Modelling Settlement Patterns for Metropolitan Regions: Inputs from Remote Sensing     

P. Misra 《Journal of the Indian Society of Remote Sensing》1996,24(4):287-289

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IGU commission on regional systems and policies     

Misra  R. P. 《GeoJournal》1983,7(5):461-461

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Evaluation of fertility indicators associated with arsenic-contaminated paddy fields soil   总被引：1，自引：0，他引：1  

P. S. Chauhan  S. K. Mishra  S. Misra  V. K. Dixit  S. Pandey  P. Khare  M. H. Khan  S. Dwivedi  A. Lehri 《International Journal of Environmental Science and Technology》2018,15(11):2447-2458

Emerging environmental issues related to heavy metal contamination in rice draw great concern about the soil quality of paddy farming lands irrigated with groundwater. Investigating the functioning of soil microorganisms exposed to heavy metal contamination is imperative for agricultural soil manipulations. The current study accentuates the influence of heavy metals on microbial activity and community composition in arable soil of West Bengal State of India. The result revealed that the fertility indicators (activity of all soil enzymes) and growth-limiting factors (soil N and P) were negatively correlated with the heavy metal stress except the soil total organic content which demonstrated significant positive correlation with the heavy metals. In case of functional diversity of soil, all the considered diversity indices exhibited no specific pattern along with the availability of heavy metals. Further, despite the heavy metal contamination, we observed a very complex and indifferent pattern of bacterial community composition along the heavy metal contamination sites. Overall, we found that γ-Proteobacteria had been the most abundant bacterial community followed by Actinobacteria, Firmicutes, β-Proteobacteria and α-Proteobacteria. Commemorating all the results, we can infer that arsenic and other heavy metal contamination is deteriorating the soil quality and hence warrants immediate attention of concerned soil scientist and agronomists.  相似文献   

Modeling the X-Ray Timing Properties of Cygnus X-1 Caused by Waves Propagating in a Transition Disk     

Misra R 《The Astrophysical journal》2000,535(2):L95-L98

We found a subsystem of globular clusters in M31 that appears to have a formation history separate from the rest. The member clusters of this subsystem, identified from their distinct distribution in the metallicity-distance diagram, (1) have a common medium metallicity range of -0.9<&sqbl0;Fe&solm0;H&sqbr0;<-0.4, (2) have a line-of-sight velocity distribution with no significant projected rotational motion, and (3) are populated outside the inner subsystem of globular clusters of similar metallicity that shows a significant net rotational motion as a whole. We suggest that this subsystem of globular clusters was formed during a merging event of a dwarf galaxy that took place well after the initial collapse event when most of the globular clusters in M31 were formed.  相似文献   

Archean Granitoids at the Contact of Eastern Ghat Granulite Belt and Singhbhum-Orissa Craton, in Bhuban-Rengali Sector, Orissa, India     

S. Misra  S. Moitra  S. Bhattacharya  T.V. Sivaraman 《Gondwana Research》2000,3(2):205

The small granite plutons occurring at the contact of the Singhbhum-Orissa Iron Ore craton (IOC) to the north and the Eastern Ghat Granulite Belt (EGGB) to the south in eastern Indian shield are characterised by the presence of enclaves of the granulites of EGGB and the greenschist facies rocks of IOC. These granites also bear the imprints of later cataclastic deformation which is present at the contact of the IOC and the EGGB. In situ Pb-Pb zircon dating of these granites gives minimum age of their formation 2.80 Ga. A whole-rock three point Rb-Sr isochron age of this rock is found to be 2.90 Ga. Therefore, the true age of formation of these granites will be around 2.90–2.80 Ga. These granitic rocks also contain xenocrystic zircon components of 3.50 Ga and show a later metasomatic or metamorphic effect 2.48 Ga obtained from the analyses on overgrowths developed on 2.80 Ga old zircon cores. The presence of granulitic enclaves within these contact zone granite indicates that the granulite facies metamorphism of the EGGB is 2.80 Ga or still older in age. The cataclastic deformations observed at the contact zone of the two adjacent cratons is definitely younger than 2.80 Ga and possibly related to 2.48 Ga event observed from the overgrowths. As 2.80 Ga granite plutons of small dimensions are also observed at the western margin of the IOC; it can be concluded that a geologic event occurred 2.80 Ga over the IOC when small granite bodies evolved at the marginal part of this craton after its stabilisation at 3.09 Ga.  相似文献   

http://www.sciencedirect.com/science/article/pii/S1674987113000546     

Saibal Gupta  William K.Mohanty  Animesh Mandal  Surajit Misra 《地学前缘(英文版)》2014,5(1):17-24

