445 research outputs found
Assessment of pharmacological activity and bioavailability of the new derivative 1,3,4-thiadiazole
Acexazolamide is a new derivative of 1,3,4-thiadiazole and acexamic acid. In animal experiments, acute toxicity, pharmacological activity and bioavailability of acexazolamide were evaluate
Conditioned Unitary Transformation on biphotons
A conditioned unitary transformation ( polarization rotation) is
performed at single-photon level. The transformation is realized by rotating
polarization for one of the photons of a polarization-entangled biphoton state
(signal photon) by means of a Pockel's cell triggered by the detection of the
other (idler) photon after polarization selection. As a result, polarization
degree for the signal beam changes from zero to the value given by the idler
detector quantum efficiency. This result is relevant to practical realization
of various quantum information schemes and can be used for developing a new
method of absolute quantum efficiency calibration
Design and evaluation of pharmacological properties of a new 1,3,4-thiadiazolylamide derivative of 2-propylpentanoic acid
The use of the pharmacophoric approach is a promising direction for modifying the chemical structure of 2-propylpentanoic (valproic) acid in order to obtain new drug
ΠΠΎΡΡΡΠΈΡΠΈΠ΅Π½Ρ ΡΡΠΌΠ°: ΠΎΡΠ΅Π½ΠΊΠ° ΡΡΠΌΠΎΠ²ΡΡ Ρ Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ ΡΠ°Π΄ΠΈΠΎΡΠΎΡΠΎΠ½Π½ΠΎΠ³ΠΎ ΡΡΠ°ΠΊΡΠ° Π½Π° ΠΎΡΠ½ΠΎΠ²Π΅ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΠΎΠ² ΠΈΠ·ΠΌΠ΅ΡΠ΅Π½ΠΈΡ ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠ° ΡΡΠΌΠ°
In radiophotonic microwave transmission systems, as in any radioelectronic systems, noise characteristics determine the potential of accuracy and range. As a measure of the difference between the noise characteristics of optoelectronic microwave signal converters from ideal ones, the use of the noise figures of the elements included in their composition is proposed. The effect of such a criterion is demonstrated by the example of the optoelectronic microwave oscillator (OEO). Based on the results of the study of the optoelectronic microwave oscillator noise parameters quantitative characteristics of the conversion of the OEO elements noise sources into phase and amplitude fluctuations of the output microwave oscillation are obtained. The analysis of the interaction of the OEO elements noise with the microwave harmonic oscillation is performed. The technique for measuring the noise conversion characteristics using the noise figure has been developed. The results of measuring characteristics of the interaction of harmonic oscillation with the optoelectronic components additive and multiplicative noise of optoelectronic components are presented. Based on the values of the noise figure, the possibilities of reducing the noise levels of microwave signal converters are evaluated and recommendations are made to reduce the influence of the noise.Π ΡΠ°Π΄ΠΈΠΎΡΠΎΡΠΎΠ½Π½ΡΡ
