Characterization of Mechanisms and Processes Controlling Groundwater Recharge and its Quality in Drought-Prone Region of Central India (Buldhana,Maharashtra) Using Isotope Hydrochemical and End-Member Mixing Modeling     

Keesari  Tirumalesh  Roy  Annadasankar  Mohokar  Hemant  Pant  Diksha  Sinha  U. K. 《Natural Resources Research》2020,29(3):1951-1973

A thorough study on understanding of groundwater recharge sources and mechanisms was attempted by integrating the hydrogeological, geochemical and isotopic information along with groundwater dating and end-member mixing analysis (EMMA). This study was necessitated due to prolonged dryness and unavailability of freshwater in semi arid Deccan trap regions of Central India. In addition, groundwater resources are not characterized well in terms of their geochemical nature and recharge sources. The hydrogeochemical inferences suggest that aquifer I consists of recently recharged water dominated by Ca–Mg–HCO₃ facies, while groundwater in aquifer II shows water–rock interaction and ion exchange processes. Presence of agricultural contaminant, nitrate, in both aquifers infers limited hydraulic interconnection, which is supported by unconfined to semi-confined nature of aquifers. Groundwater in both aquifers is unsaturated with respect to carbonate and sulfate minerals indicating lesser water–rock interaction and shorter residence time. This inference is corroborated by tritium age of groundwater (aquifer I: 0.7–2 years old and aquifer II: 2–4.2 years old). Stable water isotopes (δ²H, δ¹⁸O) suggest that groundwater is a mixture of rainwater and evaporated water (surface water and irrigation return flow). EMMA analysis indicates three groundwater recharge sources with irrigation return flow being the dominant source compared to others (rainwater and surface waters). A conceptual model depicting groundwater chemistry, recharge and dynamics is prepared based on the inferences.

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On the MgH oscillator strengths     

K. Sinha 《Journal of Astrophysics and Astronomy》1981,2(3):285-288

The theoretical estimates of the oscillator strengths by Kirby, Saxon and Liu (1979) for theA II₂ — XΣ² system of the MgH molecule are compared with the solar photospheric results. It is found that the two results are in reasonable agreement.  相似文献   

Measurement of electron temperatures in the lower ionosphere by detecting the space potential on the langmuir probe characteristic     

B.H. Subbaraya  Satya Prakash  S.P. Gupta  H.S.S. Sinha 《Planetary and Space Science》1974,22(1):180-181

Electron temperatures have been determined at Thumba on Nike Apache flight 10.11 (12 March 1967, 1857 hr IST) by the usual retarding potential analysis and by using an a.c. modulation technique for detecting the space potential on the Langmuir probe characteristic. Simultaneous measurements with the two techniques show that the space potential technique gives temperatures which are related to the temperatures obtained from the retarding potential analysis in a manner remarkably similar to the relations obtained by Booker and Smith as well as by Carlson and Sayers between radar temperatures and d.c. probe temperatures. This result is interesting in view of the fact that radar temperatures have been found to be in good agreement with the temperatures obtained by a.c. modulation techniques on satellite borne probes. The space potential technique is simple, requires limited additional electronics, does not make stringent demands on telemetry and can be easily adopted for rocket borne Langmuir probes.  相似文献   

Spectrophotometry of Comet Bradfield (1980t) during post-perihelion period     

P. S. Goraya  B. K. Sinha  U. S. Chaubey  B. B. Sanwal 《Earth, Moon, and Planets》1982,26(1):3-9

Spectrum scans of the head of Comet Bradfield (1980t) covering the wavelength range 365–640 nm were made on two nights when the heliocentric distance of the comet varied from 0.55 to 0.58 AU. The emission features of the CN band at 388 nm and Swan band sequence of C₂ at 474 nm, 516 nm, and 563 nm are identified and absolute fluxes in these bands as well as in the continuum are derived. The continuum energy distribution curves of the comet have been compared with those of the Sun and the star Crv (G5 III). An estimate of the number of C₂ and CN molecules in the head of the comet has been made through the measured intensities of their respective bands lying in this region.  相似文献   

The diurnal heat budget of the thermosphere     

S. Chandra  A.K. Sinha 《Planetary and Space Science》1973,21(4):593-604

Detailed numerical calculations of thermospheric heat sources and sinks are presented and their relative importance is discussed in reference to the energy balance phenomena of the neutral atmosphere. It is shown that the thermal energy available from the absorption in the Schumann-Runge continuum leading to photo-dissociation of O₂ is by far the largest energy source in the lower thermosphere. Other sources of varying importance in different altitude ranges are: (1) energy from photoelectrons; (2) energy exchange from thermal plasma; (3) chemical reaction (ion-electron dissociative recombination) energy gain; (4) kinetic and dissipative energy associated with the neutral wind. The energy sinks of importance are (1) thermal conduction at the lower boundary (120km); and (2) radiative cooling of atomic oxygen.It is shown that the combined energy from processes 2–4 constitutes only a small fraction of the total energy available from photoelectrons and is in phase with the latter. These secondary sources (processes 2–4), therefore, do not constitute a significant energy source and their contribution can be simply incorporated into photoelectron energy (process 1) by defining an effective photo-ionization heating efficiency. The heating efficiencies for photo-ionization (including processes 2–4) and photo-dissociation are estimated to be 0.5 and 0.3, respectively.As the important heat input (photo-dissociation) and loss (conduction and radiation) rates are basically governed by the O₂ and O densities, any diurnal or seasonal variation in these constituents at the lower boundary would have profound effects on the thermal structure of the overlying atmosphere. For this and other reasons, it is suggested that a choice of lower boundary much below 120km, e.g. near the mesopause level (90 km), should be more appropriate for general thermospheric studies.  相似文献   

