• Title/Summary/Keyword: direct kinematics

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Fipronil impairs the fertilization competence of boar spermatozoa

  • Adikari Arachchige Dilki Indrachapa Adikari;Malavige Romesha Chandanee;Byeong-Yeon Kim;Young-Joo Yi
    • Korean Journal of Agricultural Science
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    • v.49 no.1
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    • pp.103-112
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    • 2022
  • Fipronil is a popular insecticide used in both agricultural and domestic fields. Factors that affect sperm and eggs have a direct influence on reproductive outcomes. This study was undertaken to assess the effect of varying concentrations (10 - 200 μM) of fipronil and incubation times (30 min and 2 hrs) on boar spermatozoa. Spermatozoa were evaluated for motility, motion kinematics, viability, chromatin stability, and for the generation of intracellular reactive oxygen species (ROS) and the results were compared to those from corresponding controls. The findings revealed a significant, dose-dependent reduction in sperm motility in all fipronil treatment groups at 30 min of incubation (p < 0.05). A similar dose-dependent reduction in sperm motility was observed subsequent to fipronil exposure for 2 hrs of incubation (p < 0.05). Groups treated with fipronil showed a gradual reduction in motion kinematics (p < 0.05). Moreover, a significantly higher percentage of dead sperm was observed at 200 μM fipronil, as compared to the highest live percentage obtained in controls (p < 0.05). Evaluating the sperm chromatin integrity revealed a significantly higher percentage of damaged chromatin in spermatozoa incubated with 200 μM of fipronil. Moreover, ROS production was significantly higher in fipronil-exposed sperm (p < 0.05). In conclusion, boar spermatozoa incubated with fipronil showed decreased levels of sperm motility and viability, weaker chromatin integrity, and increased levels of intracellular ROS generation, all of which indicate that exposure to fipronil potentially impairs the fertilization competence of boar spermatozoa.

The Biomechancial Effects of an Interspinous Spacer Implant on 3-D Motions for the Treatment of Lumbar Spinal Stenosis (요추부 척추관 협착증 치료를 위한 극돌기간 삽입술의 3차원 분석을 통한 생체역학적 효과 분석)

  • 이희성;신규철;문수정;정태곤;이권용;이성재
    • Proceedings of the Korean Society of Precision Engineering Conference
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    • 2004.10a
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    • pp.1207-1210
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    • 2004
  • As many humans age, degenerative lumbar spinal stenosis (DLSS) becomes a major cause of lower limb discomfort and disability. By surgical treatment method of DLSS, the existing surgical treatment methods using internal fixation have showed degeneration changes of an adjacent vertebrae and loss of lumbar spine lordosis-kyphosis due to eliminating a motion. For solving the problems of internal fixation, a novel interspinous spacer has been developed to treat DLSS by surgical treatment method. In this study, we evaluated the biomechanical effects of the interspinous spacer on the kinematics of the porcine lumbar spine before and after insertion of the implant. For this purpose, a device that is capable of measuring 3-D motions were built based on direct linear transformation (DLT) algorithm written with MATLAB program. Results showed that in extension, a change of the mean angle between the intact and the implanted specimens at L4-L5 was 1.87 degree difference and the implant reduced the extension range of motion of the L4-L5 (p&lt;0.05). But the range of motion in flexion, axial rotation and lateral bending at the adjacent segments was not statistically affected by the implant. In conclusion, we thought that interspinous spacer may have remedical value for DLSS by flexing human lumbar spine.

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Stochastic dynamic instability response of piezoelectric functionally graded beams supported by elastic foundation

  • Shegokara, Niranjan L.;Lal, Achchhe
    • Advances in aircraft and spacecraft science
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    • v.3 no.4
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    • pp.471-502
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    • 2016
  • This paper presents the dynamic instability analysis of un-damped elastically supported piezoelectric functionally graded (FG) beams subjected to in-plane static and dynamic periodic thermomechanical loadings with uncertain system properties. The elastic foundation model is assumed as one parameter Pasternak foundation with Winkler cubic nonlinearity. The piezoelectric FG beam is subjected to non-uniform temperature distribution with temperature dependent material properties. The Young's modulus and Poison's ratio of ceramic, metal and piezoelectric, density of respective ceramic and metal, volume fraction exponent and foundation parameters are taken as uncertain system properties. The basic nonlinear formulation of the beam is based on higher order shear deformation theory (HSDT) with von-Karman strain kinematics. The governing deterministic static and dynamic random instability equation and regions is solved by Bolotin's approach with Newmark's time integration method combined with first order perturbation technique (FOPT). Typical numerical results in terms of the mean and standard deviation of dynamic instability analysis are presented to examine the effect of slenderness ratios, volume fraction exponents, foundation parameters, amplitude ratios, temperature increments and position of piezoelectric layers by changing the random system properties. The correctness of the present stochastic model is examined by comparing the results with direct Monte Caro simulation (MCS).

