Polarized microwave forward model simulations for tropical storm <Emphasis Type="Italic">Fanoos</Emphasis>     

C. Balaji  M. Deiveegan  S. P. Venkateshan  R. M. Gairola  A. Sarkar  V. K. Agarwal 《Journal of Earth System Science》2009,118(4):331-343

In the present study, forward radiative transfer simulations are carried out for the tropical cyclone Fanoos that hit the coast off south India in December 2005. The in-house radiative transfer package used for this study employs the doubling and adding method to calculate radiances leaving the top of the one dimensional precipitating atmosphere. The particle drop size distribution is assumed to follow a modified gamma distribution in respect of the cloud liquid water and cloud ice water content. For precipitation, the Marshall-Palmer particle size distribution is used. All the hydrometeor particles are assumed to be spherical and Lorentz Mie theory is used to evaluate the interaction parameters like absorption, scattering coefficients and polarized scattering matrix. In order to validate the drop size distributions and interaction parameter calculations, the simulated brightness temperatures are compared with the TMI measured brightness temperatures for all the channels. For carrying out this exercise, vertical hydrometeors retrieved by TMI are used as input. The differences between simulated and measured brightness temperatures are found to be within ±10%. The maximum difference in the brightness temperatures between the present work and the Eddington model which the TRMM algorithm employs is about 4.5K. This may become significant when retrieval of precipitation is attempted by combining the forward model with a suitable retrieval strategy, under tropical conditions.  相似文献   

Harmonics of low-amplitude anisotropic wave trains in cosmic rays     

Rajesh K. Mishra  Rekha Agarwal Mishra 《Planetary and Space Science》2008,56(11):1488-1498

The purpose of this work is to investigate the first three harmonics of low-amplitude anisotropic wave trains (LAEs) of cosmic ray intensity and their association with solar and heliospheric parameters. The significant behaviour of these events is that the amplitude remains low for the first harmonic and high for the second/third harmonics, whereas direction of the anisotropy shift is towards earlier hours for the first harmonic and towards later hours for the second/third harmonic compared to annual average anisotropy. The first two harmonics are found to correlate well with the solar activity cycle during these LAEs. The amplitude and the direction of the first two harmonics do not show any significant association with the polarity change of the Bx/By component of the interplanetary magnetic field during LAEs. However, the third harmonic (amplitude and phase) shows some positive correlation with the Bx and negative correlation with the By component. The occurrence of LAEs is dominant for the positive polarity of Bx and the negative polarity of By. The occurrence of LAEs is dominant during the period of average solar wind velocity but their occurrence during high-speed solar wind streams cannot be overlooked. The frequency of occurrence of these LAEs is more during co-rotating streams.The amplitude of first and second harmonic shows deviations for different values of geomagnetic activity index Ap. However, the amplitude of second harmonic and direction of all the three harmonics do not show any significant association with the Ap-index. The Ap-index consistently remains in the range 14?Kp?31 during these events.The amplitude of first and third harmonic and the direction of first harmonic show deviations for different values of proton density. However, the amplitude of the second harmonic and the direction of the second and third harmonics do not show any significant association with proton density. The occurrence of LAEs is dominant when proton density remains ?20. The cosmic ray intensity during LAEs has good anti-correlation with interplanetary magnetic field strength (B) and its Bx component, whereas it shows a good correlation with its By component. However, it shows significant anti-correlation with sunspot number, the product (R×V) and (R×B).  相似文献   

Possibility of Large Deposits of Gas Hydrates in Deeper Waters of India     

Ashutosh Rastogi  B. Deka  I. L. Budhiraja  Girish C. Agarwal 《Marine Georesources & Geotechnology》1999,17(1):49-63

The available geological and thermodynamic data, essential for the formation and accumulation of gas hydrates, have been integrated and broadly interpreted for the deeper waters of India. The preliminary studies indicate that, in all probability, vast gas hydrate resources exist in the shallow sediments under deep waters. The area of the Bay of Bengal and Arabian Sea, off the coast of India and Andaman Islands, have accumulated thick sediments, over 22 and 10 km, respec tively, during collision of the Indian Plate with the Tibetan Plate. Bottom Simulating Reflectors (BSRs), indicating the likely presence of gas hydrates, have been observed from multichannel and single-channel seismic reflec tion data west of the Andaman Islands and Kerala-Konkan offshore. The Indian continental shelf, slope, and rise areas have, at places, shown the presence of gas-charged sediments and gas seeps through faults. There are commercial oil and gas fields in the shallow waters of both the east and west coasts of India. These are indicative of generation of both biogenic as well as thermogenic gases in the offshore areas of India. For the first time, an attempt has been made to estimate in-place gas hydrate resources under deep waters of India beyond 600 m water depth to the legal continental shelf boundary, and to the Andaman Islands. The gas hydrate resources appear to be vast, and require extensive exploratory efforts for their precise mapping and quantitative assessment.  相似文献   

