Evaluation of conditions under which unprotected parts of the human body may freeze in urban air during winter

Relationships between the human skin temperature and a combination of air temperature and wind speed are obtained. These relationships have been used to estimate the climatic conditions leading to the possible freezing of unprotected parts of the face in urban air during winter.The possibility of utilizing relationships governing the heat balance of man, including nomograms and graphs constructed for estimating climatic conditions in urban areas, for isolating zones of different functional importance in the boundaries of a subdivision and of a city, and for estimating the efficiency of various architectural designs in improving the microclimate, are discussed.Originally published inTrudy Main Geophys. Obs. 248, 1969, pp. 74–81. Translated by A. Nurklik, Atmospheric Environment Service, Toronto, Canada.     

An instantaneous 3-D analysis of turbulent flow in the wake of a hemisphere

Instantaneous three-dimensional velocity fields in the wake of a hemisphere located on an open channel bed are obtained by using multi-section flow visualization and a Mass-Consistent model. Instantaneous pictures of the organized structures are taken at a short time interval to investigate their behaviors at high Reynolds number. At high Reynolds number, the large vortex in the hemisphere wake is similar to the hairpin vortex observed at low Reynolds number. However, the long legs of the hairpin in the streamwise direction are not observed. A secondary hairpin vortex has been generated on the upstream side of the large hairpin vortex. Instantaneous spatial distributions of fluctuating velocity, vorticity production, etc. are presented and discussed.     

Geodynamics and seismicity of the Pamir-Himalayas region

Deep seismic sounding studies carried out in 1974–79 allowed an important peculiarity of the deep structure of the Pamir-Himalayas region to be established: the thickness of the Earth's crust is almost twice as large here as on the stable plates (65–75 and 35–37 km, respectively). The absence of any evidence for doubling of crustal thickness provides grounds for rejecting the hypothesis of subduction of the rigid Hindustan plate under the geosynclinal folded constructions of the Punjab syntaxis of the Himalayas. The steep inclination of all major faults, dissecting the Earth's crust and often dislocating the M surface, is also counter to this hypothesis. Several faults reflect the dynamics and conditions of formation of deep layers of the lithosphere. For example, the structural seam of the Indus, which has an almost sheer tilt and which penetrates to subcrustal depths, is a channel along which ophiolite associations of crystalline rocks were squeezed from the mantle. The Fore Himalayan and Major Himalayan faults are the boundaries between different structural facial zones. The band of greatest thickness of crust extends within the zone of greatest thickness of the asthenospheric layer; a deep minimum in the Bouguer anomalies (?550 mGal) corresponds to this zone, as does also a depression on the surface of the geoid.Seismicity of the lithosphere of the Pamir-Himalayas region is caused by geodynamic processes manifested in the higher lithospheric layers by block displacements of the Earth's crust (mostly uplifts), and in the lower parts by shifts of the steeply inclined mantle blocks (the Pamir-Hindukush seismic focal zone).     

Interaction of internal waves and turbulence in the ocean

Within the framework of the semiempirical theory of turbulence for stratified fluids some aspects of the problem of internal wave-turbulence interaction in the upper layer of the ocean are discussed. The conditions of amplification and sustaining of turbulence by internal waves are investigated. Stationary distributions of turbulent energy are found for a stratified fluid with a shear flow produced, for example, by a low-frequency internal wave. The internal wave damping due to both turbulent viscosity and turbulent diffusion in the thermocline is studied. For a two-layer model damping constant is determined as a function of the wave number. The variation of surface turbulence by internal waves is estimated and the role of this process in slick formation is considered.     

Specific structure of convection currents in the system layered intrusion–feeding conduit–parental magma chamber

The structure of convection currents was experimentally studied in the model system layered intrusion–feeding conduit–parental magma chamber. Persistent hydrodynamical and thermophysical interaction between interrelated melts of the parental magma and intrusive body occurs through the feeding conduit. Being associated, they control the structure of convection currents and mechanisms of heat and mass transfer in the intrusive, conduit, and magma chamber. The existence of two convection countercurrents in the conduit has experimentally been established: inner central lifting jet and outer annular downward current along the conduit walls. At the top of the conduit, the downward current has the lowest temperature and appears to be quite in equilibrium with the earlier precipitated crystals. Moving downward along the conduit wall, the annular descending current interacts with the lifting jet and, as a result, becomes hotter and undersaturated relative to the crystals that formed before. Thus, there is no possibility for heterogeneous crystallization to occur on the walls of conduit. The experimentally simulated mechanism of melt interaction in a whole natural system rules out the possibility of formation of a zone of immobile melt with stable steady-state temperature stratification anywhere in the chamber's volume.     

An investigation of macroscopic motions using the Ca+ lines in the prominence of 15 October 1969

The fine structure of the quiescent prominence of 15 October 1969, observed at Abastumani Astrophysical Observatory of the Academy of Sciences of Georgia, U.S.S.R. with the horizontal telescope, is studied.The complex non-gaussian Ca⁺ K line profiles are decomposed into gaussian components and the distribution of the velocity field is plotted.Estimating the direction of the motion by the appearance of the spectral line and by the distribution of the velocity field, we conclude that there is a left-handed screw. Having used the high dispersion spectral data published, we find that prominences showing left-handed screws fall in the northern hemisphere of the Sun and those with right-handed screws in the southern hemisphere.The influence of Coriolis acceleration on quiescent prominences is discussed.     

Theory of superdense matter and degenerate stellar configurations

During the last two decades the theory of degenerate stellar configurations has been developed in works by Ambartsumian and Sahakian, as well as in some other papers. This article is further progress in this direction. Systematic investigations of thermodynamic properties of the ground and metastable states of degenerate plasma have been carried out over the total range of pressures. It was found that in the range of densities 3×10¹⁰???3×10¹⁴ g cm^?3 there exists a pionization effect which plays an important role in the thermodynamics of degenerate plasma. The pion condensate present in nuclear matter promotes the existence of metastable nuclear clusters with the nuclear numberA?10⁶. The equation of state of degenerate stellar matter has been notably revised and, accordingly, the neutron star parameters have been calculated anew. The role of the pion condensate in generating strong magnetic fields observed in the pulsars is discussed.