In the eastern part of the Indian shield,late PaleozoiceMesozoic sedimentary rocks of the Talchir Basin lie precisely along a contact of Neoproterozoic age between granulites of the Eastern Ghats Mobile Belt(EGMB)and amphibolite facies rocks of the Rengali Province.At present,the northern part of the basin experiences periodic seismicity by reactivation of faults located both within the basin,and in the Rengali Province to the north.Detailed gravity data collected across the basin show that Bouguer anomalies decrease from the EGMB(wt15 mGal),through the basin(w 10 mGal),into the Rengali Province(w 15 mGal).The data are consistent with the reportedly uncompensated nature of the EGMB,and indicate that the crust below the Rengali Province has a cratonic gravity signature.The contact between the two domains with distinct sub-surface structure,inferred from gravity data,coincides with the North Orissa Boundary Fault(NOBF)that defnes the northern boundary of the Talchir Basin.Post-Gondwana faults are also localized along the northern margin of the basin,and present-day seismic tremors also have epicenters close to the NOBF.This indicates that the NOBF was formed by reactivation of a Neoproterozoic terrane boundary,and continues to be susceptible to seismic activity even at the present-day.  相似文献   

Corrected Hawking temperature of Warped AdS3 rotating Black Hole by using tunneling method     

Rajesh Misra  Chandra Rekha Mahanta 《Astrophysics and Space Science》2013,344(1):63-67

In this paper, we have calculated the corrected Hawking temperature for the Warped AdS₃ rotating Black Hole by using the tunneling method beyond the semi-classical approximation for the Warped AdS₃ rotating Black Hole. For this purpose, we have isolated the r-t sector of the metric from the angular part throughout a coordinate transformation near the horizon.  相似文献   

Modulational instability of ion-acoustic wave packets in quantum pair-ion plasmas     

A. P. Misra  N. K. Ghosh 《Astrophysics and Space Science》2011,331(2):605-609

Amplitude modulation of quantum ion-acoustic waves (QIAWs) in a quantum electron-pair-ion plasma is studied. It is shown that the quantum coupling parameter H (being the ratio of the plasmonic energy density to the Fermi energy) is ultimate responsible for the modulational stability of QIAW packets, without which the wave becomes modulational unstable. New regimes for the modulational stability (MS) and instability (MI) are obtained in terms of H and the positive to negative ion density ratio β. The growth rate of MI is obtained, the maximum value of which increases with β and decreases with H. The results could be important for understanding the origin of modulated QIAW packets in the environments of dense astrophysical objects, laboratory negative ion plasmas as well as for the next generation laser solid density plasma experiments.  相似文献   

Relationship between interplanetary (IP) parameters and geomagnetic indices during IP shock events of 2005     

Jatin Rathod  Girija Rajaram  Radharani Alyana  A. Chandrasekhar Reddy  D. S. Misra  C. G. Patil  M. Y. S. Prasad  A. G. Ananth 《Journal of Astrophysics and Astronomy》2008,29(1-2):293-302

In the present study, we investigate the possible relationship of IP parameters of solar wind and interplanetary magnetic field with ground-based geomagnetic indices. To carry out the study, we take all the IP shock events listed by Proton Monitor onboard Solar and Heliospheric Observatory (SOHO) during 2005, and plot the time variations of all the IP parameters and geomagnetic parameters (±5 days), centered at the shock arrival time. Next, we obtain scatter plots of absolute values of solar wind parameters such as Vsw, Nsw and Interplanetary Magnetic Field (IMF) components Bx, By, Bz and total B with the values of geomagnetic parameters such as Dst, Kp indices, dayside Magnetopause (MP) distance and Cosmic-Ray Neutron Monitor count (CRNM). The scatter plots show that before the IP shock, the pattern is random with no clear relationship. Following the shock, a clear pattern emerges with a type of relationship being seen — clear for SHARP shocks and less clear for DIFFUSE shocks. A total of 10 shock events for 2005 have been studied. Typical examples of this behaviour are the shock events of January 21, 2005 and May 15, 2005. Our study suggests a definite correlation between changes in the solar wind and interplanetary magnetic field parameters and ground-based geomagnetic response. We are trying to obtain quantitative relationships between these for shock events of 2005.  相似文献   

<Emphasis Type="Bold">Rhodophycean algae from the Lower Cretaceous of the Cauvery Basin,South India</Emphasis> by P.K. Misra,S. Kishore,S.K. Singh and A.K. Jauhri. Jour. Geol. Soc. India,v.73, 2009, pp.325–334     

P. K. Misra  S. Kishore  S. K. Singh  A. K. Jauhri 《Journal of the Geological Society of India》2009,74(1):139-140

Discussion

Rhodophycean algae from the Lower Cretaceous of the Cauvery Basin, South India by P.K. Misra, S. Kishore, S.K. Singh and A.K. Jauhri. Jour. Geol. Soc. India, v.73, 2009, pp.325–334  相似文献