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Water samples from precipitation, glacier melt, snow melt, glacial lake, streams and karst springs were collected across SE
of Kashmir Valley, to understand the hydrogeochemical processes governing the evolution of the water in a natural and non-industrial
area of western Himalayas. The time series data on solute chemistry suggest that the hydrochemical processes controlling the
chemistry of spring waters is more complex than the surface water. This is attributed to more time available for infiltrating
water to interact with the diverse host lithology. Total dissolved solids (TDS), in general, increases with decrease in altitude.
However, high TDS of some streams at higher altitudes and low TDS of some springs at lower altitudes indicated contribution
of high TDS waters from glacial lakes and low TDS waters from streams, respectively. The results show that some karst springs
are recharged by surface water; Achabalnag by the Bringi stream and Andernag and Martandnag by the Liddar stream. Calcite
dissolution, dedolomitization and silicate weathering were found to be the main processes controlling the chemistry of the
spring waters and calcite dissolution as the dominant process in controlling the chemistry of the surface waters. The spring
waters were undersaturated with respect to calcite and dolomite in most of the seasons except in November, which is attributed
to the replenishment of the CO2 by recharging waters during most of the seasons. 相似文献
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SIDDHARTHA BHATTACHARYYA APURBA BERA SOMNATH BHARADWAJ N. D. RAMESH BHAT JAYARAM N. CHENGALUR 《Journal of Astrophysics and Astronomy》2017,38(1):17
We developed a generic formalism to estimate the event rate and the redshift distribution of Fast Radio Bursts (FRBs) in our previous publication (Bera et al. 2016), considering FRBs are of an extragalactic origin. In this paper, we present (a) the predicted pulse widths of FRBs by considering two different scattering models, (b) the minimum total energy required to detect events, (c) the redshift distribution and (d) the detection rates of FRBs for the Ooty Wide Field Array (OWFA). The energy spectrum of FRBs is modelled as a power law with an exponent ?α and our analysis spans a range ?3≤α≤5. We find that OWFA will be capable of detecting FRBs with α≥0. The redshift distribution and the event rates of FRBs are estimated by assuming two different energy distribution functions; a Delta function and a Schechter luminosity function with an exponent ?2≤γ≤2. We consider an empirical scattering model based on pulsar observations (model I) as well as a theoretical model (model II) expected for the intergalactic medium. The redshift distributions peak at a particular redshift z p for a fixed value of α, which lie in the range 0.3≤z p ≤1 for the scattering model I and remain flat and extend up to high redshifts (z?5) for the scattering model II. 相似文献
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A combination of ray theory and diffraction theory has been used to simulate reflections of seismic pulses from a full plane and reflections and diffractions from a half plane buried horizontally in earth models with linear increase of velocity with depth. Wave forms of signals reflected from a full plane in this case are modifications of the source pulse, even if the medium is assumed to be perfectly elastic. The extent of pulse modification increases with increase of the velocity gradient. The duration of the reflected pulse is always longer than that of the source pulse. The pulses diffracted from the edge of the half plane in such cases do not lie along hyperbolic curves in the time-offset plane. Diffracted signals can be observed only up to a limited distance from the edge of the half plane equalling half the horizontal range of the ray which is tangential to the half plane and has its end points at the level of the source and the receiver. 相似文献
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