ΡΠΈΡΡΠ΅ΠΌΠ°Ρ
ΠΏΠ΅ΡΠ΅Π΄Π°ΡΠΈ Π‘ΠΠ§-ΡΠΈΠ³Π½Π°Π»ΠΎΠ², ΠΊΠ°ΠΊ ΠΈ Π² Π»ΡΠ±ΡΡ
ΡΠ°Π΄ΠΈΠΎΡΠ»Π΅ΠΊΡΡΠΎΠ½Π½ΡΡ
ΡΠΈΡΡΠ΅ΠΌΠ°Ρ
, ΡΡΠΌΠΎΠ²ΡΠ΅ Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊΠΈ ΠΎΠΏΡΠ΅Π΄Π΅Π»ΡΡΡ ΠΏΠΎΡΠ΅Π½ΡΠΈΠ°Π»ΡΠ½ΡΠ΅ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎΡΡΠΈ ΠΏΠΎ ΡΠΎΡΠ½ΠΎΡΡΠΈ ΠΈ Π΄Π°Π»ΡΠ½ΠΎΡΡΠΈ Π΄Π΅ΠΉΡΡΠ²ΠΈΡ. ΠΡΠ΅Π΄Π»ΠΎΠΆΠ΅Π½ΠΎ Π² ΠΊΠ°ΡΠ΅ΡΡΠ²Π΅ ΠΌΠ΅ΡΡ ΠΎΡΠ»ΠΈΡΠΈΡ ΡΡΠΌΠΎΠ²ΡΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ ΠΎΠΏΡΠΎΡΠ»Π΅ΠΊΡΡΠΎΠ½Π½ΡΡ
ΠΏΡΠ΅ΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°ΡΠ΅Π»Π΅ΠΉ Π‘ΠΠ§-ΡΠΈΠ³Π½Π°Π»ΠΎΠ² ΠΎΡ ΠΈΠ΄Π΅Π°Π»Π° ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°ΡΡ ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΡ ΡΡΠΌΠ° ΡΠ»Π΅ΠΌΠ΅Π½ΡΠΎΠ², Π²Ρ
ΠΎΠ΄ΡΡΠΈΡ
Π² ΠΈΡ
ΡΠΎΡΡΠ°Π². ΠΠ° ΠΏΡΠΈΠΌΠ΅ΡΠ΅ ΠΎΠΏΡΠΎΡΠ»Π΅ΠΊΡΡΠΎΠ½Π½ΠΎΠ³ΠΎ (ΠΠ) Π‘ΠΠ§-Π³Π΅Π½Π΅ΡΠ°ΡΠΎΡΠ° ΠΏΠΎΠΊΠ°Π·Π°Π½ΠΎ Π΄Π΅ΠΉΡΡΠ²ΠΈΠ΅ ΡΠ°ΠΊΠΎΠ³ΠΎ ΠΊΡΠΈΡΠ΅ΡΠΈΡ. ΠΠΏΠΈΡΠ°ΡΡΡ Π½Π° ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΡ ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΡ ΡΡΠΌΠΎΠ²ΡΡ
ΠΏΠ°ΡΠ°ΠΌΠ΅ΡΡΠΎΠ² ΠΠ Π‘ΠΠ§-Π³Π΅Π½Π΅ΡΠ°ΡΠΎΡΠ°, ΠΏΠΎΠ»ΡΡΠ΅Π½Ρ ΠΊΠΎΠ»ΠΈΡΠ΅ΡΡΠ²Π΅Π½Π½ΡΠ΅ Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊΠΈ ΠΏΡΠ΅ΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°Π½ΠΈΡ ΠΈΡΡΠΎΡΠ½ΠΈΠΊΠΎΠ² ΡΡΠΌΠΎΠ² ΡΠ»Π΅ΠΌΠ΅Π½ΡΠΎΠ², Π²Ρ
ΠΎΠ΄ΡΡΠΈΡ
Π² ΡΠΎΡΡΠ°Π² ΠΠ Π³Π΅Π½Π΅ΡΠ°ΡΠΎΡΠ°, Π²ΠΎ ΡΠ»ΡΠΊΡΡΠ°ΡΠΈΠΈ ΡΠ°Π·Ρ ΠΈ Π°ΠΌΠΏΠ»ΠΈΡΡΠ΄Ρ Π²ΡΡ
ΠΎΠ΄Π½ΠΎΠ³ΠΎ Π‘ΠΠ§-ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΡ. ΠΡΠΏΠΎΠ»Π½Π΅Π½ Π°Π½Π°Π»ΠΈΠ· Π²Π·Π°ΠΈΠΌΠΎΠ΄Π΅ΠΉΡΡΠ²ΠΈΡ ΡΡΠΌΠΎΠ² ΡΠ»Π΅ΠΌΠ΅Π½ΡΠΎΠ² ΠΠ Π³Π΅Π½Π΅ΡΠ°ΡΠΎΡΠ° Ρ Π‘ΠΠ§ Π³Π°ΡΠΌΠΎΠ½ΠΈΡΠ΅ΡΠΊΠΈΠΌ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΠ΅ΠΌ. Π Π°Π·ΡΠ°Π±ΠΎΡΠ°Π½Π° ΠΌΠ΅ΡΠΎΠ΄ΠΈΠΊΠ° ΠΈΠ·ΠΌΠ΅ΡΠ΅Π½ΠΈΡ Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ ΠΏΡΠ΅ΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°Π½ΠΈΡ ΡΡΠΌΠΎΠ² Ρ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½ΠΈΠ΅ΠΌ ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠ° ΡΡΠΌΠ°. ΠΡΠΈΠ²Π΅Π΄Π΅Π½Ρ ΡΠ΅Π·ΡΠ»ΡΡΠ°ΡΡ ΠΈΠ·ΠΌΠ΅ΡΠ΅Π½ΠΈΡ ΡΡΠΌΠΎΠ²ΡΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ Π²Π·Π°ΠΈΠΌΠΎΠ΄Π΅ΠΉΡΡΠ²ΠΈΡ Π³Π°ΡΠΌΠΎΠ½ΠΈΡΠ΅ΡΠΊΠΎΠ³ΠΎ ΠΊΠΎΠ»Π΅Π±Π°Π½ΠΈΡ Ρ Π°Π΄Π΄ΠΈΡΠΈΠ²Π½ΡΠΌ ΠΈ ΠΌΡΠ»ΡΡΠΈΠΏΠ»ΠΈΠΊΠ°ΡΠΈΠ²Π½ΡΠΌ ΡΡΠΌΠΎΠΌ ΠΎΠΏΡΠΎΡΠ»Π΅ΠΊΡΡΠΎΠ½Π½ΡΡ
ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½ΡΠΎΠ². ΠΠΎ Π·Π½Π°ΡΠ΅Π½ΠΈΡΠΌ ΠΊΠΎΡΡΡΠΈΡΠΈΠ΅Π½ΡΠ° ΡΡΠΌΠ° ΠΎΡΠ΅Π½ΠΈΠ²Π°ΡΡΡΡ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎΡΡΠΈ ΡΠΌΠ΅Π½ΡΡΠ΅Π½ΠΈΡ ΡΡΠΎΠ²Π½Π΅ΠΉ ΡΡΠΌΠΎΠ² ΠΏΡΠ΅ΠΎΠ±ΡΠ°Π·ΠΎΠ²Π°ΡΠ΅Π»Π΅ΠΉ Π‘ΠΠ§-ΡΠΈΠ³Π½Π°Π»ΠΎΠ² ΠΈ Π΄Π°ΡΡΡΡ ΡΠ΅ΠΊΠΎΠΌΠ΅Π½Π΄Π°ΡΠΈΠΈ ΠΏΠΎ ΡΠΌΠ΅Π½ΡΡΠ΅Π½ΠΈΡ Π²Π»ΠΈΡΠ½ΠΈΡ ΡΡΠΌΠΎΠ²
Status of the FLUTE RF System Upgrade
FLUTE (Ferninfrarot Linac- Und Test-Experiment) is a compact versatile linac-based accelerator test facility at KIT. Its main goal is to serve as a platform for a variety of accelerator studies and to generate strong ultra-short THz pulses for photon science. It will also serve as an injector for a Very Large Acceptance compact Storage Ring (VLA-cSR), which will be realized at KIT in the framework of the compact STorage Ring for Accelerator Research and Technology (cSTART) project. To achieve acceleration of electrons in the RF photoinjector and LINAC (from FLUTE) with high stability, it is necessary to provide stable RF power. For this goal, an upgrade of the existing RF system design has been proposed and is currently being implemented. This contribution will report on the updated RF system design and the commissioning status of the new RF system components
Probing AGN with spectropolarimetry: accretion disk and SMBH parameters
The interaction of a supermassive black hole with the matter of an accretion
disk in the presence of a magnetic field is the key mechanism of energy release
in active galactic nuclei. However, determining the physical parameters of this
system, such as the spin and mass of the black hole, the shape and parameters
of the rotation of the accretion disk, and the geometry of the magnetic field
in the accretion disk is a complex and not completely solved problem. We have
previously shown, based on our numerical models, that these estimates can be
obtained from just three parameters: the black hole mass, bolometric
luminosity, and optical polarization. In this paper, we estimate the accretion
disk and black hole parameters for a sample of 14 type 1 Seyfert galaxies.
Using the spectropolarimetric data obtained by us, we selected only those
objects in which the polarization of optical radiation is generated mainly by
the mechanism in the accretion disk. Despite the small statistics, our results
for such a sample are consistent with our previous conclusions and show a
discrepancy between the disk magnetic field parameters and the classical
Shakura-Sunyaev disk model.Comment: 9 pages, 5 figure
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