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  • 1
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    In:  Geophys. J. Int., Ottawa, Bundesanstalt für Geowissenschaften und Rohstoffe, vol. 165, no. 1, pp. 373-381, pp. 2371
    Publication Date: 2006
    Keywords: Crustal deformation (cf. Earthquake precursor: deformation or strain) ; Tectonics ; Geodesy ; Iran ; Subduction zone ; GJI ; active ; deformation, ; collision, ; Subduction
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  • 2
    Publication Date: 2015-12-01
    Description: We construct self-similar inflow–outflow solutions for a hot viscous–resistive accretion flow with large-scale magnetic fields that have odd symmetry with respect to the equatorial plane in B and even symmetry in B r and B . Following previous authors, we also assume that the polar velocity v is non-zero. We focus on four parameters: β r 0 , β 0 (the plasma beta parameters associated with magnetic field components at the equatorial plane), the magnetic resistivity 0 and the density index n  = –dln /dln r . The resulting flow solutions are divided into two parts, consisting of an inflow region with a negative radial velocity ( v r 〈 0) and an outflow region with v r  〉 0. Our results show that stronger outflows emerge for smaller β r 0 (≤10 –2 for n  〉 1) and larger values of β 0 , 0 and n .
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 3
    Publication Date: 2015-12-13
    Description: We present the effect of a hydrodynamical wind on the structure and the surface temperature of a vertically self-gravitating magnetized advection-dominated accretion flows (ADAFs) using self-similar solutions. Also a model for an axisymmetric, steady-state, vertically self-gravitating hot accretion flow threaded by a toroidal magnetic field has been formulated. The model is based on α-prescription for turbulence viscosity. It is found that the thickness and radial velocity of the disc are reduced significantly as wind gets stronger. In particular, the solutions indicated that the wind and advection have the same effects on the structure of the disc. We also find that the thin ADAF becomes hotter by including the wind parameter and the self-gravity parameter.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 4
    Publication Date: 2014-03-21
    Description: Dynamics of clumps within a magnetized advection-dominated accretion flow is investigated by solving the collisionless Boltzmann equation and considering the drag force due to the relative velocity between the clumps and the gas. Toroidal component of the magnetic field is assumed to be dominant. Dynamical properties of the hot gaseous component such as the radial and the rotational velocities are affected by the magnetic effects, and so, drag force varies depending on the strength of magnetic field and the velocity dispersion of the clumps is then modified significantly. We show that when magnetic pressure is less than the gas pressure, the root of the averaged radial velocity square of the clumps decreases at the inner parts of the hot flow and increases slightly at its outer edge.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 5
    Publication Date: 2019
    Description: 〈span〉〈div〉Abstract〈/div〉The alveolinid taxa, found in three stratigraphic sections of Eocene shallow-marine successions in the western Alborz (Baghdareh and Gheynarjeh sections) and eastern Iran (Chenesht section) regions, have been studied to determine their systematics and biostratigraphy for the first time. The rich alveolinid assemblages in these regions are correlated with coeval faunas (in shallow benthic zones) of the Tethyan province. The 29 species of alveolinids identified include: 〈span〉Glomalveolina lepidula〈/span〉, 〈span〉Alveolina ellipsoidalis〈/span〉, 〈span〉A〈/span〉. 〈span〉moussoulensis〈/span〉, 〈span〉A〈/span〉. 〈span〉subpyrenaica〈/span〉, 〈span〉A〈/span〉. aff. 〈span〉sakaraensis〈/span〉, 〈span〉A〈/span〉. 〈span〉tumida〈/span〉, 〈span〉A〈/span〉. 〈span〉decipiens〈/span〉, 〈span〉A〈/span〉. 〈span〉pisiformis〈/span〉, 〈span〉A〈/span〉. 〈span〉aragonensis〈/span〉, 〈span〉A〈/span〉. 〈span〉laxa〈/span〉, 〈span〉A〈/span〉. 〈span〉ilerdensis〈/span〉, 〈span〉A〈/span〉. 〈span〉rotundata〈/span〉, 〈span〉A〈/span〉. gr. 〈span〉guidonis〈/span〉, 〈span〉A〈/span〉. 〈span〉elliptica nuttalli〈/span〉, 〈span〉A〈/span〉. 〈span〉citrea〈/span〉, 〈span〉A〈/span〉. cf. 〈span〉citrea〈/span〉, 〈span〉A〈/span〉. cf. 〈span〉rugosa〈/span〉, 〈span〉A〈/span〉. cf. 〈span〉distefanoi〈/span〉, 〈span〉A〈/span〉. cf. 〈span〉montanarii〈/span〉, 〈span〉A〈/span〉. 〈span〉cremae〈/span〉, 〈span〉A〈/span〉. gr. 〈span〉cremae〈/span〉, 〈span〉A〈/span〉. cf. 〈span〉minuta〈/span〉, 〈span〉A〈/span〉. 〈span〉canavarii〈/span〉, 〈span〉A〈/span〉. 〈span〉oblonga〈/span〉, 〈span〉A〈/span〉. 〈span〉decastroi〈/span〉, 〈span〉A〈/span〉. aff. 〈span〉haymanensis〈/span〉, 〈span〉A〈/span〉. 〈span〉bayburtensis〈/span〉, 〈span〉A〈/span〉. 〈span〉frumentiformis〈/span〉, and 〈span〉A〈/span〉. aff. 〈span〉palermitana〈/span〉. On the basis of their distribution ranges, five Tethyan foraminiferal biozones have been recorded from the middle Ilerdian and Cuisian (SBZ7–8 and SBZ10–12) sedimentary successions. The data imply a close affinity between the studied area and other localities in the western Tethyan province.〈/span〉
