1,965 research outputs found
Editorial: Controversies and solutions in environmental sciences: Addressing toxicity of sediments and soils
This is the author's accepted manuscript. The final published article is available from the link below. Copyright @ 2007 Ecomed Publishers
Effect of arm movement on balance performance in children: role of expertise in gymnastics
OBJECTIVE: Studies have shown that balance performance is better in gymnasts compared to age-/sex-matched controls and further studies revealed superior performance when arms were free to move during assessment of balance. However, it is unknown whether free arm movement during balance testing differentially affects balance performance with respect to sports expertise (i.e., gymnasts areΒ less affected than age-/sex-matched controls). Therefore, we investigated the effect of arm movement on balance performance in young female gymnasts compared to age-/sex-matched controls while performing balance tasks with various difficulty levels. RESULTS: In both samples, balance performance (except for the timed one-legged stance) was significantly better during free compared to restricted arm movement conditions and this was especially observed in the highest task difficulty condition of the 3-m beam walking backward test. These findings revealed that balance performance is positively affected by free arm movements, but this does not seem to be additionally influenced by the achieved expertise level in young gymnasts
A BeppoSAX observation of the super-soft source CAL87
We report on a BeppoSAX Concentrator Spectrometer observation of the
super-soft source (SSS) CAL87. The X-ray emission in SSS is believed to arise
from nuclear burning of accreted material on the surface of a white dwarf (WD).
An absorbed blackbody spectral model gives a chi^2_v of 1.18 and a temperature
of 42 +/- ^13 _11 eV. However, the derived luminosity and radius are greater
than the Eddington limit and radius of a WD. Including an O viii edge at 0.871
keV gives a significantly better fit (at > 95% confidence) and results in more
realistic values of the source luminosity and radius. We also fit WD atmosphere
models to the CAL87 spectrum. These also give reasonable bolometric
luminosities and radii in the ranges 2.7-4.8 10^{36} erg/s and 8-20 10^7 cm,
respectively. These results support the view that the X-ray emission from CAL87
results from nuclear burning in the atmosphere of a WD.Comment: 4 pages. Accepted for publication in A&A (Letters
Murine cytomegalovirus inhibits interferon Ξ³-induced antigen presentation to CD4 T cells by macrophages via regulation of expression of major histocompatibility complex class II-associated genes
CD4 T cells and interferon γ (IFN-γ) are required for clearance of murine cytomegalovirus (MCMV) infection from the salivary gland in a process taking weeks to months. To explain the inefficiency of salivary gland clearance we hypothesized that MCMV interferes with IFN-γ induced antigen presentation to CD4 T cells. MCMV infection inhibited IFN-γ-induced presentation of major histocompatibility complex (MHC) class II associated peptide antigen by differentiated bone marrow macrophages (BMMΦs) to a T cell hybridoma via impairment of MHC class II cell surface expression. This effect was independent of IFN-α/β induction by MCMV infection, and required direct infection of the BMMΦs with live virus. Inhibition of MHC