The Cadmium Zinc Telluride Imager on AstroSat     

V. Bhalerao  D. Bhattacharya  A. Vibhute  P. Pawar  A. R. Rao  M. K. Hingar  Rakesh Khanna  A. P. K. Kutty  J. P. Malkar  M. H. Patil  Y. K. Arora  S. Sinha  P. Priya  Essy Samuel  S. Sreekumar  P. Vinod  N. P. S. Mithun  S. V. Vadawale  N. Vagshette  K. H. Navalgund  K. S. Sarma  R. Pandiyan  S. Seetha  K. Subbarao 《Journal of Astrophysics and Astronomy》2017,38(2):31

The Cadmium Zinc Telluride Imager (CZTI) is a high energy, wide-field imaging instrument on AstroSat. CZTI’s namesake Cadmium Zinc Telluride detectors cover an energy range from 20 keV to \(>200\) keV, with 11% energy resolution at 60 keV. The coded aperture mask attains an angular resolution of 17\(^\prime \) over a 4.6\(^\circ \) \(\times \) 4.6\(^\circ \)  (FWHM) field-of-view. CZTI functions as an open detector above 100 keV, continuously sensitive to GRBs and other transients in about 30% of the sky. The pixellated detectors are sensitive to polarization above \(\sim \)100 keV, with exciting possibilities for polarization studies of transients and bright persistent sources. In this paper, we provide details of the complete CZTI instrument, detectors, coded aperture mask, mechanical and electronic configuration, as well as data and products.  相似文献   

Scanning sky monitor (SSM) onboard AstroSat     

M. C. Ramadevi  S. Seetha  Dipankar Bhattacharya  B. T. Ravishankar  N. Sitaramamurthy  G. Meena  M. Ramakrishna Sharma  Ravi Kulkarni  V. Chandra Babu  Kumar  Brajpal Singh  Anand Jain  Reena Yadav  S. Vaishali  B. N. Ashoka  Anil Agarwal  K. Balaji  G. Nagesh  Manoj Kumar  Dhruti Ranjan Gaan  Prashanth Kulshresta  Pankaj Agarwal  Mathew Sebastian  A. Rajarajan  D. Radhika  Anuj Nandi  V. Girish  Vivek Kumar Agarwal  Ankur Kushwaha  Nirmal Kumar Iyer 《Experimental Astronomy》2017,44(1):11-23

Scanning Sky Monitor (SSM) onboard AstroSat is an Xray sky monitor in the soft X-ray band designed with a large field of view to detect and locate transient X-ray sources and alert the astronomical community about interesting phenomena in the X-ray sky. SSM comprises position sensitive proportional counters with 1D coded mask for imaging. There are three detector units mounted on a platform capable of rotation which helps covering about 50% of the sky in one full rotation. This paper discusses the elaborate details of the instrument and few immediate results from the instrument after launch.  相似文献   

Alternating augite‐plagioclase wedges in basement dolerites of Lockne impact structure,Sweden: A new shock wave‐induced deformation feature          下载免费PDF全文

A. Agarwal  B. Reznik  L. M. Alva‐Valdivia  D. C. Srivastava 《Meteoritics & planetary science》2017,52(3):458-470

This paper reports peculiar alternating augite‐plagioclase wedges in basement dolerites of Lockne impact structure, Sweden. The combined microscopic and spectroscopic studies of the micro/nanoscale wedges reveal that these are deformation‐induced features. First, samples showing wedges, 12 out of 18 studied, are distributed in the impact structure within a radius of up to 10 km from the crater center. Second, the margins between the augite and labradorite wedges are sharp and the {110} prismatic cleavage of augite develops into fractures and thereafter into wedges. The fractures are filled with molten labradorite pushed from the neighboring bulk labradorite grain. Third, compared to the bulk labradorite, the dislocation density and the residual strain in the labradorite wedges are significantly higher. A possible mechanism of genesis of the wedges is proposed. The mechanism explains that passing of the shock waves in the basement dolerite induced (i) formation of microfractures in augite and labradorite; (ii) development of the augite prismatic cleavages into the wedges, which overprint the microfracture in the labradorite wedges; and (iii) thereafter, infilling of microfractures in the augite wedges by labradorite.  相似文献   

