336 research outputs found

    Mechanical Properties of Thermoplastic Variable-Angle Composite Laminations for Conical Shells

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    Thermoplastic composite automated fiber placement technology, as one of the extreme manufacturing technologies for large or extra large composite components with complex surface shapes, has been widely used in the field of aerospace vehicles. This paper takes 8 lamination groups with different initial placement angles generated by the conical shell variable angle placement algorithm as research objects. Variable angle placement algorithm for conical shell and finite element model establishment method for thermoplastic composite laminations of variable angle with different initial placement angles are presented. Static, modal and buckling analyses are conducted for each group. The results show that stress-strain relation, modal and buckling strength of variable-angle laminations vary regularly with the initial placement angle.ВСхнология автоматичСской ΡƒΠΊΠ»Π°Π΄ΠΊΠΈ тСрмопластичного ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚Π½ΠΎΠ³ΠΎ Π²ΠΎΠ»ΠΎΠΊΠ½Π°, ΡΠ²Π»ΡΡŽΡ‰Π°ΡΡΡ ΠΎΠ΄Π½ΠΎΠΉ ΠΈΠ· Ρ€Π°Π΄ΠΈΠΊΠ°Π»ΡŒΠ½Ρ‹Ρ… Ρ‚Π΅Ρ…Π½ΠΎΠ»ΠΎΠ³ΠΈΠΉ получСния Π±ΠΎΠ»ΡŒΡˆΠΈΡ… ΠΈΠ»ΠΈ ΠΎΡ‡Π΅Π½ΡŒ Π±ΠΎΠ»ΡŒΡˆΠΈΡ… ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚ΠΎΠ² ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚ΠΎΠ² с комплСксными Ρ„ΠΎΡ€ΠΌΠ°ΠΌΠΈ повСрхности, ΡˆΠΈΡ€ΠΎΠΊΠΎ ΠΈΡΠΏΠΎΠ»ΡŒΠ·ΡƒΠ΅Ρ‚ΡΡ Π² Π°Π²ΠΈΠ°Ρ†ΠΈΠΎΠ½Π½ΠΎ-космичСской ΠΏΡ€ΠΎΠΌΡ‹ΡˆΠ»Π΅Π½Π½ΠΎΡΡ‚ΠΈ. Π’ качСствС ΠΎΠ±ΡŠΠ΅ΠΊΡ‚ΠΎΠ² исслСдования использовали восСмь Π³Ρ€ΡƒΠΏΠΏ слоистых ΠΌΠ°Ρ‚Π΅Ρ€ΠΈΠ°Π»ΠΎΠ² с Ρ€Π°Π·Π»ΠΈΡ‡Π½Ρ‹ΠΌΠΈ ΡƒΠ³Π»Π°ΠΌΠΈ конструктивного размСщСния, ΠΊΠΎΡ‚ΠΎΡ€Ρ‹Π΅ Π±Ρ‹Π»ΠΈ созданы с ΠΏΠΎΠΌΠΎΡ‰ΡŒΡŽ Π°Π»Π³ΠΎΡ€ΠΈΡ‚ΠΌΠ° размСщСния ΠΏΠ΅Ρ€Π΅ΠΌΠ΅Π½Π½ΠΎΠ³ΠΎ ΡƒΠ³Π»Π° коничСской ΠΎΠ±ΠΎΠ»ΠΎΡ‡ΠΊΠΈ. ΠŸΡ€Π΅Π΄ΡΡ‚Π°Π²Π»Π΅Π½Ρ‹ Π°Π»Π³ΠΎΡ€ΠΈΡ‚ΠΌ размСщСния ΠΏΠ΅Ρ€Π΅ΠΌΠ΅Π½Π½ΠΎΠ³ΠΎ ΡƒΠ³Π»Π° для коничСской ΠΎΠ±ΠΎΠ»ΠΎΡ‡ΠΊΠΈ ΠΈ модСль Π½Π° основС ΠΌΠ΅Ρ‚ΠΎΠ΄Π° ΠΊΠΎΠ½Π΅Ρ‡Π½Ρ‹Ρ… элСмСнтов для тСрмопластичных слоистых ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚ΠΎΠ² с ΠΏΠ΅Ρ€Π΅ΠΌΠ΅Π½Π½Ρ‹ΠΌ ΡƒΠ³Π»ΠΎΠΌ. Для ΠΊΠ°ΠΆΠ΄ΠΎΠΉ Π³Ρ€ΡƒΠΏΠΏΡ‹ ΠΌΠ°Ρ‚Π΅Ρ€ΠΈΠ°Π»ΠΎΠ² ΠΏΡ€ΠΎΠ²Π΅Π΄Π΅Π½Ρ‹ статистичСский Π°Π½Π°Π»ΠΈΠ·, исслСдованиС ΠΌΠ΅Ρ‚ΠΎΠ΄ΠΎΠΌ разлоТСния ΠΏΠΎ собствСнным Ρ„ΠΎΡ€ΠΌΠ°ΠΌ ΠΈ расчСт устойчивости. УстановлСно, Ρ‡Ρ‚ΠΎ Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡ‚ΡŒ напряТСниС–дСформация, модальная ΠΏΡ€ΠΎΡ‡Π½ΠΎΡΡ‚ΡŒ ΠΈ ΠΏΡ€ΠΎΡ‡Π½ΠΎΡΡ‚ΡŒ ΠΏΡ€ΠΈ ΠΏΡ€ΠΎΠ΄ΠΎΠ»ΡŒΠ½ΠΎΠΌ ΠΈΠ·Π³ΠΈΠ±Π΅ слоистых ΠΌΠ°Ρ‚Π΅Ρ€ΠΈΠ°Π»ΠΎΠ² с ΠΏΠ΅Ρ€Π΅ΠΌΠ΅Π½Π½Ρ‹ΠΌ ΡƒΠ³Π»ΠΎΠΌ пСриодичСски ΠΈΠ·ΠΌΠ΅Π½ΡΡŽΡ‚ΡΡ Π² зависимости ΠΎΡ‚ ΡƒΠ³Π»Π° конструктивного размСщСния.