Estimation of Fried's Parameter From Specklegrams of Solar Features     

Sridharan  R.  Venkatakrishnan  P.  Verma  V.K. 《Solar physics》2002,211(1-2):395-410

A few methods of estimating Fried's parameter (r ₀) from specklegrams of solar features are described. Some of these methods were used to estimate r ₀ for the speckle data obtained from Kodaikanal Observatory (KO), Uttar Pradesh State Observatory (UPSO) and Udaipur Solar Observatory (USO). The average value of r ₀ was found to be 3 cm at USO and UPSO during our observations. At KO, values of r ₀ ranging from 6 to 10 cm were estimated.  相似文献   

Determination of the Maximum Acceptable Toxicant Concentration (MATC) and the safe Concentration for Certain Aquatic Pollutants     

S. R. Verma  I. P. Tonk  R. C. Dalela 《洁净——土壤、空气、水》1981,9(3):247-254

— The 96 h TL₅₀ values, the maximum acceptable toxicant concentration (MATC) and the safe concentrations were determined for various aquatic pollutants, viz. thiotox, chlordane, metasystox, dichlorvos, sevin and carbofuran (pesticides), phenol, pentachlorophenol and dinitrophenol (phenolic compounds), cadmium chloride and copper sulphate (heavy metal), swascofix P₁₄, swanic 6 L and swascol 1P (synthetic detergent) using the larvae (the most sensitive stage of the life cycle) of Cyprinus carpio, a fresh water exotic carp. — The estimated MATC ranged between 0.009 and 400 μg/1 for all the pollutants; — the calculated value of the application factor (AF) ranged between 0.0096 and 0.0978. — The safe concentrations were determined for each pollutant by the lowest value of application factor worked out in the present investigation; — safe concentrations were also worked out by different formulae given by different workers. The values obtained were compared with the safe concentrations value worked out by the authors of the present study.  相似文献   

Resistivity Investigations for Ground Water in Metamorphic Areas Near Dhanbad, India   总被引：3，自引：0，他引：3  

R. K. Verma  M. K. Rao  C. V. Rao 《Ground water》1980,18(1):46-55

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Influence of pH on the Toxicity of Phenol and its Two Derivatives Pentachlorophenol and Dinitrophenol to Some Fresh Water Teleosts     

R. C. Dalela  Saroj Rani  Sarita Rani  S. R. Verma 《洁净——土壤、空气、水》1980,8(6):623-629

— The fish Colisa fasciatus, Saccobranchus fossilis and Notopterus notopterus were exposed to phenol, pentachlorophenol and dinitrophenol at four pH levels, i. e. 4.6 + 0.12, 6.0±0.14, 7.3 ±0.10 and 8.8 ±0.13, to evaluate the effect of pH on the toxicity of these chemicals. — A change in pH from 7.3 ± 0.10 to 6.0 ± 0.14 increased toxicity to a certain degree while a change from 7.3 ± 0.10 to 4.6 ± 0.12 potentiated the toxicity of phenol, pentachlorophenol and dinitrophenol 5.05, 19.30 and 22.33 times, respectively for Notopterus notopterus, 3.59, 4.39 and 4.73 times, tespectively for Colisa fasciatus and 3.04, 4.68 and 5.85 times, respectively for Saccobranchus fossilis. — A change in pH from 7.3 ± 0.10 to 8.8 ± 0.13 has a protective effect on the toxicities.  相似文献   

Seismotectonics of the Hindukush and Baluchistan arc     

R.K. Verma  M. Mukhopadhyay  A.K. Bhanja 《Tectonophysics》1980,66(4):301-322

A seismicity map of that part of the Pakistan-Afghanistan region lying between the latitudes 28° to 38°N and longitudes 66° to 75°E is given using all available data for the period 1890–1970. The earthquakes of magnitude 4.5 and above were considered in the preparation of this map. On the basis of this map, it is observed that the seismicity pattern over the well-known Hindukush region is quite complex. Two prominent, mutually orthogonal, seismicity lineaments, namely the northvestern and the north-eastern trends, characterize the Hindukush area. The northwestern trend appears to extend from the Main Boundary Fault of the Kashmir Himalaya on the southeast to the plains of the Amu Darya in Uzbekistan on the northwest beyond the Hindukush. The Sulaiman and Kirthar ranges of Pakistan are well-defined zones of intermontane seismicity exhibiting north-south alignment.Thirty-two new focal-mechanism solutions for the above-mentioned region have been determined. These, together with the results obtained by earlier workers, suggest the pre-dominance of strike-slip faulting in the area. The Hazara Mountains, the Sulaiman wrench zone and the Kirthar wrench zone, as well as the supposed extension of the Murray ridge up to the Karachi coast, appear to be mostly undergoing strike-slip movements.In the Hindukush region, thrust and strike-slip faulting are found to be equally prevalent. Almost all the thrust-type mechanisms belonging to the Hindukush area have both the nodal planes in the NW-SE direction for shallow as well as intermediate depth earthquakes. The dip of P-axes for the events indicating thrust type mechanisms rarely exceeds 35°. The direction of the seismic slip vector obtained through thrust type solutions is always directed towards the northeast. The epicentral pattern together with these results suggest a deep-seated fault zone paralleling the northwesterly seismic zone underneath the Hindukush. This NW-lineament has a preference for thrust faulting, and it appears to extend from the vicinity of the Main Boundary Fault of the Kashmir Himalaya on the southeast of Uzbekistan on the northwest through Hindukush. Almost orthogonal to this NW-seismic zone, there is a NE-seismic lineament in which there is a preference for strike-slip faulting.The above results are discussed from the point of view of convergence of the Indian and Eurasian plates in the light of plate tectonics theory.  相似文献   

