238 research outputs found
Выбор оптимальных методов технологии и контроля при проведении гидроразрыва пласта ( на примере Самотлорского месторождения)
Представлен анализ текущего состояния разработки месторождения и основных методов повышения эффективности разработки. Произведен выбор оптимальных технологий с
учетом их фильтрационноемкостных свойств. Показано влияние синтетического
полимера на свойства проводимости трещин поле стадий ГРП.The analysis of the current state of development of the field and the main methods to improve development efficiency is presented. The selection of optimal technologies with
taking into account their filtration-capacitive properties. The effect of synthetic
polymer on the conductivity properties of fractures in the field of hydraulic fracturing stages
Замена электродвигателя ПЭН турбоприводом на Кемеровской ТЭЦ
В данной работе рассматривается возможность замены электродвигателя ПЭН турбоприводом на Кемеровской ТЭЦ, с установкой турбопривода на существующий фундамент. Целью работы является оценка возможности увеличения отпуска электроэнергии от станции в результате уменьшения затрат на собственные нужды и повышение маневренности ТЭЦ.In this paper we consider the possibility of replacing the turbine drive motor PEN to Kemerovo CHP , with the installation of turbine drive on the existing foundation. The aim is to assess the possibility of increasing the supply of electric power from the plant by reducing the costs of their own needs and improving maneuverability CHP
Asteroseismology with the WIRE satellite. I. Combining Ground- and Space-based Photometry of the Delta Scuti Star Epsilon Cephei
We have analysed ground-based multi-colour Stromgren photometry and
single-filter photometry from the star tracker on the WIRE satellite of the
delta scuti star Epsilon Cephei. The ground-based data set consists of 16
nights of data collected over 164 days, while the satellite data are nearly
continuous coverage of the star during 14 days. The spectral window and noise
level of the satellite data are superior to the ground-based data and this data
set is used to locate the frequencies. However, we can use the ground-based
data to improve the accuracy of the frequencies due to the much longer time
baseline. We detect 26 oscillation frequencies in the WIRE data set, but only
some of these can be seen clearly in the ground-based data. We have used the
multi-colour ground-based photometry to determine amplitude and phase
differences in the Stromgren b-y colour and the y filter in an attempt to
identify the radial degree of the oscillation frequencies. We conclude that the
accuracies of the amplitudes and phases are not sufficient to constrain
theoretical models of Epsilon Cephei. We find no evidence for rotational
splitting or the large separation among the frequencies detected in the WIRE
data set. To be able to identify oscillation frequencies in delta scuti stars
with the method we have applied, it is crucial to obtain more complete coverage
from multi-site campaigns with a long time baseline and in multiple filters.
This is important when planning photometric and spectroscopic ground-based
support for future satellite missions like COROT and KEPLER.Comment: 13 pages, 12 figures, 4 tables. Fig. 4 reduced in quality. Accepted
by A&
Abundance analysis of targets for the COROT / MONS asteroseimology missions I. Semi-automatic abundance analysis of the gamma Dor star HD 49434
One of the goals of the ground-based support program for the COROT and
MONS/Roemer satellite missions is to select and characterise suitable target
stars for the part of the missions dedicated to asteroseismology. While the
global atmospheric parameters may be determined with good accuracy from the
Stromgren indices, careful abundance analysis must be made for the proposed
main targets. This is a time consuming process considering the long list of
primary and secondary targets. We have therefore developed new software called
VWA for this task. The VWA automatically selects the least blended lines from
the atomic line database VALD, and consequently adjusts the abundance in order
to find the best match between the calculated and observed spectra. The
variability of HD 49434 was discovered as part of COROT ground-based support
observations. Here we present a detailed abundance analysis of HD 49434 using
VWA. For most elements we find abundances somewhat below the Solar values, in
particular we find [Fe/H] = -0.13(14). We also present the results from the
study of the variability that is seen in spectroscopic and photometric time
series observations. From the characteristics of the variation seen in
photometry and in the line profiles we propose that HD 49434 is a variable star
of the gamma Doradus type.Comment: 10 pages, 6 figure
Effects of parental acclimation and energy limitation in response to high CO2 exposure in Atlantic cod
Ocean acidification (OA), the dissolution of excess anthropogenic carbon dioxide in ocean waters, is a potential stressor to many marine fish species. Whether species have the potential to acclimate and adapt to changes in the seawater carbonate chemistry is still largely unanswered. Simulation experiments across several generations are challenging for large commercially exploited species because of their long generation times. For Atlantic cod (Gadus morhua), we present first data on the effects of parental acclimation to elevated aquatic CO2 on larval survival, a fundamental parameter determining population recruitment. The parental generation in this study was exposed to either ambient or elevated aquatic CO2 levels simulating end-of-century OA levels (~1100 µatm CO2) for six weeks prior to spawning. Upon fully reciprocal exposure of the F1 generation, we quantified larval survival, combined with two larval feeding regimes in order to investigate the potential effect of energy limitation. We found a significant reduction in larval survival at elevated CO2 that was partly compensated by parental acclimation to the same CO2 exposure. Such compensation was only observed in the treatment with high food availability. This complex 3-way interaction indicates that surplus metabolic resources need to be available to allow a transgenerational alleviation response to ocean acidification
Ten years of antibiotic consumption in ambulatory care: Trends in prescribing practice and antibiotic resistance in Austria
GAUDI: a preparatory archive for the COROT mission
The GAUDI database (Ground-based Asteroseismology Uniform Database Interface,
http://sdc.laeff.esa.es/gaudi/) is a preparatory archive for the COROT
(COnvection, ROtation and planetary Transits,
http://www.astrsp-mrs.fr/projets/corot/) mission developed at LAEFF (Laboratory
for Space Astrophysics and Theoretical Physics, http://www.laeff.esa.es). Its
intention is to make the ground-based observations obtained in the preparation
of the asteroseismology programme available in a simple and efficient way. It
contains spectroscopic and photometric data together with inferred physical
parameters for more than 1500 objects gathered since January 1998 in 6 years of
observational campaigns. In this paper, the main functionalities and
characteristics of the system are described. The observations have been
collected at ESO-La Silla, Telescopio Nazionale Galileo, Observatoire de
Haute-Provence, South African Astronomical Observatory, Tautenberg Observatory
and Sierra Nevada Observatory.Comment: 12 pages, 3 figures (quality degraded). Accepted for publication in
The Astronomical Journa
Documentation on key drivers and physiological tolerance limits for resident and invasive species:Report: BIO-C3 Deliverable, D1.2
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