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81.
Dr. Niranjan Deb Chatterjee 《Contributions to Mineralogy and Petrology》1962,8(6):432-439
Occurences of stable vesuvianite-epidote paragenesis within greenschist facies of metamorphism are described. It is suggested that this paragenesis gives way to grossularite-diopside (plus vesuvianiteor epidote) assemblage in the almandine-amphibolite facies. This interpretation conforms best to the results of petrographic observations and also satisfies the topological requirements of the CaO-(Mg, Fe2+, Mn)O-(Al, Fe3+)2O3-SiO2H2O-CO2 system, to which these assemblages belong. Contrary to the ideas in vogue, it is suggested that vesuvianite can very well originate within the greenschist facies, whereas the appearence of grossularite and diopside (consequent on which vesuvianite and epidote becomesmutually incompatible) ushers the almandine-amphibolite facies in. 相似文献
82.
M. Deb 《Mineralium Deposita》1979,14(1):21-31
Massive stratiform zinc-lead-copper sulfide ores, in association with cordierite-anthophyllite rocks, occur in adjacent localities of Ambaji and Deri, in Western India. The metasedimentary country rocks, interlayered with amphibolites and intruded by acidic to intermediate plutonic rocks, belong to the Precambrian Delhi Supergroup. The ore minerals identified by detailed mineragraphic studies include: sphalerite, galena, chalcopyrite, pyrite, pyrrhotite (both monclinic and hexagonal phases), magnetite, ilmenite, rutile, arsenopyrite, molybdenite, cubanite, mackinawite, boulangerite, gudmundite, meneghinite, lautite, tenantite, native bismuth, native silver, chalcocite and covellite. The common sulfide-silicate schistosity in the ores, flowage of sulfide streaks and tails around rotated poikiloblasts and in their pressure shadow region developed during early folding (F1) and regional metamorphism of the rocks under green schist facies condition. These were superimposed by a pervasive hornfelsic fabric involving sulfides and silicates and including microfabrics due to annealing and grain growth in sulfides, during a subsequent phase of low pressure thermal metamorphism and related tectonism (F2). Finally certain deformation features and some uncommon fabrics like martensitic lamellae in galena and subgrains in sphalerite developed during a mild deformation episode (F3) in the waning stages of tectonism in the area. Compositional change in the ores during thermal metamorphism was minimal. 相似文献
83.
The Neoproterozoic Purana succession in the eastern part of Chattisgarh basin around Sarangarh has been classified into a conglomerate-sandstone-shale dominated proximal assemblage, and a lithographic limestone-shale dominated distal assemblage. The proximal assemblage constitutes the Chandarpur Group, and unconformably overlies the Archean crystalline basement complex. The Chandarpur succession has been classified into three formations that were deposited in fan-fan delta, deep water prodelta and storm- tide dominated prograding shelf environments. The distal assemblage, the Raipur Group, conformably overlies the Chandarpur Group, and may be subdivided into two shale-dominated formations separated by a limestone-dominated formation. The limestone sequence, the Sarangarh Limestone, comprises a lower member of mixed carbonate-siliciclastic succession deposited in a storm dominated shallow water platform, and an upper member of pelagic limestone that grades upward into a deep water shale, the Gunderdehi Shale. The rapid transition from shallow water platformal succession to deep-water pelagic limestone and shale points to abrupt deepening of the basin and drowning of the craton. The peak of transgression is represented by a persistent horizon of black limestone, a product of basin wide anoxia. Disposition of facies belts in proximal and distal assemblages and palaeocurrent directions measured from different facies belts point to a north-northwesterly palaeoslope of the basin. Signatures of intense storm and tidal currents in different litho-units collectively point to an open marine circulation condition. It has been inferred that the basin was connected to a major seaway that skirted the northern and north-western margin of the craton. Development of thick fan-delta sequence at the base of the succession, occurrence of felsic welded tuff within the Gunderdehi Shale, thick sandstone-mudstone cyclothems in the Chandarpur Group, and abrupt drowning of the carbonate platform leading to pelagic sedimentation collectively point to major tectonic control on basin evolution. The basin developed as a cratonic rift and evolved into a deeply subsiding one, without any major stratigraphic hiatus, through episodic tectonic pulses. 相似文献
84.
