31 research outputs found

    Π­ΠΊΡΠΏΠ΅Ρ€ΠΈΠΌΠ΅Π½Ρ‚Π°Π»ΡŒΠ½ΠΎΠ΅ обоснованиС установки ацСтабулярного ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Π° с Π½Π΅Π΄ΠΎΠΏΠΎΠΊΡ€Ρ‹Ρ‚ΠΈΠ΅ΠΌ ΠΏΡ€ΠΈ эндопротСзировании ΠΏΠ°Ρ†ΠΈΠ΅Π½Ρ‚ΠΎΠ² с тяТСлой ΡΡ‚Π΅ΠΏΠ΅Π½ΡŒΡŽ дисплазии

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    Purpose. Estimation of critical value of acetabular component uncoverage enabling its implantation without an additional support. Methods. A comparative analysis of an original method for intraoperative measurement of uncoverage space of acetabular component based on the measurement of the depth of uncovered sector with X-ray control by the same technique was carried out. Mathematical computer modeling based on the finite element techniqueand the mechanical experiment were performed. Critical values of uncoverage enabling safe primary fixation of acetabular component were estimated in designed models. Results. High rate of coincidence of direct intraoperative and postoperative measurements by radiograms was obtained, testifying to the possibility of application of this technique of uncoverage estimation at the stage of preoperative X-ray planning in patients with different degree of dysplasia. Using the finite element technique and the mechanical experiment on pelvis models, a possibility of mounting anacetabular component with moderate uncoverage within 25% without screws and with significant uncoverage to 35% with additional two screws fixation was demonstrated.ЦСль Ρ€Π°Π±ΠΎΡ‚Ρ‹ - ΠΎΠΏΡ€Π΅Π΄Π΅Π»Π΅Π½ΠΈΠ΅ критичСской Π²Π΅Π»ΠΈΡ‡ΠΈΠ½Ρ‹ нСдопокрытия ацСтабулярного ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Π°, ΠΏΡ€ΠΈ ΠΊΠΎΡ‚ΠΎΡ€ΠΎΠΉ Π²ΠΎΠ·ΠΌΠΎΠΆΠ½Π° Π΅Π³ΠΎ имплантация Π±Π΅Π· использования Π΄ΠΎΠΏΠΎΠ»Π½ΠΈΡ‚Π΅Π»ΡŒΠ½ΠΎΠΉ ΠΎΠΏΠΎΡ€Ρ‹. ΠœΠ΅Ρ‚ΠΎΠ΄Ρ‹. ΠŸΡ€ΠΎΠ²Π΅Π΄Π΅Π½ ΡΡ€Π°Π²Π½ΠΈΡ‚Π΅Π»ΡŒΠ½Ρ‹ΠΉ Π°Π½Π°Π»ΠΈΠ· ΠΎΡ€ΠΈΠ³ΠΈΠ½Π°Π»ΡŒΠ½ΠΎΠ³ΠΎ способа ΠΈΠ½Ρ‚Ρ€Π°ΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ измСрСния ΠΏΠ»ΠΎΡ‰Π°Π΄ΠΈ нСдопокрытия Π²Π΅Ρ€Ρ‚Π»ΡƒΠΆΠ½ΠΎΠ³ΠΎ ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Π°, основанного Π½Π° ΠΈΠ·ΠΌΠ΅Ρ€Π΅Π½ΠΈΠΈ Π³Π»ΡƒΠ±ΠΈΠ½Ρ‹ Π½Π΅ΠΏΠΎΠΊΡ€Ρ‹Ρ‚ΠΎΠ³ΠΎ сСктора, с рСнтгСновской ΠΎΡ†Π΅Π½ΠΊΠΎΠΉ Ρ‚Π΅ΠΌ ΠΆΠ΅ способом. ΠžΡΡƒΡ‰Π΅ΡΡ‚Π²Π»Π΅Π½Ρ‹ матСматичСскоС ΠΊΠΎΠΌΠΏΡŒΡŽΡ‚Π΅Ρ€Π½ΠΎΠ΅ ΠΌΠΎΠ΄Π΅Π»ΠΈΡ€ΠΎΠ²Π°Π½ΠΈΠ΅ Π½Π° основС ΠΌΠ΅Ρ‚ΠΎΠ΄Π° ΠΊΠΎΠ½Π΅Ρ‡Π½Ρ‹Ρ… элСмСнтов ΠΈ мСханичСский экспСримСнт. Π’ Ρ€Π°Π·Ρ€Π°Π±ΠΎΡ‚Π°Π½Π½Ρ‹Ρ… модСлях ΠΎΠΏΡ€Π΅Π΄Π΅Π»ΡΠ»ΠΈΡΡŒ критичСскиС Π²Π΅Π»ΠΈΡ‡ΠΈΠ½Ρ‹ нСдопокрытия, ΠΏΡ€ΠΈ ΠΊΠΎΡ‚ΠΎΡ€Ρ‹Ρ… Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎ обСспСчСниС Π½Π°Π΄Π΅ΠΆΠ½ΠΎΠΉ ΠΏΠ΅Ρ€Π²ΠΈΡ‡Π½ΠΎΠΉ фиксации ацСтабулярного ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Π° Π Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹. ВыявлСна высокая ΡΡ‚Π΅ΠΏΠ΅Π½ΡŒ совпадСния прямых ΠΈΠ½Ρ‚Ρ€Π°ΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½Ρ‹Ρ… ΠΈ послСопСрационных ΠΈΠ·ΠΌΠ΅Ρ€Π΅Π½ΠΈΠΉ ΠΏΠΎ Ρ€Π΅Π½Ρ‚Π³Π΅Π½ΠΎΠ³Ρ€Π°ΠΌΠΌΠ°ΠΌ, Ρ‡Ρ‚ΠΎ ΡΠ²ΠΈΠ΄Π΅Ρ‚Π΅Π»ΡŒΡΡ‚Π²ΡƒΠ΅Ρ‚ ΠΎ возмоТности примСнСния Π΄Π°Π½Π½ΠΎΠ³ΠΎ ΠΌΠ΅Ρ‚ΠΎΠ΄Π° ΠΎΡ†Π΅Π½ΠΊΠΈ нСдопокрытия Π½Π° этапС ΠΏΡ€Π΅Π΄ΠΎΠΏΠ΅Ρ€Π°Ρ†ΠΈΠΎΠ½Π½ΠΎΠ³ΠΎ рСнтгСновского планирования Ρƒ ΠΏΠ°Ρ†ΠΈΠ΅Π½Ρ‚ΠΎΠ² с Ρ€Π°Π·Π»ΠΈΡ‡Π½ΠΎΠΉ ΡΡ‚Π΅ΠΏΠ΅Π½ΡŒΡŽ дисплазии. Π‘ ΠΏΠΎΠΌΠΎΡ‰ΡŒΡŽ ΠΌΠ΅Ρ‚ΠΎΠ΄Π° ΠΊΠΎΠ½Π΅Ρ‡Π½Ρ‹Ρ… элСмСнтов ΠΈ мСханичСского экспСримСнта Π½Π° модСлях Ρ‚Π°Π·Π° ΠΏΠΎΠΊΠ°Π·Π°Π½Π° Π²ΠΎΠ·ΠΌΠΎΠΆΠ½ΠΎΡΡ‚ΡŒ установки ацСтабулярного ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Π° с ΡƒΠΌΠ΅Ρ€Π΅Π½Π½Ρ‹ΠΌ Π½Π΅Π΄ΠΎΠΏΠΎΠΊΡ€Ρ‹Ρ‚ΠΈΠ΅ΠΌ Π² ΠΏΡ€Π΅Π΄Π΅Π»Π°Ρ… 25% Π±Π΅Π· Π²ΠΈΠ½Ρ‚ΠΎΠ² ΠΈ со Π·Π½Π°Ρ‡ΠΈΡ‚Π΅Π»ΡŒΠ½Ρ‹ΠΌ Π½Π΅Π΄ΠΎΠΏΠΎΠΊΡ€Ρ‹Ρ‚ΠΈΠ΅ΠΌ Π΄ΠΎ 35% с Π΄ΠΎΠΏΠΎΠ»Π½ΠΈΡ‚Π΅Π»ΡŒΠ½ΠΎΠΉ фиксациСй двумя Π²ΠΈΠ½Ρ‚Π°ΠΌΠΈ

