Studies on Schumann Resonance Phenomena and Some Recent Advancements     

Abhijit Ghosh  Biswas  Debasish  Hazra  Pranab  Guha  Gautam  De  S. S. 《Geomagnetism and Aeronomy》2019,59(8):980-994

Geomagnetism and Aeronomy - Discrete spectra of frequencies at 8, 14, 20, 26, … Hz are generated by electromagnetic emission from lightning sources and can be regarded as excitation of AC...  相似文献   

Neutral fermions as the missing mass matter in galactic halos     

B. Datta  C. Sivaram  S. K. Ghosh 《Astrophysics and Space Science》1985,111(2):413-417

We point out that several independent considerations rule out the hypothesis that the missing mass in galactic halos is dominated by massive neutral fermions such as neutrinos, gravitinos or photinos.  相似文献   

Diffusion of the galactic cosmic rays in the vicinity of the solar system     

L. I. Dorman  A. Ghosh  V. S. Ptuskin 《Astrophysics and Space Science》1985,109(1):87-97

Cosmic-ray propagation in the vicinity of 1 kpc from the Sun is considered. The data on the 10¹²–10¹⁵ eV particle anisotropy, on 10¹² eV electron spectrum, and on temporal cosmic-ray variations are analyzed. The diffusion coefficientD(10¹²–10¹³ eV)=10²⁹–10³⁰ cm²s^–1 inferred from the analysis coincides with its standard value in the large-halo model withh=15 kpc. The total power of cosmic-ray generation, about 3×10⁴⁹ erg per SN in the proton component and about 10⁴⁸ erg per SN in the electron component, typical of the galactic diffusion model is in agreement with the obtained parameters of local sources.  相似文献   

Spin evolution of neutron stars in binary systems     

Pranab Ghosh 《Journal of Astrophysics and Astronomy》1995,16(2):289-305

I review our understanding of the evolution of the spin periods of neutron stars in binary stellar systems, from their birth as fast, spin-powered pulsars, through their middle life as accretion-powered pulsars, upto their recycling or “rebirth” as spin-powered pulsars with relatively low magnetic fields and fast rotation. I discuss how the new-born neutron star is spun down by electromagnetic and “propeller” torques, until accretion of matter from the companion star begins, and the neutron star becomes an accretion-powered X-ray pulsar. Detailed observations of massive radio pulsar binaries like PSR 1259-63 will yield valuable information about this phase of initial spindown. I indicate how the spin of the neutron star then evolves under accretion torques during the subsequent phase as an accretion-powered pulsar. Finally, I describe how the neutron star is spun up to short periods again during the subsequent phase of recycling, with the accompanying reduction in the stellar magnetic field, the origins of which are still not completely understood.  相似文献   

Rapid simultaneous observations of Feii and Balmer emission lines of X Oph     

K. K. Ghosh  K. Jayakumar 《Astrophysics and Space Science》1988,141(2):293-301

Sudden brightening of FeII and Balmer (H and H) lines of X Oph was observed on 28–29 May, 1986. Equivalent width of FeII and H lines increased by a factor of two and that for H line by a factor of four, during the brigtening phase of the star. This brightening phenomena has been explained in the framework of Coronal Radiative Instability.  相似文献   

Pattern of sedimentation during the Late Paleozoic,Gondwanaland glaciation: An example from the Talchir Formation,Satpura Gondwana basin,central India   总被引：2，自引：0，他引：2  

Chandan Chakraborty  Sanjoy Kumar Ghosh 《Journal of Earth System Science》2008,117(4):499-519

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Dynamic Response of Machine Foundation on Layered Soil: Cone Model Versus Experiments   总被引：1，自引：0，他引：1  

P. K. Pradhan  A. Mandal  D. K. Baidya  D. P. Ghosh 《Geotechnical and Geological Engineering》2008,26(4):453-468

This paper presents the experimental validation of analytical solution based on cone model for machine foundation vibration analysis on layered soil. Impedance functions for a rigid massless circular foundation resting on a two layered soil system subjected to vertical harmonic excitation are found using cone model. Linear hysteretic material damping is introduced using correspondence principle. The frequency-amplitude response of a massive foundation is then computed using impedance functions. To verify the solution field experiments are conducted in two different layered soil systems such as gravel layer over in situ soil and gravel layer over concrete slab (rigid base). A total 72 numbers of vertical vibration tests on square model footing were conducted using Lazan type mechanical oscillator, varying the influencing parameters such as depth of top layer, static weight of foundation and dynamic force level. The frequency-amplitude response in general and in particular the resonant frequencies and resonant amplitudes predicted by cone model is compared with the results of experimental investigation, which shows a close agreement. Thus the cone model is reliable in its application to machine foundation vibration on layered soil.  相似文献   

Determination of true velocity dispersion and the dark matter problem in clusters of galaxies     

Amitabha Ghosh 《Astrophysics and Space Science》1995,227(1-2):41-52

According to the convention normally followed the redshifts of the galaxies in a cluster are assumed to be of purely dopplerian origin. The resulting velocity dispersion, when used in the virial theorem, leads to a very large proportion of dark matter to be present in the galaxy clusters. However, the recently proposed model of velocity dependent cosmic drag cause redshifts of photons and it is necessary to develop a procedure to determine the true velocity dispersion from the gross redshift data. A method for this has been presented in the paper. Coma and Perseus clusters have been investigated using this procedure and theM/L ratios for both were found to be approximately of the order of 30, i.e., approximately the order ofM/L ratios for individual galaxies. A study of them -z relation indicates that the galaxies with higher redshifts have fainter magnitudes. Distortion of the redshift plots and the typical elongation of the core regions along the line-of-sight is also explained.  相似文献   

Discovery of <Emphasis Type="Italic">Elephas</Emphasis> cf. <Emphasis Type="Italic">namadicus</Emphasis> from the late Pleistocene strata of Marginal Ganga Plain     

Rupa Ghosh  R. K. Sehgal  Pradeep Srivastava  U. K. Shukla  A. C. Nanda  D. S. Singh 《Journal of the Geological Society of India》2016,88(5):559-568

We describe an elephant skull recovered from a cliff section of Dhasan river of Marginal Ganga Plain. The dental morphology and cranial features of the skull have been compared with the known species of Elephas from the Indian subcontinent. Although it shows very near resemblance to Elephas namadicus, but being an isolated specimen its specific identity cannot be proclaimed with certainty. As such, the specimen is provisionally referred as E. cf. namadicus. The Optically Stimulated Luminescence ages place this find at ~56 ka BP. This is the first chronologically well constrained report of E. cf. namadicus from the Ganga Plain.  相似文献   

Characterizing the 2D shape complexity dynamics of the islands of Sundarbans,Bangladesh: a fractal dimension approach     

Sugata Hazra  Anirban Mukhopadhyay  Abhra Chanda  Parimal Mondal  Tuhin Ghosh  Sandip Mukherjee  Mashfiqus Salehin 《Environmental Earth Sciences》2016,75(20):1367

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