Sarbani Patranabis Deb 《Journal of Earth System Science》2005,114(3):211-226
The Neoproterozoic Kansapathar Sandstone of the Chattisgarh basin, a shallow marine shelf bar sequence, consists of mineralogically
and texturally mature sandstones with subordinate siltstones, mudstones and conglomerates. The sediments were transported,
reworked and deposited in subtidal environments by strong tidal currents of macrotidal regime as well as storms, and accumulated
as discrete shoaling-upward features, separated from each other by muddy to low-energy sandy deposits. The sandbodies developed
into shoaling up linear bars, often more than a kilometre in length, through accretion of thick cross-stratified units in
transverse directions under the influence of ebb and flood tidal currents, as well as in longitudinal direction affected by
southeasterly flowing along-shore currents. The aggrading upper surfaces of the bars experienced protracted reworking by strong
oscillatory wave currents leading to extensive development of subaqueous 2D or 3D dunes mantled with lag pebble deposits at
different points. With continued shoaling and progradation, the bars amalgamated into large sandstone sheets with the development
of high energy beach deposits and coastal sand flats in the uppermost part of the sequence. The presence of rill marks, flat-topped
ripples, wrinkle marks, desiccation cracks and adhesion warts point to intertidal conditions with intermittent exposure. The
high energy sandstone bars overlie a thick mudstone-dominated shelf sequence across a sharp interface indicating rapid change
in the sea-level, provenance, rate of sediment generation and sediment input, and circulation condition in the shelf. A quiet
muddy shelf was replaced by a major sand-depositing environment with strong, open marine circulation. An interplay of tidal
currents, oscillatory wave currents and storm currents generated a complex flow pattern that varied in time and space from
bimodal-bipolar to strongly unimodal flows.
Close parallelism of wave ripple crests, trend of linear bars and unidirectional flows suggest that the elongate bars were
parallel to sub-parallel to the coastline, and were strongly influenced by along shore drift. The inferred coastline was broadly
N-S. The large-scale structures in the bar sandstones, emplacement of vast amount of sand and migration of large bedforms
under strong macrotidal currents collectively indicate that the Kansapathar shelf was intimately connected with an open ocean
basin towards north-northwest. 相似文献
85.
Debasis Deb Akshay Kumar Rajat Pal Singh Rosha 《Geotechnical and Geological Engineering》2006,24(4):1021-1037
Leg pressure data from all shields of a longwall face are monitored and recorded in the surface computer. An algorithm is
developed to detect peak pressures or periodic roof weightings from these pressure data. The intensities and locations of
periodic roof weighting are further analyzed using artificial neural network for forecasting of forthcoming shield pressures.
The network was trained using data 153 m (500 ft) of face advance. Shield pressures are forecasted for the successive nine
mining cycles or approximately 9 m of face advancement. The results obtained validate the efficacy of the developed model. 相似文献
86.
A. K. Upadhyay K. K. Gupta J. K. Sircar M. K. Deb G. L. Mundhara 《Environmental Geology》2007,51(8):1447-1453
The importance of study of heavy metal distribution in river sediments is a component in understanding the exogenic cycling
as well as in assessing the effect of anthropogenic influences of the elements. In India, the river Subernarekha flows over
Precambrian terrain of Singhbhum craton in the eastern India. The geological succession in this part of India is through (1)
iron ore series, (2) ultrabasic igneous rocks, (3) diorite, (4) granite, (5) newer dolerites, (6) newer tertiary and (7) alluvium.
The first four groups belong to the Archaean era, and the representative is the iron ore series consisting of iron ore, manganese
and chromite which are abundantly present. The primary rock types are schist and quartzite layers. One main tributary, the
Kharkhai flow through granite and schist and quartzite layers. Two important creeks are Gurma and Garra, respectively. The
former after originating in basic igneous area travels through schist quartzite, while the later one originates in granite
area where some functional but old gold mines are located. Freshly deposited sediments of river were collected upstream and
downstream the industrial zone (East Singhbhum district). Samples were collected from four locations and analysed in <63 μm
sediment fraction for heavy metals like Ni, Co and Cr by adsorption stripping voltammetry on hanging mercury drop electrode
and Hg by anodic stripping voltammetry using polished rotating gold disk electrode. Enrichment of these metals over and above
the local natural concentration level (NCL) has been calculated and applied to determine metal-pollution index (MPI) proposed
by Goncalves et al. and also geo-accumulation index (I
geo) by Muller. Based on Muller’s classification, Ni, Cr and Hg have been classified from unpolluted to moderately polluted range
in pre-monsoon period but for metals Ni and Cr, during the post-monsoon period the values have reached moderately polluted
level while Hg has been classified under unpolluted to moderately polluted level except at the monitoring station situated
upstream to Gurma Creek where it was found at unpolluted level. Presence of natural resources of the minerals is primarily
the reason for their detection in river sediments (lithogenic) but some anthropogenic sources are also contributing for their
presence at some sampling stations. Hg is considered to be chalcophilic in nature and is detected wherever known sulphidic
ores of copper or nickel are present. 相似文献
87.