    Signatures of the slow solar wind streams from active regions in the inner corona

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    Some of local sources of the slow solar wind can be associated with spectroscopically detected plasma outflows at edges of active regions accompanied with specific signatures in the inner corona. The EUV telescopes (e.g. SPIRIT/CORONAS-F, TESIS/CORONAS-Photon and SWAP/PROBA2) sometimes observed extended ray-like structures seen at the limb above active regions in 1MK iron emission lines and described as "coronal rays". To verify the relationship between coronal rays and plasma outflows, we analyze an isolated active region (AR) adjacent to small coronal hole (CH) observed by different EUV instruments in the end of July - beginning of August 2009. On August 1 EIS revealed in the AR two compact outflows with the Doppler velocities V =10-30 km/s accompanied with fan loops diverging from their regions. At the limb the ARCH interface region produced coronal rays observed by EUVI/STEREO-A on July 31 as well as by TESIS on August 7. The rays were co-aligned with open magnetic field lines expanded to the streamer stalks. Using the DEM analysis, it was found that the fan loops diverged from the outflow regions had the dominant temperature of ~1 MK, which is similar to that of the outgoing plasma streams. Parameters of the solar wind measured by STEREO-B, ACE, WIND, STEREO-A were conformed with identification of the ARCH as a source region at the Wang-Sheeley-Arge map of derived coronal holes for CR 2086. The results of the study support the suggestion that coronal rays can represent signatures of outflows from ARs propagating in the inner corona along open field lines into the heliosphere.Comment: Accepted for publication in Solar Physics; 31 Pages; 13 Figure

    Nanolocalized UV source of laser radiation

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    We show the results of optical nonlinear interaction of laser light with plasmonic nanostructures. Creation of a nanolocalized source of UV radiation (Ξ» = 260 nm) of the record high intensity was demonstated. Possibility of use of the source for biomedical applications was shown

    Nanolocalized UV source of laser radiation

    No full text
    We show the results of optical nonlinear interaction of laser light with plasmonic nanostructures. Creation of a nanolocalized source of UV radiation (Ξ» = 260 nm) of the record high intensity was demonstated. Possibility of use of the source for biomedical applications was shown

    Single photon transport by a moving atom through sub-wavelength hole

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    The results of investigation of photon transport through the subwavelength hole in the opaque screen by using single neutral atom are represented. The basis of the proposed and implemented method is the absorption of a photon by a neutral atom immediately before the subwavelength aperture, traveling of the atoms through the hole and emission of a photon on the other side of the screen. Realized method is the alternative approach to existing for photon transport through a subwavelength aperture: 1) self-sustained transmittance of a photon through the aperture according to the Bethe’s model; 2) extra ordinary transmission because of surface-plasmon excitation

    Single photon transport by a moving atom through sub-wavelength hole

    No full text
    The results of investigation of photon transport through the subwavelength hole in the opaque screen by using single neutral atom are represented. The basis of the proposed and implemented method is the absorption of a photon by a neutral atom immediately before the subwavelength aperture, traveling of the atoms through the hole and emission of a photon on the other side of the screen. Realized method is the alternative approach to existing for photon transport through a subwavelength aperture: 1) self-sustained transmittance of a photon through the aperture according to the Bethe’s model; 2) extra ordinary transmission because of surface-plasmon excitation
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