Some thougths on the evolution of Himalaya and the Northern limit of the Indian Shield

Based on the sedimentological studies and the distribution of fossil-bearing horizons in the Himalaya a new model for the evolution of Himalaya is visualized. It is proposed that the Lesser and Central Himalaya constitute an integral part of the Peninsular Indian shield. The unfossiliferous orthoquartzite-shale-carbonate sequences of Lesser and Central Himalaya represent Precambrian sediments, deposited in a shallow tidal sea. Within the Lesser Himalaya there are thin detached marine fossiliferous horizons of three ages, viz. Carboniferous-Permian, Jurassic-Cretaceous and Eocene, located in a narrow E-W running zone (Dogadda-Subathu Zone), representing deposits of three transgressions in this zone.This zone is analogous to the Narbada Valley zone of the Peninsular India, where rocks of Permian, Cretaceous and Eocene ages are present. This model properly explains the unfossiliferous nature of the Lesser Himalayan sediments and demands the northern limit of Indian Plate north of Himalaya.

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Zusammenfassung Aufgrand sedimentologischer Untersuchungen und der Verteilung fossilführender Schichten im Himalaya wird ein neues Modell der Himalayaentwicklung dargestellt. Es wird angenommen, daß der Außen- und Zentralhimalaya fester Bestandteil des indischen Schildes waren. Die fossilleeren Abfolgen von Orthoquarziten, Tonen und Kalken des Außen- und Zentralhimalaya bestehen aus präkambrischen Sedimenten, die ehemals in einem Flachmeer unter Gezeiteneinfluß abgelagert wurden. Im Bereich des Außenhimalaya finden sich geringmächtige Einschaltungen mit mariner Fauna, die dem Permokarbon, Jura/Kreide und Eozän zuzuordnen sind. Sie liegen innerhalb einer schmalen E/W-verlaufenden Zone (Dogadda-Subathu Zone) und entsprechen 3 Transgressionen in diesem Gebiet.Diese Zone ist dem Narbada Valley-Bereich der indischen Halbinsel vergleichbar, wo ebenfalls Ablagerungen aus Perm, Kreide und Eozän angetroffen werden.Durch dieses Modell läßt sich die Art der fossilleeren Sedimente des Außenhimalaya erklären. Es führt zu der Annahme, daß die Nordgrenze der indischen Platte nördlich des Himalaya zu suchen ist.

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Résumé Un nouveau modèle de l'évolution de l'Himalaya est présenté, basé sur des études sédimentologiques et sur la répartition des horizons fossilifères, suivant lequel l'Himalaya Central et Externe ferait intégralement partie du boncliez péninsulaire Indien.Les séquences non fossilifères d'orthoquartzites-schistes-carbonates de l'Himalaya Central et Externe représentent des sédiments précambriens déposés dans un environnement marin peu profond soumis aux marées. Dans la région de l'Himalaya Externe, on observe de minces intercalations fossiliferes marines correspondant à trois phases de transgression, au Permo-Carbonifére, au Jurassique-Crétacé et à l'Eocène. Ces horizons sont localisés dans une zone étroite, de direction E-W, la zone de Dogadda-Subathu.Cette zone est comparable à la Valleé de Narbada en Inde péninsulaire, qui comporte également des dépôts permiens, crétacés et éocènes. Le modèle propose permet d'expliquer la nature non fossilifère de la plupart des sédiments de l'Himalaya Externe et conduit á rechercher la limite Nord de la plaque indienne au Nord de l'Himalaya.

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Application of magnetic susceptibility anisotropy technique to the study of geological structures in the Armorican massif, France

Magnetic susceptibility anisotropy analyses have been carried out on 300 samples of rock from various metamorphosed regions of Normandy and Brittany, within the northern half of the Armorican massif, to test the ability of the magnetic fabric method (in a relatively complex region where structures have been well charted) to delineate regional structures. The two major structural directions to emerge from the study were a ENE—WSW striking magnetic foliation plane, conforming to a Variscan direction of the Bocaine syncline in the Granville region of Normandy and a ESE—WNW striking magnetic foliation plane conforming to the Armorican direction in the Chateaulin syncline region of Brittany. The magnetic fabric of sites elsewhere confirmed localised structures and minor synclinal structures.

The major advantages of the technique of studying magnetic fabric over petrofabric are the speed at which magnetic fabric can be measured (2 minutes per sample compared with up to 24 h using X-ray goniometry techniques) and the sensitivity of the magnetic fabric to very slight stresses.     

The socioeconomic impacts of nuclear generating stations: An analysis of the Rancho Seco and peach bottom facilities

This paper presents the results of a comparative analysis of the socioeconomic impacts of the construction and operation of two nuclear generating stations. Although the construction of nuclear power plants is typically a multiyear process utilizing large numbers of workers and requiring large expenditures for equipment and materials, the socioeconomic changes in the areas in which the plants are located were small and temporary. The extent and size of the changes were found to be related to the size of the work force residing in the local area, the magnitude of local utility and contractor purchases, the amount of tax payments resulting from the plant, and the level of involvement of area groups over plant-related issues.     