GeoJournal - The study was accomplished to identify the key factors of women empowerment in organic farming. Sankamphaeng, Mae On, Mae Taeng, Doi Saket and San Sai districts of Chiang Mai province... 相似文献
88.
Natural Hazards - Ionospheric effects like scintillations and anomalous variations in total electron content (TEC) monitored with Global Positioning System (GPS) satellites of L1 frequency over... 相似文献
89.
Asru K. Chaudhuri Joydip Mukhopadhyay Sarbani Patranabis Deb S.K. Chanda 《Gondwana Research》1999,2(2):213
The Peninsular India hosts extensive record of Mesoproterozoic, and Neoproterozoic successions in several mobile belts, and cratonic basins. The successions provide excellent opportunities for chronostratigraphic classification, in tune with the chronometric classification adopted by IUGS for inter-regional correlation on a global scale. Major tectono-thermal events at 1000–950 Ma in the mobile belts, correlatable with the Grenville orogeny may be considered as the datum for Meso-Neoproterozoic classification in India. Principles of chronostratigraphic classification, however, can not be applied yet to the cratonic successions of India because of inadequate radiometric data, paucity of biostratigraphic studies, and lack of regionally correlatable stratigraphic or palaeoclimatic datum. The kimberlite magmatism which affected the Peninsular India on a continental scale at about 1100 Ma, holds the key to the identification of Neoproterozoic successions of the cratonic basins. Thus, the stratigraphically confined diamond-bearing conglomerates and/or the tuffs associated with kimberlites, may be considered as the datum to define the base of the Neoproterozoic, fixed at about 1000 Ma. Accordingly, the Rewa, and Bhander Groups in the Vindhyan basin, the Kurnool Group in the Cuddapah basin, the Jagdalpur Formation in the Indravati basin, and the Sullavai Group in the Pranhita-Godavari basin are taken to represent the Neoproterozoic successions in the Peninsular India. The Chattisgarh Group in the central India, the lower part of the Marwar Supergroup in western Rajasthan, the Badami Group in the Kaladgi basin, and the Bhima Group are the other “possible Neoproterozoics” in the Peninsula.The closing phase of the Mesoproterozoic in all these basins are characterised by stable shelf lithologic associations attesting to high crustal stability. The Neoproterozoic basins, by contrast, mark a new phase of rifting, and extension, and the basin fills exhibit signatures of initial instability which evolved with time into a more stable platformal condition. A major episode of sea level rise has been recorded in most of the basins. The riftogenic origin, and evolution of the basins are comparable with the history of Neoproterozoic basins of Australia though there is no unequivocal record of glaciation in the Indian formations. 相似文献
90.
We present CCD photometric observations of the W UMa type contact binary EK Comae Berenices using the 2 m telescope of IUCAA Girawali Observatory, India. The star was classified as a W UMa type binary of subtype-W by Samec et al. (1996). The new V band photometric observations of the star reveal that shape of the light curve has changed significantly from the one observed by Samec et al. (1996). A detailed analysis of the light curve obtained from the high-precision CCD photometric observations of the star indicates that EK Comae Berenices is not a W-type but an A-type totally eclipsing W UMa contact binary. The photometric mass ratio is determined to be 0.349 ± 0.005. A temperature difference of ΔT = 141 ± 10 K between the components and an orbital inclination of i[°] = 89.800 ± 0.075 were obtained for the binary system. Absolute values of masses, radii and luminosities are estimated by means of the standard mass-luminosity relation for zero age main-sequence stars. The star shows O’Connell effect, asymmetries in the light curve shape around the primary and secondary maximum. The observed O’Connell effect is explained by the presence of a hot spot on the primary component. 相似文献