Paleomagnetic study of a vertical sequence of traps from Mount Pavagarh,Gujrat, India     

R.K. Verma  G.S. Mital 《Physics of the Earth and Planetary Interiors》1974,8(1):63-74

The paleomagnetism of 22 flows which range in composition from olivine basalts to rhyolite and in elevation from 450 ft. to 2680 ft., from Mount Pavagarh, situated in Gujrat, India, has been studied. The igneous activity represented by these flows belongs to the Deccan Trap Plateau Basalt Series. Sixteen flows ranging in elevation from 900 to 2680 ft. showed normal magnetization with upward inclination, consistent with the position of India in the southern hemisphere during the period of their eruption. Four flows from elevation 450 ft. to 730 ft. showed intermediate as well as discordant directions. The paleomagnetic results obtained from these flows have been correlated with those of Deccan traps from other areas. The amount of paleosecular variation represented by these flows has been estimated and compared with that from similar vertical sequences of traps studied from other areas. It has been found that the magnitude of paleosecular variation varied during the period of Deccan trap activity. An estimate of continental drift has been made from mean pole position of the several vertical sequences of traps. This indicates that a drift of the Indian landmass of the order of 24° took place during the entire period represented by the Deccan trap activity. The results of paleomagnetic studies of other sedimentary and igneous formations of Cretaceous age are reviewed in the light of recent results on Deccan traps.  相似文献   

From the Journal Editor     

Kamlesh Lulla 《国际地球制图》2013,28(2)

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Magnetohydrodynamic effects on radiation-driven shock waves     

B. G. Verma  D. D. Dube 《Astrophysics and Space Science》1986,124(1):43-51

A similarity solution for the flow variables behind a radiation-driven magnetohydrodynamic shock wave has been obtained. Owing to absorption of radiation incident on the shock layer, it is assumed that the total energy contained behind the shock surface is increasing. The ambient medium in which shock wave moves is non-uniform and it is optically thin so that there is no interaction with the incident radiation. A comparison has been made between the results with and without the magnetic field when the density and azimuthal magnetic field distributions are variable.While this paper was in press, Professor Verma passed away on 4 April 1985, without being able to read its proofs.  相似文献   

Relationship of great soft X-ray flares with other solar activity phenomena     

V. K. Verma 《Astrophysics and Space Science》2011,334(1):83-102

We present study of relationship of GSXR flares with Hα flares, hard X-ray (HXR) bursts, microwave (MW) bursts at 15.4 GHz, type II/IV radio bursts, coronal mass ejections (CMEs), protons flares (>10 MeV) and ground level enhancement (GLE) events we find that about 85.7%, 93%, 97%, 69%, 60%, 11.1%, 79%, 46%, and 23%% GSXR flares are related/associated with observed Hα flares, HXR bursts, MW bursts at 15.4 GHz, type II radio bursts, type IV radio bursts, GLE events, CMEs, halo CMEs, and proton flares (>10 MeV), respectively. In the paper we have studied the onset time delay of GSXR flares with Hα flares, HXR, and MW bursts which shows the during majority GSXR flares SXR emissions start before the Hα, HXR and MW emissions, respectively while during 15–20% of GSXR flares the SXR emissions start after the onset of Hα, HXT and MW emissions, respectively indicating two types of solar flares. The, onset time interval between SXR emissions and type II radio bursts, type IV radio bursts, GLE events CMEs, halo CMEs, and protons flares are 1–15 min, 1–20 min, 21–30 min, 21–40 min, 21–40 min, and 1–4 hrs, respectively. Following the majority results we are of the view that the present investigations support solar flares models which suggest flare triggering first in the corona and then move to chromospheres/ photosphere to starts emissions in other wavelengths. The result of the present work is largely consistent with “big flare syndrome” proposed by Kahler (1982).  相似文献   

Dark energy as a manifestation of the non-constant cosmological constant     

Murli Manohar Verma 《Astrophysics and Space Science》2010,330(1):101-105

We propose a time-varying cosmological constant with a fixed equation of state, which evolves mainly through its interaction with the background during most of the long history of the universe. However, such an interaction does not exist in the very early- and the late-time universe and this produces the acceleration during these eras when it becomes very nearly a constant. It is found that after the initial inflationary phase, the cosmological constant, which we call the lambda parameter, rolls down from a large constant value to another but very small constant value and further dominates the present epoch showing up in the form of dark energy, driving the acceleration.  相似文献