Source parameters of the Burma-India border earthquake of July 29, 1970, from body waves

The source parameters are determined for the Burma-India border earthquake of July 29, 1970, from body-wave spectra. We obtain seismic moment [ , ] · 10²⁶ dyne cm, source dimension [ ] km, radiated energy [ , −E_R (S) = 1.35] · 10²⁰ ergs and the stress drop = 11 bars.     

Geochemical background in soils: a linear process domain? An example from Istria (Croatia)

Definition of geochemical background in exploration and environmental geochemistry has always been regarded as contingent upon scale and investigated locality but mostly under assumption that hosts of processes that produce the data more or less conform individually to Gaussian law of “central tendencies”. Recently, understanding of pedogenesis as synergetic process being characterized by non-linear dynamics renders thermodynamic approach directly applicable in assessment of geochemical thresholds, with concepts of linearity and normality set alongside in solving the problems of soil geochemistry. Seen from this perspective the work is an attempt to relate conceptual fundamentals of non-linear dynamical theory to basic statistical methods in order to elucidate the nature and origins of element subpopulations hidden in the original geochemical data from the soils of Istrian Peninsula (western Croatia). To this purpose the two major groups of soils were selected for analysis depending on the type of bedrock as one of the main soil-forming factors. Geochemical data were subjected to the trimming procedure by which the outliers were removed from the total data collective and attributed to non-linear causes precluding simple cause-and-effect relationships as the sine qua non of Gaussian distribution. Geochemical background is then defined as the normal range of data of the remaining (trimmed) dataset indicating the “thermodynamic branch” of the specific soil processes as opposed to outliers being described as dissipative structures.     

An Improvized Core-Drilling Technique and a New Device for Osteohistology of Fossil Bones: Implementation on a Jurassic Sauropod Dinosaur from India

An improvized version of the conventional core drilling technique, based on a new device is introduced in the current work for extracting cores from fossil bones to understand their microanatomy. A powerful, low-speed electric drill with an autolubrication facility is used as the new device, and the bone specimen is placed on a permanently fixed platform beneath the drill bit. It avoids the vibration-induced wobbling of the conventional handheld drill machine and helps in precision sampling. Long drill bits of the new device result in extraction of long cores, reduce premature breakages of cores, and recovery of the entire bone microstructure for high resolution deduction of palaeobiological information. As this version of drilling technique is less destructive, it has better sampling coverage, where fossil bones can be restored to their original shapes and preserved with almost no loss in gross morphology. This is first time such a device for extraction of fossil drill cores has been installed. After test run on dummy samples, the new device has been successfully implemented for extraction of eleven cores from various long bones of the early Jurassic sauropod dinosaur Barapasaurus tagorei. The fossil bones are restored to their pre-coring shapes, the detail protocols of which are discussed here for the first time.     

Template-based classification of SDSS-<Emphasis Type="BoldItalic">GALEX</Emphasis> point sources

We have classified a sample of 37,492 objects from SDSS into QSOs, galaxies and stars using photometric data over five wave bands (u, g, r, i and z) and UV GALEX data over two wave bands (near-UV and far-UV) based on a template fitting method. The advantage of this method of classification is that it does not require any spectroscopic data and hence the objects for which spectroscopic data is not available can also be studied using this technique. In this study, we have found that our method is consistent by spectroscopic methods given that their UV information is available. Our study shows that the UV colours are especially important for separating quasars and stars, as well as spiral and starburst galaxies. Thus it is evident that the UV bands play a crucial role in the classification and characterization of astronomical objects that emit over a wide range of wavelengths, but especially for those that are bright at UV. We have achieved the efficiency of 89% for the QSOs, 63% for the galaxies and 84% for the stars. This classification is also found to be in agreement with the emission line diagnostic diagrams.     

Determination of 3D Trajectories of Knots in Solar Prominences Using MSDP Data

In this paper we present a new method of restoration of the true three-dimensional (3D) trajectories of prominence knots using ground-based observations taken with a single telescope that is equipped with a Multi-Channel Subtractive Double Pass imaging spectrograph. Our method allows us to evaluate the true 3D trajectories of the prominence knots without any assumptions concerning the shape of the trajectories or the dynamics of the motion. The reconstructed trajectories of several knots observed in three prominences are presented.     

Some anisotropic spatially-homogeneous cosmological models with electromagnetic field

Considering Bianchi type-I metric, cosmological models of a perfect fluid with an electromagnetic field have been obtained, using a supplementary condition between the metric potentials. The four-current is either zero or space-like. The model has expanding and shearing but non-rotating fluid flow which is also geodetic. The requirement of positive conductivity imposes an additional restriction on the model. Various physical and mathematical properties of the model have been discussed.