On Coronal Loop Heating by Torsional Alfvén Waves     

U. Narain  P. Agarwal  R.K. Sharma  L. Prasad  B.N. Dwivedi 《Solar physics》2001,199(2):307-315

Heating of coronal loops by linear resonant Alfvén waves, excited by the footpoints motions in the photosphere, has been studied. The analysis of single-layer heating is extended to multilayer heating, in semiempirical treatment. Heating and nonthermal velocities in different layers of loops in X-ray bright points, active regions, and large-scale structures are estimated. The average value of velocity is found to be in agreement with the observations.  相似文献   

Study of drainage pattern through aerial data in Naugarh area of Varanasi district, U.P.   总被引：1，自引：0，他引：1  

C S Agarwal 《Journal of the Indian Society of Remote Sensing》1998,26(4):169-175

Drainage pattern of Naugarh Block of district Varanasi has been mapped. The basin characterestics have been analysed is terms of basin morphology and related parameters. The drainage system of the region is composed of 3 perennial rivers with 7 sub-basins. A total of 1223 streams. of 1st to 6th order exist, out of which 761 are of 1st order and 350 of 2nd order which hold sufficient amount of water duing the peak monsoon period Surface water resources could be enhanced in the region by constructing check dams and creating artificial recharge through effective and management.  相似文献   

Origin of high fluoride in groundwater in the North Gujarat-Cambay region, India   总被引：2，自引：0，他引：2  

S. K. Gupta  R. D. Deshpande  Meetu Agarwal  B. R. Raval 《Hydrogeology Journal》2005,13(4):596-605

This paper reports on the origin of high fluoride in a regional alluvial aquifer system under water stress in the North Gujarat-Cambay (NGC) region in western India. This region is severely affected by endemic fluorosis due to ingestion of groundwater containing excessive fluoride. With an objective to understand factors controlling high fluoride concentration in groundwater of this region, 225 groundwater samples have been analysed for various chemical parameters. Samples were collected from different depth zones tapping shallow dug wells, geothermal springs, hand-pumps and tubewells, including free flowing artesian wells up to 450 m depth from the aquifers in the Quaternary alluvial formation covering most of the study area. No relation was found between fluoride concentration and depth of sampled groundwater. However, certain sub-aquifer zones have been identified within the Cambay Basin where groundwater contains relatively high fluoride concentration. In general, areas of high fluoride overlap areas with high electrical conductivity (EC). On the west flank of the Cambay Basin in the low lying belt linking Little Rann of Kachchh-Nalsarovar-Gulf of Khambhat (LRK-NS-GK), high fluoride and EC in shallow aquifers originate from evaporative enrichment. On the east flank of Cambay Basin, some high fluoride pockets are observed which are probably due to preferential dissolution of high fluoride bearing minerals. On this flank high fluoride is also associated with thermal springs. Within the Cambay Basin, alternating belts of low and high fluoride concentrations are ascribed to groundwater recharge during the past wet and arid climatic phases, respectively. This is based on groundwater radiocarbon age contours of ~20 ka overlapping the high fluoride belt.

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Resumen Este artículo reporta sobre el origen de altas concentraciones de flúor en un sistema regional de acuíferos bajo presión hídrica en la región del norte de Gujarat-Cambay (NGC) del occidente de India. Esta región está afectada severamente por fluorosis endémica debido a la ingestión de agua subterránea que contiene exceso de flúor. Se tomaron 225 muestras de agua subterránea las cuales fueron analizadas por varios parámetros químicos con el objetivo de entender los factores que controlan las elevadas concentraciones de flúor en esta región. Las muestras se colectaron a diferentes profundidades en pozos someros, manantiales geotermales, pozos con bombas de mano, y pozos entubados incluyendo pozos artesianos de flujo libre de hasta 450 m de profundidad emplazados en los acuíferos de la formación aluvial Cuaternaria que cubre la mayor parte del área de estudio. No se encontró ninguna relación entre la concentración de flúor y la profundidad de las muestras de agua subterránea. Sin embargo, se identificaron dentro de la cuenca Cambay algunas zonas sub-acuíferas donde el agua subterránea contiene concentraciones relativamente altas de flúor. En general, las áreas con elevada concentración de flúor están sobrepuestas a áreas de alta conductividad eléctrica (CE). Sobre el flanco occidental de la cuenca Cambay, en la faja baja que une Little Rann con Kachchh-Nalsarovar-Golfo de Khamhat (LRK-NS-GK), las altas concentraciones de flúor y altas CE en acuíferos someros se derivan de enriquecimiento por evaporitas. Sobre el flanco oriental de la cuenca Cambay se observaron algunos cuerpos con alta concentración de flúor los cuales se deben probablemente a la disolución preferencial de minerales con alto contenido de flúor. En este flanco el alto contenido de flúor también se asocia con manantiales termales. Dentro de la cuenca Cambay existen fajas alternantes, con concentraciones altas y bajas de flúor, las cuales se atribuyen a recarga de agua subterránea durante las fases climáticas pasadas, húmedas y áridas, respectivamente. Este planteamiento se basa en contornos de edades de ~20 ka de radiocarbono que están sobrepuestos a la faja alta en flúor.