ВСхнологія Π°Π²Ρ‚ΠΎΠΌΠ°Ρ‚ΠΈΡ‡Π½ΠΎΠ³ΠΎ укладання тСрмопластичного ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚Π½ΠΎΠ³ΠΎ Π²ΠΎΠ»ΠΎΠΊΠ½Π°, Ρ‰ΠΎ Ρ” ΠΎΠ΄Π½Ρ–Ρ”ΡŽ Π· Ρ€Π°Π΄ΠΈΠΊΠ°Π»ΡŒΠ½ΠΈΡ… Ρ‚Π΅Ρ…Π½ΠΎΠ»ΠΎΠ³Ρ–ΠΉ отримання Π²Π΅Π»ΠΈΠΊΠΈΡ… Π°Π±ΠΎ Π΄ΡƒΠΆΠ΅ Π²Π΅Π»ΠΈΠΊΠΈΡ… ΠΊΠΎΠΌΠΏΠΎΠ½Π΅Π½Ρ‚Ρ–Π² ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚Ρ–Π² Ρ–Π· комплСксними Ρ„ΠΎΡ€ΠΌΠ°ΠΌΠΈ ΠΏΠΎΠ²Π΅Ρ€Ρ…Π½Ρ–, ΡˆΠΈΡ€ΠΎΠΊΠΎ Π²ΠΈΠΊΠΎΡ€ΠΈΡΡ‚ΠΎΠ²ΡƒΡ”Ρ‚ΡŒΡΡ Π² Π°Π²Ρ–Π°Ρ†Ρ–ΠΉΠ½ΠΎ-космічній промисловості. ΠžΠ±β€™Ρ”ΠΊΡ‚ΠΎΠΌ дослідТСння слугували вісім Π³Ρ€ΡƒΠΏ ΡˆΠ°Ρ€ΡƒΠ²Π°Ρ‚ΠΈΡ… ΠΌΠ°Ρ‚Π΅Ρ€Ρ–Π°Π»Ρ–Π² Ρ–Π· Ρ€Ρ–Π·Π½ΠΈΠΌΠΈ ΠΊΡƒΡ‚Π°ΠΌΠΈ конструктивного розміщСння, які ΠΎΡ‚Ρ€ΠΈΠΌΠ°Π½ΠΎ Π·Π° допомогою Π°Π»Π³ΠΎΡ€ΠΈΡ‚ΠΌΠ° розміщСння Π·ΠΌΡ–Π½Π½ΠΎΠ³ΠΎ ΠΊΡƒΡ‚Π° ΠΊΠΎΠ½Ρ–Ρ‡Π½ΠΎΡ— ΠΎΠ±ΠΎΠ»ΠΎΠ½ΠΊΠΈ. ΠŸΡ€Π΅Π΄ΡΡ‚Π°Π²Π»Π΅Π½ΠΎ Π°Π»Π³ΠΎΡ€ΠΈΡ‚ΠΌ розміщСння Π·ΠΌΡ–Π½Π½ΠΎΠ³ΠΎ ΠΊΡƒΡ‚Π° для ΠΊΠΎΠ½Ρ–Ρ‡Π½ΠΎΡ— ΠΎΠ±ΠΎΠ»ΠΎΠ½ΠΊΠΈ Ρ– модСль Π½Π° основі ΠΌΠ΅Ρ‚ΠΎΠ΄Ρƒ скінчСнних Π΅Π»Π΅ΠΌΠ΅Π½Ρ‚Ρ–Π² для тСрмопластичних ΡˆΠ°Ρ€ΡƒΠ²Π°Ρ‚ΠΈΡ… ΠΊΠΎΠΌΠΏΠΎΠ·ΠΈΡ‚Ρ–Π² Π·Ρ– Π·ΠΌΡ–Π½Π½ΠΈΠΌ ΠΊΡƒΡ‚ΠΎΠΌ. Для ΠΊΠΎΠΆΠ½ΠΎΡ— Π³Ρ€ΡƒΠΏΠΈ ΠΌΠ°Ρ‚Π΅Ρ€Ρ–Π°Π»Ρ–Π² ΠΏΡ€ΠΎΠ²Π΅Π΄Π΅Π½ΠΎ статистичний Π°Π½Π°Π»Ρ–Π·, дослідТСння ΠΌΠ΅Ρ‚ΠΎΠ΄ΠΎΠΌ розкладання Π·Π° власними Ρ„ΠΎΡ€ΠΌΠ°ΠΌΠΈ Ρ– Ρ€ΠΎΠ·Ρ€Π°Ρ…ΡƒΠ½ΠΎΠΊ стійкості. УстановлСно, Ρ‰ΠΎ Π·Π°Π»Π΅ΠΆΠ½Ρ–ΡΡ‚ΡŒ напруТСння–дСформація, модальна ΠΌΡ–Ρ†Π½Ρ–ΡΡ‚ΡŒ Ρ– ΠΌΡ–Ρ†Π½Ρ–ΡΡ‚ΡŒ ΠΏΡ€ΠΈ ΠΏΠΎΠ·Π΄ΠΎΠ²ΠΆΠ½ΡŒΠΎΠΌΡƒ Π·Π³ΠΈΠ½Ρ– ΡˆΠ°Ρ€ΡƒΠ²Π°Ρ‚ΠΈΡ… ΠΌΠ°Ρ‚Π΅Ρ€Ρ–Π°Π»Ρ–Π² Π·Ρ– Π·ΠΌΡ–Π½Π½ΠΈΠΌ ΠΊΡƒΡ‚ΠΎΠΌ ΠΏΠ΅Ρ€Ρ–ΠΎΠ΄ΠΈΡ‡Π½ΠΎ Π·ΠΌΡ–Π½ΡŽΡŽΡ‚ΡŒΡΡ Π² залСТності Π²Ρ–Π΄ ΠΊΡƒΡ‚Π° конструктивного розміщСння

