Study of aerodynamics of stream flow in server rooms using numerical modeling

This paper analyzes various schemes of air exchange in server rooms. Top-down and down-top vertical cooling schemes for small server rooms using local AC systems were analyzed. Numerical models were developed for the study of heat and mass transfer and server aerodynamics, which make it possible to evaluate the cooling efficiency of electronic equipment when placed in an arbitrary configuration. To study the thermal and velocity fields, numerical simulation of the stream flow processes was performed using the FlowVision software. This paper shows the advantage of the selected air-conditioning scheme compared to the existing ventilation system. Modeling results may be used for designing small server rooms. © 2019 IOP Publishing Ltd. All rights reserved

A simultaneous pancreas-kidney transplantation for type 1 diabetes mellitus after a long-term of receiving hemodialysis renal replacement therapy. Clinical сase

At the present time, a simultaneous pancreas-kidney transplantation (SPKT) is an effective method of treatment for patients on renal replacement therapy by hemodialysis program in the outcome of the terminal stage of diabetic nephropathy. This method of treatment solves several problems: it reduces the severity of intoxication syndrome, contributes to the achievement of euglycemia in most cases, which certainly allows to slow the progression of micro- and macrovascular complications of diabetes. Despite of positive effect of euglycaemia and kidney function normalization, the accumulated metabolic memory legacy of long-term uncompensated diabetes mellitus is realized, which makes a posttransplantational rehabilitation of patients difficult. A duration of hemodialysis therapy is known as a cardiovascular events risk factor, which affects the surgery result and favorable posttransplant period. More often after successful SPKT microvascular diabetic complications are stabilized, but macrovascular diabetic complications, diabetic neuroosteoarthropathy and mineral and bone disease are progressed. That’s why is necessary to perform regular examination after SPKT by a team of specialists, including nephrologist, endocrinologist, cardiologist, ophthalmologist with correction of ongoing therapy. Therefore both the preparation of  the patient for transplantation with the earliest possible placement on the waiting list and the post-transplant rehabilitation afterwards are extremely important

The Tidal Potential of a Homogeneous Torus with an Elliptical Section of the Sleeve

In this paper the problem of the tidal potential of a homogeneous gravitating torus with an elliptical cross-section sleeve is solved. In particular, the potentials in analytical form in the vicinity of the center of the torus and its external region are found. This torus can serve as a gravitational model of the Kuiper belt

Equilibrium Figures inside the Dark-Matter Ring and the Shapes of Elliptical Galaxies

We solve the general problem of the theory of equilibrium figures and analyze two classes of liquid rotating gravitating figures residing inside a gravitating ring or torus. These figures form families of sequences of generalized oblate spheroids and triaxial ellipsoids, which at the lower limit of the tidal parameter α = 0 have the form of the Maclaurin spheroids and the Jacobi ellipsoids. In intermediate cases 0 < α ≤ αmax each new sequence of axisymmetric equilibrium figures has two non-rotating boundary spheroids. At the upper limit αmax/(πGρ) = 0.1867 the sequence degenerates into a single non-rotating spheroid with the eccentricity ecr ≈ 0.96 corresponding to the flattening limit of elliptical galaxies (E7). We also perform a detailed study of the sequences of generalized triaxial ellipsoids and find bifurcation points of triaxial ellipsoids in the sequences of generalized spheroids. We use this method to explain the shapes of E-galaxies. According to observations, very slowly rotating oblate E-type galaxies are known that have the shapes, which, because of instability, cannot be supported by velocity dispersion anisotropy exclusively. The hypothesis of a massive dark-matter outer ring requires no extreme anisotropy of pressure; it not only explains the shape of these elliptical galaxies, but also sheds new light on the riddle of the ellipticity limit (E7) of elliptical galaxies