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Résumé Cet article étudie lorigine des teneurs élevées en Fluorure dans un système aquifère alluvial régional, soumis à un stress hydrique dans le Nord Gujarat–région Cambay (NGC) à lOuest de lInde. Cette région est sévèrement affectée par une fluorose endémique, due à lingestion deau souterraine très riche en fluor. Avec pour objectif de comprendre les paramètres contrôlant les fortes teneurs en fluor, 225 échantillons deau souterraine ont été analysés sur différents paramètres. Les échantillons ont été pris à différentes profondeurs : puits de surface, sources géothermiques, pompes à main, forages artésiens jaillissant dont la profondeur avoisine les 450 m dans les formations alluviales quaternaire recouvrant la plus grande partie de la région étudiée. Il ny a pas de relation entre la profondeur et les teneurs en fluorure. Néanmoins, certaines zones sub-aquifères ont été identifiées dans le Basin de Cambay où leau souterraine présentait des concentrations relativement élevées en fluorure. En général les zones de hautes concentrations en fluorure recouvrent les zones à fortes conductivité électrique (abréviation en anglais: EC). Sur le flanc Ouest du bassin de Cambay dans le mince lit reliant Little Ran de Kachchh-Nalsarovar au golfe de Khambhat (LRK-NS-GK), les fortes teneurs en fluorure et les EC dans la nappe phréatique proviennent de lenrichissement par les évaporites. Sur le flanc Est du bassin, des poches de teneurs élevées en fluorures ont été observées, probablement dues à des dissolutions préférentielles de minéraux fluorés. Sur ce flanc des teneurs sont également associées à la présence de sources géothermales. Dans le bassin de Cambay, les alternances de couches lits à fortes teneurs et de lits à faibles teneurs sont expliquées par la recharge durant les périodes climatiques humides et les périodes climatiques plus sèches. Ceci est corroboré par les datations au radiocarbone (environ 20.000 an) au dessus du lit riche en fluorure.

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Use of Remote Sensing and Geospatial Technique for Pre-feasibility Analysis of Rural Water Pipeline Grids     

Priyom Roy  J. Chandramohan  K. Vinod Kumar  Arul Raj  Mobina Shaik  Vinod Bothale  P. G. Diwakar 《Journal of the Indian Society of Remote Sensing》2017,45(4):667-672

The article outlines a procedure of pre-feasibility analysis of planned rural water supply pipeline grids in India. Usually, these type of pre feasibility studies prior to actual implementation, is carried out based on ground surveys and is time consuming. In this work, we use thematic spatial data, such as geomorphology and landuse–landcover along with digital elevation model (DEM) to carry out the pre-feasibility assessment of proposed pipeline grids. DEM generated from CartoSat-1 stereo data has been used to understand the possible topographic hindrances along the planned pipeline route and optimise the same. Further, topographic data also indicates the possible routes of gravity assisted flow. The geomorphology thematic data interpreted from Resourcesat-1 LISS III imagery is used to identify possible geomorphologic hindrances along the pipeline route. Similarly, landuse–landcover information derived from Resourcesat-2 LISS III images, was used to assess the land use/cover impact of the planed pipeline corridor. This has been demonstrated, in the current article using a hypothetical pipeline route. The activity can be carried in a specially designed geo-spatial interface in NRSC/ISRO Bhuvan geoportal. This type of assessment can prove to be time saving and cost effective at a pre-feasibility stage.  相似文献