    Transpolar arc observation after solar wind entry into the high-latitude magnetosphere

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    Recently, Cluster observations have revealed the presence of new regions of solar wind plasma entry at the high-latitude magnetospheric lobes tailward of the cusp region, mostly during periods of northward interplanetary magnetic field. In this study, observations from the Global Ultraviolet Imager (GUVI) experiment on board the TIMED spacecraft and Wideband Imaging Camera imager on board the IMAGE satellite are used to investigate a possible link between solar wind entry and the formation of transpolar arcs in the polar cap. We focus on a case when transpolar arc formation was observed twice right after the two solar wind entry events were detected by the Cluster spacecraft. In addition, GUVI and IMAGE observations show a simultaneous occurrence of auroral activity at low and high latitudes after the second entry event, possibly indicating a two-part structure of the continuous band of the transpolar arc

    Quiet in class: classification, noise and the dendritic cell algorithm

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    Theoretical analyses of the Dendritic Cell Algorithm (DCA) have yielded several criticisms about its underlying structure and operation. As a result, several alterations and fixes have been suggested in the literature to correct for these findings. A contribution of this work is to investigate the effects of replacing the classification stage of the DCA (which is known to be flawed) with a traditional machine learning technique. This work goes on to question the merits of those unique properties of the DCA that are yet to be thoroughly analysed. If none of these properties can be found to have a benefit over traditional approaches, then β€œfixing” the DCA is arguably less efficient than simply creating a new algorithm. This work examines the dynamic filtering property of the DCA and questions the utility of this unique feature for the anomaly detection problem. It is found that this feature, while advantageous for noisy, time-ordered classification, is not as useful as a traditional static filter for processing a synthetic dataset. It is concluded that there are still unique features of the DCA left to investigate. Areas that may be of benefit to the Artificial Immune Systems community are suggested

    Observation of Two New N* Peaks in J/psi -> ppiβˆ’nΛ‰p pi^- \bar n and pΛ‰Ο€+n\bar p\pi^+n Decays

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    The Ο€N\pi N system in decays of J/Οˆβ†’NΛ‰NΟ€J/\psi\to\bar NN\pi is limited to be isospin 1/2 by isospin conservation. This provides a big advantage in studying Nβˆ—β†’Ο€NN^*\to \pi N compared with Ο€N\pi N and Ξ³N\gamma N experiments which mix isospin 1/2 and 3/2 for the Ο€N\pi N system. Using 58 million J/ψJ/\psi decays collected with the Beijing Electron Positron Collider, more than 100 thousand J/Οˆβ†’pΟ€βˆ’nΛ‰+c.c.J/\psi \to p \pi^- \bar n + c.c. events are obtained. Besides two well known Nβˆ—N^* peaks at 1500 MeV and 1670 MeV, there are two new, clear Nβˆ—N^* peaks in the pΟ€p\pi invariant mass spectrum around 1360 MeV and 2030 MeV. They are the first direct observation of the Nβˆ—(1440)N^*(1440) peak and a long-sought "missing" Nβˆ—N^* peak above 2 GeV in the Ο€N\pi N invariant mass spectrum. A simple Breit-Wigner fit gives the mass and width for the Nβˆ—(1440)N^*(1440) peak as 1358Β±6Β±161358\pm 6 \pm 16 MeV and 179Β±26Β±50179\pm 26\pm 50 MeV, and for the new Nβˆ—N^* peak above 2 GeV as 2068Β±3βˆ’40+152068\pm 3^{+15}_{-40} MeV and 165Β±14Β±40165\pm 14\pm 40 MeV, respectively

    Solar wind pressure pulse‐driven magnetospheric vortices and their global consequences

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    We report the in situ observation of a plasma vortex induced by a solar wind dynamic pressure enhancement in the nightside plasma sheet using multipoint measurements from Time History of Events and Macroscale Interactions during Substorms (THEMIS) satellites. The vortex has a scale of 5–10 Re and propagates several Re downtail, expanding while propagating. The features of the vortex are consistent with the prediction of the Sibeck (1990) model, and the vortex can penetrate deep (~8 Re ) in the dawn‐dusk direction and couple to field line oscillations. Global magnetohydrodynamics simulations are carried out, and it is found that the simulation and observations are consistent with each other. Data from THEMIS ground magnetometer stations indicate a poleward propagating vortex in the ionosphere, with a rotational sense consistent with the existence of the vortex observed in the magnetotail. Key Points Solar wind pressure pulse‐driven vortex was observed in the magnetosphere Simulation and ground magnetic field data confirm this tailward moving vortex The vortex can penetrate deep inside the tail plasma sheet and couple to FLRsPeer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/107999/1/jgra51112.pd

    Search for Invisible Decays of Ξ·\eta and Ξ·β€²\eta^\prime in J/Οˆβ†’Ο•Ξ·J/\psi \to \phi\eta and ϕη′\phi \eta^\prime

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    Using a data sample of 58Γ—10658\times 10^6 J/ψJ/\psi decays collected with the BES II detector at the BEPC, searches for invisible decays of Ξ·\eta and Ξ·β€²\eta^\prime in J/ψJ/\psi to ϕη\phi\eta and ϕη′\phi\eta^\prime are performed. The Ο•\phi signals, which are reconstructed in K+Kβˆ’K^+K^- final states, are used to tag the Ξ·\eta and Ξ·β€²\eta^\prime decays. No signals are found for the invisible decays of either Ξ·\eta or Ξ·β€²\eta^\prime, and upper limits at the 90% confidence level are determined to be 1.65Γ—10βˆ’31.65 \times 10^{-3} for the ratio B(Ξ·β†’invisible)B(Ξ·β†’Ξ³Ξ³)\frac{B(\eta\to \text{invisible})}{B(\eta\to\gamma\gamma)} and 6.69Γ—10βˆ’26.69\times 10^{-2} for B(Ξ·β€²β†’invisible)B(Ξ·β€²β†’Ξ³Ξ³)\frac{B(\eta^\prime\to \text{invisible})}{B(\eta^\prime\to\gamma\gamma)}. These are the first searches for Ξ·\eta and Ξ·β€²\eta^\prime decays into invisible final states.Comment: 5 pages, 4 figures; Added references, Corrected typo

