses in conjunction with international scenario and identifies future
challenges of Indian landscape level biodiversity studies. 相似文献
A cosmological model has been constructed in the framework of Brans-Dicke(BD) gravity,based on an inter-conversion between matter and dark energy, for a spatially flat universe in the era of pressureless dust. To account for the non-conservation of the matter content, a function of time f(t) has been arbitrarily put into the expression for the density of matter(ρa^3= f(t)ρ_0 a_0~3). By definition, f(t) is proportional to the matter content of the universe. Using suitable ansatzes for the scale factor and scalar field, the functional form of f(t) has been determined from the BD field equations. The scale factor has been so chosen that it would cause a signature flip in the deceleration parameter with time. The function f(t) decreases monotonically with time, indicating a transformation of matter into dark energy. The time dependence of the proportions of matter and dark energy in the universe has been determined. The effect of non-conservation of the matter content upon various cosmological parameters has been explored in the present study. Two models of matter-energy interaction have been proposed and f(t) has been expressed as a function of their interaction term. The dark energy equation-of-state(EoS) parameter has been expressed and analyzed in terms of f(t). 相似文献
The main objective of the present research was to examine the risk of fluoride-rich groundwater in the Shanmuganadhi River basin, south India on human health. The non-carcinogenic risks were estimated into two classes: (1) risks associated with oral intake of water and (2) risks associated with dermal contact. Hazard Quotient for oral intake and dermal contact was separately calculated for adult men, adult women and children from the geochemical results of 61 representative samples collected from the wells constructed in hard rock aquifers during the post- (January-2018) and pre-monsoon (May-2018) seasons. The collected samples were analyzed immediately after the field work for all the major ions and fluoride. Finally, total hazard index was calculated for adults (men and women) and children to evaluate the risk. It directed that 41%, 49% and 74% of post-monsoon samples and 30%, 43% and 62% of pre-monsoon samples possessed a non-carcinogenic risk for men, women and children, respectively. Because the basin falls in the drought-prone region, the water supply for drinking and cultivation are commonly based on groundwater resources. The study revealed that the minerals such as apatite, fluorite, biotite and pyroxene in the hornblende–biotite gneiss formation contribute fluoride ions to the groundwater system due to water–rock interaction mechanism. The Durov diagram depicted that dissolution of silicate minerals and cation exchange are the foremost hydrogeochemical activities, which decide the overall chemical composition of groundwater in this region. The ionic concentrations including fluoride increased with respect to depth of occurrence of groundwater. Escalation of the water table due to monsoon recharge and artificial recharge through a check dam decreased the total dissolved solids and fluoride ion concentration. The investigation conducted around the existing check dam at Kaldurai village highlighted that the fluoride concentration is below the allowable limit of 1.5 mg/l (WHO in World health statistics 2017: monitoring health for the SDGs, Sustainable Development Goals. World Health Organization, Geneva, 2017) in the wells closer to the check dam toward the downstream side. The concentration increased with distance, which lead the groundwater unsuitable for consumption. Therefore, it is recommended to implement the managed aquifer recharge using check dams in the other parts of the basin to enrich the quantity and applicability of groundwater.
We introduce a photogravitational version of Hill's problem to include the effect of radiation of the primaries, and discuss
its equilibrium points and zero velocity curves. As a first application we use this model to study Hill stability of orbits
around the small primary. The estimates obtained for the maximum distance of Hill stable orbits are compared to the predicted
maximum sizes of accretion disks in binary stars according to recent theories based on periodic orbits as streamlines of the
disks.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
The data from OGO-5 and OSO-7 X-ray experiments have been compared with optical data from six chromospheric flares with filament disruption associated with slow thermal X-ray bursts. Filament activation accompanied by a slight X-ray enhancement precedes the first evidence of Hα flare by a few minutes. Rapid increase of the soft X-ray flux accompanies the phase of fastest expansion of the filament. Plateau or slow decay phases in the X-ray flux are associated with slowing and termination of filament expansion. The soft X-ray flux increases as F~(A + Bh) h, where h is the height of the disrupted prominence at any given time and A and B are constants. We suggest that the soft X-ray emission originates from a growing shell of roughly constant thickness of high-temperature plasma due to the compression of the coronal gas by the expanding prominence. 相似文献
Einstein's equations have been solved for perfect fluid distribution. The solution obtained may be considered as inhomogeneous generalisation of Bianchi type-VIo cosmological model. 相似文献