class II cell surface expression was associated with a six- to eighffold reduction in IFN-γ induced IAb mRNA levels, and comparable decreases in IFN-γ induced expression of invariant chain (Ii), H-2Ma, and H-2Mb mRNAs. Steady state levels of several constitutive host mRNAs, including β-actin, cyclophilin, and CD45 were not significantly decreased by MCMV infection, ruling out a general effect of MCMV infection on mRNA levels. MCMV effects were specific to certain MHC genes since IFN-γ-induced transporter associated with antigen presentation (TAP)2 mRNA levels were minimally altered in infected cells. Analysis of early upstream events in the IFN-γ signaling pathway revealed that MCMV did not affect activation and nuclear translocation of STAT1α, and had minor effects on the early induction of IRF-1 mRNA and protein. We conclude that MCMV infection interferes with IFN-γ-mediated induction of specific MHC genes and the Ii at a stage subsequent to STAT1α activation and nuclear translocation. This impairs antigen presentation to CD4 T cells, and may contribute to the capacity of MCMV to spread and persist within the infected host
Study of led lamp power supply
Π Π΄Π°Π½Π½ΠΎΠΉ ΡΡΠ°ΡΡΠ΅ ΠΈΡΡΠ»Π΅Π΄ΡΠ΅ΡΡΡ ΠΈΡΡΠΎΡΠ½ΠΈΠΊ ΠΏΠΈΡΠ°Π½ΠΈΡ ΡΠ²Π΅ΡΠΎΠ΄ΠΈΠΎΠ΄Π½ΠΎΠ³ΠΎ ΡΠ²Π΅ΡΠΈΠ»ΡΠ½ΠΈΠΊΠ° Ρ Π²ΡΡΠΎΠΊΠΈΠΌΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠΎΠΌ ΠΌΠΎΡΠ½ΠΎΡΡΠΈ. ΠΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½Π° ΠΌΠΈΠΊΡΠΎΡΡ
Π΅ΠΌΠ° ΠΊΠΎΡΡΠ΅ΠΊΡΠΎΡΠ° ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠ° ΠΌΠΎΡΠ½ΠΎΡΡΠΈ ΠΊΠΎΠΌΠΏΠ°Π½ΠΈΠΈ STMicroelectronics L6561 Π² ΠΎΠ±ΡΠ°ΡΠ½ΠΎΡ
ΠΎΠ΄ΠΎΠ²ΠΎΠΉ ΡΠΎΠΏΠΎΠ»ΠΎΠ³ΠΈΠΈ. Π‘ ΠΏΠΎΠΌΠΎΡΡΡ ΡΡΠΎΠΉ ΠΌΠΈΠΊΡΠΎΡΡ
Π΅ΠΌΡ ΡΠΏΡΠΎΡΠ°Π΅ΡΡΡ ΠΏΠΎΡΡΡΠΎΠ΅Π½ΠΈΠ΅ ΠΈΡΡΠΎΡΠ½ΠΈΠΊΠ° ΠΏΠΈΡΠ°Π½ΠΈΡ, ΡΡΠΈΡΡΠ²Π°Ρ ΡΡΠ°Π½Π΄Π°ΡΡΡ ΡΠ½Π΅ΡΠ³ΠΎΡΠ±Π΅ΡΠ΅ΠΆΠ΅Π½ΠΈΡ ΠΈ ΡΡΠ΅Π±ΠΎΠ²Π°Π½ΠΈΡ ΠΊ ΡΡΠΎΠ²Π½Ρ Π²Π½ΠΎΡΠΈΠΌΡΡ
Π² ΠΏΠΈΡΠ°ΡΡΡΡ ΡΠ΅ΡΡ ΠΈΡΠΊΠ°ΠΆΠ΅Π½ΠΈΠΉ.In this article, we investigate the LED lamp power supply with a high power factor. To implement this, the power factor corrector of STMicroelectronics L6561 is used in the fly-back topology. With the help of this IC simplifies the construction of the power supply, considering energy-efficiency standards and requirements for the level introduced into the mains distortion.Fir filter design using frequency sampling method
Gravitational Wave Memory of Gamma-Ray Burst Jets
Gamma-Ray Bursts (GRBs) are now considered as relativistic jets. We analyze
the gravitational waves from the acceleration stage of the GRB jets. We show
that (i) the point mass approximation is not appropriate if the opening
half-angle of the jet is larger than the inverse of the Lorentz factor of the
jet, (ii) the gravitational waveform has many step function like jumps, and
(iii) the practical DECIGO and BBO may detect such an event if the GRBs occur
in Local group of galaxy. We found that the light curve of GRBs and the
gravitational waveform are anti-correlated so that the detection of the
gravitational wave is indispensable to determine the structure of GRB jets.Comment: Revtex4, 10 pages, 6 figures, Fig.2 and Fig.3 replaced, minor changes
to text in Sec.I and Sec.V, typos corrected, some reference added, Version to
be published in PR
Anaerobic starvation survival of marine bacteria