    Direct Measurements of the Branching Fractions for D0β†’Kβˆ’e+Ξ½eD^0 \to K^-e^+\nu_e and D0β†’Ο€βˆ’e+Ξ½eD^0 \to \pi^-e^+\nu_e and Determinations of the Form Factors f+K(0)f_{+}^{K}(0) and f+Ο€(0)f^{\pi}_{+}(0)

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    The absolute branching fractions for the decays D0β†’Kβˆ’e+Ξ½eD^0 \to K^-e ^+\nu_e and D0β†’Ο€βˆ’e+Ξ½eD^0 \to \pi^-e^+\nu_e are determined using 7584Β±198Β±3417584\pm 198 \pm 341 singly tagged DΛ‰0\bar D^0 sample from the data collected around 3.773 GeV with the BES-II detector at the BEPC. In the system recoiling against the singly tagged DΛ‰0\bar D^0 meson, 104.0Β±10.9104.0\pm 10.9 events for D0β†’Kβˆ’e+Ξ½eD^0 \to K^-e ^+\nu_e and 9.0Β±3.69.0 \pm 3.6 events for D0β†’Ο€βˆ’e+Ξ½eD^0 \to \pi^-e^+\nu_e decays are observed. Those yield the absolute branching fractions to be BF(D0β†’Kβˆ’e+Ξ½e)=(3.82Β±0.40Β±0.27)BF(D^0 \to K^-e^+\nu_e)=(3.82 \pm 0.40\pm 0.27)% and BF(D0β†’Ο€βˆ’e+Ξ½e)=(0.33Β±0.13Β±0.03)BF(D^0 \to \pi^-e^+\nu_e)=(0.33 \pm 0.13\pm 0.03)%. The vector form factors are determined to be ∣f+K(0)∣=0.78Β±0.04Β±0.03|f^K_+(0)| = 0.78 \pm 0.04 \pm 0.03 and ∣f+Ο€(0)∣=0.73Β±0.14Β±0.06|f^{\pi}_+(0)| = 0.73 \pm 0.14 \pm 0.06. The ratio of the two form factors is measured to be ∣f+Ο€(0)/f+K(0)∣=0.93Β±0.19Β±0.07|f^{\pi}_+(0)/f^K_+(0)|= 0.93 \pm 0.19 \pm 0.07.Comment: 6 pages, 5 figure

    Search for the Rare Decays J/Psi --> Ds- e+ nu_e, J/Psi --> D- e+ nu_e, and J/Psi --> D0bar e+ e-

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    We report on a search for the decays J/Psi --> Ds- e+ nu_e + c.c., J/Psi --> D- e+ nu_e + c.c., and J/Psi --> D0bar e+ e- + c.c. in a sample of 5.8 * 10^7 J/Psi events collected with the BESII detector at the BEPC. No excess of signal above background is observed, and 90% confidence level upper limits on the branching fractions are set: B(J/Psi --> Ds- e+ nu_e + c.c.)<4.8*10^-5, B(J/Psi --> D- e+ nu_e + c.c.) D0bar e+ e- + c.c.)<1.1*10^-5Comment: 10 pages, 4 figure

    Measurements of J/psi Decays into 2(pi+pi-)eta and 3(pi+pi-)eta

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    Based on a sample of 5.8X 10^7 J/psi events taken with the BESII detector, the branching fractions of J/psi--> 2(pi+pi-)eta and J/psi-->3(pi+pi-)eta are measured for the first time to be (2.26+-0.08+-0.27)X10^{-3} and (7.24+-0.96+-1.11)X10^{-4}, respectively.Comment: 11 pages, 6 figure

    BESII Detector Simulation

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    A Monte Carlo program based on Geant3 has been developed for BESII detector simulation. The organization of the program is outlined, and the digitization procedure for simulating the response of various sub-detectors is described. Comparisons with data show that the performance of the program is generally satisfactory.Comment: 17 pages, 14 figures, uses elsart.cls, to be submitted to NIM
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