79 research outputs found

    Design and acoustic tests of the ATHENA WFI filter wheel assembly development model towards TRL5

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    The filter wheel (FW) assembly (FWA), developed by the CBK Institute, is one of the critical subsystems of the wide field imager (WFI) instrument on board the Advanced Telescope for High Energy Astrophysics—mission of the ESA Cosmic Vision 2015-25 space science program (launch scheduled around 2035). The instrument has to collect soft x-rays with very high quantum efficiency, thus WFI requires extremely thin optical blocking filter (OBF). Due to its thickness (∼150 nm) and large area (∼170 mm × 170 mm) needed to achieve a 40 ′ × 40 ′ instrument field of view, the filter is extremely vulnerable to acoustic loads generated during Ariane 6 rocket launch. On the other side, FW mechanism has to provide high overall reliability, so it is more favourable to launch the instrument in atmospheric pressure (without vacuum enclosure for filter protection). Design efforts of the FW subsystem were focused on two issues: providing maximal possible sound pressure level suppression and smallest possible differential pressure across the OBF, which should prevent filters from damaging. We describe the design of a reconfigurable acoustic-demonstrator model (DM) of WFI FWA created for purposes of acoustic testing. Also, the acoustic test campaign is described: test methodology, test criteria, and results discussion and its implication on future FWA design. In general, tests conducted with the FWA DM showed that current design of WFI is feasible and the project can be continued without introducing a vacuum enclosure, which would significantly increase system complexity and mass

    Cytosolic SYT/SS18 Isoforms Are Actin-Associated Proteins that Function in Matrix-Specific Adhesion

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    SYT (SYnovial sarcoma Translocated gene or SS18) is widely produced as two isoforms, SYT/L and SYT/S, that are thought to function in the nucleus as transcriptional coactivators. Using isoform-specific antibodies, we detected a sizable pool of SYT isoforms in the cytosol where the proteins were organized into filamentous arrays. Actin and actin-associated proteins co-immunoprecipitated with SYT isoforms, which also co-sedimented and co-localized with the actin cytoskeleton in cultured cells and tissues. The association of SYT with actin bundles was extensive yet stopped short of the distal ends at focal adhesions. Disruption of the actin cytoskeleton also led to a breakdown of the filamentous organization of SYT isoforms in the cytosol. RNAi ablation of SYT/L alone or both isoforms markedly impaired formation of stress fibers and focal adhesions but did not affect formation of cortical actin bundles. Furthermore, ablation of SYT led to markedly impaired adhesion and spreading on fibronectin and laminin-111 but not on collagen types I or IV. These findings indicate that cytoplasmic SYT isoforms interact with actin filaments and function in the ability cells to bind and react to specific extracellular matrices

    Transient excitation of coaxial cone antenna

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    In relation to the using of ultrawideband signals in radar and radiocommunication there appeared a variety of mathematical methods for solving the problems for such signal radiation and propagation. One of them is the method of evolutionary equations relating to the analytical methods in time domain.The essence of the method is that the basis for electromagnetic field expansion is constructed in cross-section. This permits to represent the field in waveguide or free space as a package of the modes and to trace their changes with longitudinal coordinate and passage of time. This requires to solve the evolutionary equation system that represents the second-order partial differential equations of Klein-Gordon type with given initial and boundary conditions. It is convenient to use the method for solving transient problems of radiation and propagation of waves excited by sources with arbitrary time dependencies in layered nonhomogeneous and nonstationary media.In work [2] the characteristics of the coaxial cone antenna (CCA) with a infinite screen are studied theoretically and experimentally in receiving mode. The radiator is the cone antenna excited by step of current. However, at theoretical analysis there considered only one specific case of time current dependence and used the Fourier transform of the solution for sinusoidal waves.The goal of this work is to investigate the videopulse radiation from coaxial cone antenna theoretically by means of the methods of Evolutionary Equations and Duhamel integral as well as to check experimentally the obtained results
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