Starvation affects marine bacteria also under anaerobic conditions. Some basic data obtained for anaerobic starvation survival of a fermentative and a sulfaterespiring strain indicate substantial differences. The fermentative strain, Listonella (= Vibrio) anguillarum, responded to, nutrient depletion with rapid reduction of their cell size (dwarfing) and decline of viable cell counts by three orders of magnitude. The sulfate-respiring Desulfovibrio vulgaris showed only minor reductions of the cell sizes and no loss of viability. Whereas a drastic decline of cellular protein concentrations in this strain indicated strong endogeneous respiration, starved cells of the fermenting Vibrio sp. showed increasing levels of protein after an initial decrease
ΠΠΈΠ·Π°ΠΉΠ½ Π½Π°Π³Π»ΡΠ΄Π½ΠΎ-Π΄ΠΈΠ΄Π°ΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡΠ° Π΄Π»Ρ ΡΠ΅Π°Π»ΠΈΠ·Π°ΡΠΈΠΈ ΠΏΡΠΎΠ³ΡΠ°ΠΌΠΌ ΠΎΠ±ΡΡΠ΅Π½ΠΈΡ Π² ΡΠ°Π·Π»ΠΈΡΠ½ΡΡ ΠΎΠ±Π»Π°ΡΡΡΡ ΠΈΠ·ΠΎΠ±ΡΠ°Π·ΠΈΡΠ΅Π»ΡΠ½ΠΎΠ³ΠΎ ΠΈΡΠΊΡΡΡΡΠ²Π°
Π¦Π΅Π»ΡΡ Π²ΡΠΏΡΡΠΊΠ½ΠΎΠΉ ΠΊΠ²Π°Π»ΠΈΡΠΈΠΊΠ°ΡΠΈΠΎΠ½Π½ΠΎΠΉ ΡΠ°Π±ΠΎΡΡ ΡΠ²Π»ΡΠ΅ΡΡΡ ΡΠ°Π·ΡΠ°Π±ΠΎΡΠΊΠ° Π΄ΠΈΠ΄Π°ΠΊΡΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡΠ° Π΄Π»Ρ ΠΏΡΠΎΠ²Π΅Π΄Π΅Π½ΠΈΡ ΠΌΠΎΡΡΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ Π°Π½Π°Π»ΠΈΠ·Π° Π² ΠΈΠ·ΡΡΠ΅Π½ΠΈΠΈ ΡΠ²ΠΎΡΡΠ΅ΡΠΊΠΈΡ
Π΄ΠΈΡΡΠΈΠΏΠ»ΠΈΠ½. Π ΡΠΏΠ΅ΡΠΈΠ°Π»ΠΈΠ·ΠΈΡΠΎΠ²Π°Π½Π½ΡΡ
Ρ
ΡΠ΄ΠΎΠΆΠ΅ΡΡΠ²Π΅Π½Π½ΡΡ
ΡΡΡΠ΅ΠΆΠ΄Π΅Π½ΠΈΡΡ
, ΡΡΠ°ΡΠΈΠ΅ΡΡ, Π°Π½Π°Π»ΠΈΠ·ΠΈΡΡΡ Π½Π°ΡΡΡΡ, ΠΏΡΠΈΠ΄Π°ΡΡ Π±ΠΎΠ»ΡΡΠ΅Π΅ Π·Π½Π°ΡΠ΅Π½ΠΈΠ΅ ΡΡΠΈΡΠΎΠ²ΡΠ²Π°Π½ΠΈΡ, ΠΊΠΎΠΏΠΈΡΠΎΠ²Π°Π½ΠΈΡ, Π½Π΅ΠΆΠ΅Π»ΠΈ ΡΠΎΠ±Π»ΡΠ΄Π΅Π½ΠΈΠ΅ Π·Π°ΠΊΠΎΠ½ΠΎΠΌΠ΅ΡΠ½ΠΎΡΡΠ΅ΠΉ ΠΏΠΎΡΡΡΠΎΠ΅Π½ΠΈΡ ΡΠΎΡΠΌΡ ΠΏΡΠ΅Π΄ΠΌΠ΅ΡΠ° - ΡΡΡ ΠΏΡΠΎΠ±Π»Π΅ΠΌΡ ΡΠ΅ΡΠ°Π΅Ρ Π΄ΠΈΠ΄Π°ΠΊΡΠΈΡΠ΅ΡΠΊΠΈΠΉ ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡ. Π Π°Π·ΡΠ°Π±ΠΎΡΠ°Π½Π½ΡΠΉ Π΄ΠΈΠ΄Π°ΠΊΡΠΈΡΠ΅ΡΠΊΠΈΠΉ ΠΊΠΎΠΌΠΏΠ»Π΅ΠΊΡ ΠΈΠΌΠ΅Π΅Ρ ΡΠ½ΠΈΠΊΠ°Π»ΡΠ½ΠΎΠ΅ ΡΠ΅ΡΠ΅Π½ΠΈΠ΅ ΠΈ ΠΏΠΎΠ·Π²ΠΎΠ»ΠΈΡ ΡΠ΅ΡΠΈΡΡ ΠΏΠΎΡΡΠ°Π²Π»Π΅Π½Π½ΡΠ΅ Π·Π°Π΄Π°ΡΠΈ ΠΊΠ°ΠΊ Π΄Π°Π½Π½ΠΎΠΉ ΠΠΠ , ΡΠ°ΠΊ ΠΈ Π΄ΡΡΠ³ΠΈΡ
ΠΏΡΠΎΠ΅ΠΊΡΠΎΠ², Π² ΠΎΡΠ½ΠΎΠ²Π΅ ΠΊΠΎΡΠΎΡΡΡ
Π±ΡΠ΄Π΅Ρ Π»Π΅ΠΆΠ°ΡΡ ΠΏΡΠΎΠ±Π»Π΅ΠΌΠ° ΠΏΡΠΈΠ½ΡΠΈΠΏΠ° ΡΠΎΡΠΌΠΎΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°Π½ΠΈΡ.The goal of the final qualifying work is the development of a didactic kit for morphological analysis in the study of creative disciplines. In specialized art institutions, students, analyzing nature, attach greater importance to drawing, copying, rather than observing the laws of constructing the form of the object - this problem is solved by the didactic kit. The didactic kit developed has a unique solution and will allow to solve the tasks set for both this WRC and other projects based on the problem of the form-building principle
XTE J1739-302: An Unusual New X-ray Transient
A new x-ray transient, designated XTE J1739-302, was discovered with the
Proportional Counter Array (PCA) on the Rossi X-ray Timing Explorer (RXTE) in
data from 12 August 1997. Although it was the brightest source in the Galactic
Center region while active (about 3.0 x 10^-9 ergs/cm2/s from 2 to 25 keV), it
was only observed on that one day; it was not detectable nine days earlier or
two days later. There is no known counterpart at other wavelengths, and its
proximity to the Galactic Center will make such an identification difficult due
to source confusion and extinction. The x-ray spectrum and intensity suggest a
giant outburst of a Be/neutron star binary, although no pulsations were
observed and the outburst was shorter than is usual from these systems.Comment: 11 pages incorporating 6 figures, AAStex; accepted for The
Astrophysical Journal, Part 2 (Letters
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