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Halder Debjani Kheroar Shyamal Srivastava Rajiv Kumar Panda Rabindra Kumar 《Theoretical and Applied Climatology》2020,140(3):823-838
Theoretical and Applied Climatology - Temperature and CO2 are the two most important climate parameters that affect crop yield directly. In this study, the impact of these two parameters on the... 相似文献
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Interannual variability in the Biannual Rossby waves in the tropical Indian Ocean and its relation to Indian Ocean Dipole and El Nino forcing 总被引：1，自引：0，他引：1
The interannual variability of the tropical Indian Ocean is studied using Simple Ocean Data Assimilation (SODA) sea surface
height anomalies (SSHA) and Hadley Centre Ice Sea Surface Temperature anomalies. Biannual Rossby waves (BRW) were observed
along the 1.5° S and 10.5° S latitudes during the Indian Ocean Dipole (IOD) years. The SODA SSHA and its BRW components were
comparable with those of Topex/Poseidon. The phase speed of BRW along 1.5° S is −28 cm/s, which is comparable with the theoretical
speed of first mode baroclinic (equatorially trapped) Rossby waves. This is the first study to show that no such propagation
is seen along 1.5° S during El Nino years in the absence of IOD. Thus the westward propagating downwelling BRW in the equatorial
Indian Ocean is hypothesized as a potential predictor for IOD. These waves transport heat from the eastern equatorial Indian
Ocean to west, long before the dipole formation. Along 10.5° S, the BRW formation mechanisms during the El Nino and IOD years
were found to be different. The eastern boundary variations along 10.5° S, being localized, do not influence the ocean interior
considerably. Major portion of the interannual variability of the thermocline, is caused by the Ekman pumping integrated along
the characteristic lines of Rossby waves. The study provides evidence of internal dynamics in the IOD formation. The positive
trend in the downwelling BRW (both in SODA and Topex/Poseidon) is of great concern, as it contributes to the Indian Ocean
warming. 相似文献
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Magnetoelastic disturbances in a perfectly conducting cylindrical shell in a constant magnetic field
Sachindra Kumar Bakshi 《Pure and Applied Geophysics》1969,76(1):56-64
Summary The paper deals with the problem of determining the displacements, stresses, magnetic and the electric fields of an infinite shell placed in vacuum and subjected to an impulsive excitation load. 相似文献
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A high level of electrostatic turbulence can be generated by plasma instabilities in solar flares. The turbulence, in general, has both quasistatic (ionic) and dynamic (electronic) components. Hydrogenic line profiles develop distinct features under the simultaneous effect of the quasistatic and dynamic turbulent electric fields: these features are discussed and the possible inferences that can be drawn as to the nature of the turbulent electric fields through their observation are pointed out. Solar flare spectral diagnostics along these lines can provide an observational test of the existence of turbulent electric fields in the flare region. When a detailed determination of the characteristics of these fields is feasible, it would, in turn, help in identifying the underlying plasma instability mechanisms that give rise to these fields during the flare build-up and associated processes. 相似文献
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Bakshi P. Bianchi C. Rajan S. Sivaprasad K. 《Oceanic Engineering, IEEE Journal of》1987,12(2):433-442
A simple direct inversion scheme for computing the velocity profile of an inhomogeneous slab from reflected data using the order-of-scattering method of solving the Riccati equation for a lossless medium is presented. Extension of this method to the estimation of the constant attention in a low-loss dispersive medium is also indicated. 相似文献
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Srivastava R. K. Panda R. K. Halder Debjani 《Theoretical and Applied Climatology》2017,129(3-4):1211-1225
Theoretical and Applied Climatology - The primary objective of this study was to evaluate the performance of the time-domain reflectometry (TDR) technique for daily evapotranspiration estimation of... 相似文献
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Prabal Shankar Das Rima Chatterjee Sumangal Dasgupta Ranajit Das Debjani Bakshi Mukesh Gupta 《Geophysical Prospecting》2019,67(1):150-166
Sands belonging to Kamalapuram Formation of Paleocene-Eocene age are deposited in Cauvery basin as incised valley fill during a regressive cycle. Here we attempt to quantify the influence of diagenesis on pore-filling materials using rock physics template constrained by geohistory modelling. Primarily, porosity–velocity and acoustic impedance – the ratio of P-wave and S-wave velocity (VP/Vs) cross-plots are used as rock physics templates. Rock physics template has efficiently quantified pore-filling materials namely; contact cement and non-contact cement. The estimated contact cement and non-contact cement are correlated with conventional petrophysical logs within the selected depth interval. Further, this correlation is used to interpret the composition of pore-filling materials. Shallower depth intervals (I and II) exhibit moderate non-contact cement (4–5%) and insignificant contact cement (1–2% approx.) depositions. However, deeper interval (III) records a significant amount of pore-filling materials amounting average of 12% non-contact cement and 4% contact cement. Pore-filling materials demonstrate a positive correlation with the depth of burial. The fluid response is substantially affected by the degree of diagenesis, composition and spatial distribution of pore-filling materials. Shallower depth intervals (1770–1786 m and 1858–1878 m) are relatively more sensitive to fluid changes as it is affected by insignificant contact cement. The depth interval 1770–1786 m shows class II (oil) and class III (gas) amplitude variation with offset anomalies. The sand occurring in depth interval 1858–1878 m demonstrates class IIP (oil) and II (gas) anomaly. The deeper interval (2118–2170 m) is comparatively stiffer and demonstrates class I amplitude variation with offset (oil and gas sand) anomaly. 相似文献
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