    Print ISSN: 0096-1191
    Electronic ISSN: 1943-264X
    Topics: Geosciences
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  • 6
    Publication Date: 2017-03-16
    Description: Author(s): Habib Abedi, Matthew Wright, and Amir M. Abbassi We study an anisotropic inflationary scenario in teleparallel gravity. We consider a model where the inflaton is nonminimally coupled both to torsion and a vector field, which can lead to anisotropic inflation. In the weak-coupling limit, our results coincide with the results obtained in the general… [Phys. Rev. D 95, 064020] Published Tue Mar 14, 2017
    Keywords: General relativity, alternative theories of gravity
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 7
    Publication Date: 2013-12-27
    Description: By taking into account the effect of a toroidal magnetic field and its corresponding heating, we determine the thickness of advection-dominated accretion flows. We consider an axisymmetric, rotating, steady viscous–resistive, magnetized accretion flow under an advection-dominated stage. The dominant mechanisms of energy dissipation are assumed to be turbulence viscosity and magnetic diffusivity. We adopt a self-similar assumption in the radial direction to obtain the dynamical quantities, i.e. radial, azimuthal, sound and Alfvén velocities. Our results show that the vertical component of magnetic force acts in the opposite direction to gravity and compresses the disc; thus, compared with the non-magnetic case, in general the disc half-thickness, , is significantly reduced. On the other hand, two parameters that appear due to the action of the magnetic field and reaction of the flow affect the disc thickness. The first one, β 0 , which shows the magnetic field strength at the equatorial plane, decreases . The other one, 0 , is the magnetic resistivity parameter and when it increases also increases.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 8
    Publication Date: 2018-03-06
    Description: Recent observations of the filamentary molecular clouds show that their properties deviate from the isothermal equation of state. Theoretical investigations proposed that the logatropic and the polytropic equations of state with negative indexes can provide a better description for these filamentary structures. Here, we aim to compare the effects of these softer non-isothermal equations of state with their isothermal counterpart on the global gravitational instability of a filamentary molecular cloud. By incorporating the ambipolar diffusion, we use the non-ideal magnetohydrodynamics framework for a filament that is threaded by a uniform axial magnetic field. We perturb the fluid and obtain the dispersion relation both for the logatropic and polytropic equations of state by taking the effects of magnetic field and ambipolar diffusion into account. Our results suggest that, in absence of the magnetic field, a softer equation of state makes the system more prone to gravitational instability. We also observed that a moderate magnetic field is able to enhance the stability of the filament in a way that is sensitive to the equation of state in general. However, when the magnetic field is strong, this effect is suppressed and all the equations of state have almost the same stability properties. Moreover, we find that for all the considered equations of state, the ambipolar diffusion has destabilizing effects on the filament.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 9
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Tetrahedron Letters 28 (1987), S. 1389-1391 
    ISSN: 0040-4039
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 10
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Tetrahedron Letters 30 (1989), S. 7069-7070 
    ISSN: 0040-4039
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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