Tectonic significance of Th/U ratios from Archean basalts     

A.K. Sinha 《Chemical Geology》1976,18(3):215-225

Observed Th/U ratios from Archean basalts have been altered by metamorphism and/or recent weathering. Experimental leaching of Th and U from these basalts suggests that great care is necessary in using directly observed ratios for any petrogenetic models. Calculated Th/U ratios (based on Pb isotopic composition) when used with an index oxide (SiO₂) may reveal the depth of formation of these basalts.  相似文献   

Rate of change of vorticity covariance in turbulence     

N. Kishore  Abhilasha Sinha 《Astrophysics and Space Science》1987,135(1):191-193

The present paper deals with the turbulent flow of an incompressible viscous fluid which is isotropic and spatially homogeneous. The expression for the rate of change of vorticity covariance is derived. The derived result shows that the defining scalars (r, t) and (r,t) of the rate of change of vorticity covariance solely depend upon the defining scalarQ of the two-point velocity correlation.  相似文献   

On disturbances in a semi-infinite medium traversed by a transverse magnetic field     

Dilip K. Sinha 《Pure and Applied Geophysics》1965,60(1):18-22

Summary The method of operational calculus has been used to deal with the disturbances in an elastic medium traversed by a magnetic field.  相似文献   

An active source electromagnetic sounding system for marine use   总被引：2，自引：0，他引：2  

M. C. Sinha  P. D. Patel  M. J. Unsworth  T. R. E. Owen  M. R. G. Maccormack 《Marine Geophysical Researches》1990,12(1-2):59-68

Instrumentation has been developed for carrying out active source electromagnetic sounding experiments in the deep oceans. Experiments of this type are directly and uniquely sensitive to the presence of molten or partially molten material, to temperature structure and to the porosity of upper crustal rocks such as those that accommodate hydrothermal circulation systems. Electromagnetic sounding experiments therefore represent an extremely desirable addition to the existing range of geophysical techniques for studying geological processes in thermally, hydrothermally or magmatically active regions—for example, at oceanic spreading centres.The instruments can be operated in regions of rugged, unsedimented sea bottom terrain, and are designed for investigating the distribution of electrical conductivity within the oceanic crust and uppermost mantle. The instrumentation consists of a deep towed, horizontal electric dipole transmitter and a set of free-fall, sea bottom, horizontal electric field recording devices.The transmitter is a deep-towed instrument, which is provided with power from the towing ship through a conducting cable. The transmitter package is fitted with an integral echo sounder, which allows it to be towed safely a short distance above the seabed. Electromagnetic signals are transmitted from a neutrally-buoyant antenna array, which is streamed behind the deep tow.The sea bottom receiving instruments each consist of a recoverable package which contains the instrumentation and digital recording system, an acoustic release unit, four low-noise, porous electrodes arranged in two orthogonal, horizontal dipoles, and a disposable bottom weight.The instruments have been used at sea on three occasions. On their most recent use, active source signals were successfully recorded during an experiment to investigate crustal magmatism and hydrothermal circulation beneath the axis of the East Pacific Rise.  相似文献   

Variation of γ-Ray and Particle Fluxes At the Sea Level During the Total Solar Eclipse of 24 October, 1995     

Abhijit Bhattacharyya  Sukumar Biswas  Barun K. Chatterjee  Mala Das  Pradipta K. Das  Tapan K. Das  Tarun K. De  M.H. Engineer  Rabi N. Mukherjee  Sibaji Raha  S.C. Roy  Swapan K. Saha  A.K. Sen  Bikash Sinha  Debapriyo Syam 《Astrophysics and Space Science》1997,250(2):313-326

A Total Solar Eclipse (TSE) was observed from Diamond Harbour (lat. 22.2°N, long 88.2°E) on 24 October 1995. The variation of -ray intensity was measured in the energy range of 0.3–3.0 MeV for different time spans throughout the period of the eclipse. A CR-39 detector was used to look at the change in the fluxes of neutral and charged particles. The maximum drop ( 25%) in the intensity of -ray was observed in the range 2.5–3 MeV during TSE. The CR-39 results showed the appearance of a good number of tracks and a small variation of proton and neutron flux of 10% which was not significant statistically. Low energy -ray fluxes at sea level originate from the secondary electron-photon components of cosmic rays in the atmosphere; its modulation by TSE is interpreted as follows. The cooling of the atmosphere in the path of the umbra induces a reduction of the height of the main production layer of the nuclear component, as a result of which, fewer µ^± mesons (from the decay of the^± mesons) decay to e^±. This leads to a small reduction in the flux of electron-photon component at sea level which originates from this branch; the main branch of e - component from ⁰ decay remains nearly unaffected. As the total mass of air remains the same, little or no change in the slow proton or the neutron flux at sea level is expected. These are consistent with the present observations. For a better understanding, further studies of this new phenomenon during future TSE are suggested.  相似文献