Identifying potential mergers of globular clusters: a machine-learning approach

  • Pasquato, Mario
    • The Bulletin of The Korean Astronomical Society
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    • v.39 no.2
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    • pp.89-89
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    • 2014
  • While the current consensus view holds that galaxy mergers are commonplace, it is sometimes speculated that Globular Clusters (GCs) may also have undergone merging events, possibly resulting in massive objects with a strong metallicity spread such as Omega Centauri. Galaxies are mostly far, unresolved systems whose mergers are most likely wet, resulting in observational as well as modeling difficulties, but GCs are resolved into stars that can be used as discrete dynamical tracers, and their mergers might have been dry, therefore easily simulated with an N-body code. It is however difficult to determine the observational parameters best suited to reveal a history of merging based on the positions and kinematics of GC stars, if evidence of merging is at all observable. To overcome this difficulty, we investigate the applicability of supervised and unsupervised machine learning to the automatic reconstruction of the dynamical history of a stellar system. In particular we test whether statistical clustering methods can classify simulated systems into monolithic versus merger products. We run direct N-body simulations of two identical King-model clusters undergoing a head-on collision resulting in a merged system, and other simulations of isolated King models with the same total number of particles as the merged system. After several relaxation times elapse, we extract a sample of snapshots of the sky-projected positions of particles from each simulation at different dynamical times, and we run a variety of clustering and classification algorithms to classify the snapshots into two subsets in a relevant feature space.

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The study of predictive performance of low Reynolds number turbulence model in the backward-facing step flow (후방계단유동에 대한 저레이놀즈 수 난류모형의 예측성능에 관한 연구)

  • Kim, Won-Gap;Choe, Yeong-Don
    • Transactions of the Korean Society of Mechanical Engineers B
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    • v.20 no.5
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    • pp.1661-1670
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    • 1996
  • Incompressible flow over a backward-facing step is computed by low Reynolds number turbulence models in order to compare with direct simulation results. In this study, selected low Reynolds number 1st and 2nd (Algebraic Stress Model : ASM) moment closure turbulence models are adopted and compared with each other. Each turbulence model predicts different flow characteristics, different re-attachment point, velocity profiles and Reynolds stress distribution etc. Results by .kappa.-.epsilon. turbulence models indicate that predicted re-attachment lengths are shorter than those by standard model. Turbulent intensity and eddy viscosity by low Reynolds number .kappa.-.epsilon. models are still greater than DNS results. The results by algebraic stress model (ASM) are more reasonable than those by .kappa.-.epsilon. models. The convective scheme is QUICK (Quadratic Upstream Interpolation for Convective Kinematics) and SIMPLE algorithm is adopted. Reynolds number based on step height and inlet free stream velocity is 5100.

Analytic Generation of Reach Volume Based on Range of Two Degrees of Freedom Motion (2자유도 동작범위를 고려한 reach volume의 해석적 생성)

  • Kee, Do-Hyung
    • Journal of Korean Institute of Industrial Engineers
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    • v.23 no.1
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    • pp.147-162
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    • 1997
  • When designing workplaces or arranging controls on panel, devices and controls should be placed within the reach of operator's arm or foot to guarantee effective performances. Most of the existing research on the reach volume were based on measurements of a few subject's arm reach, and limited to Caucasian and Chinese populations. Furthermore, reach volume considering foot or trunk motion have not been investigated. Range of human joint motion and that of two degrees of freedom motion are needed to generate reach volume analytically using the sweeping algorithm. However, range of two degrees of freedom motion has not been measured up to now. Therefore, range of two degrees of freedom motion was measured in this research, where 47 college students were participated voluntarily as subjects. The results showed that the motion of one joint can be limited by the motion of another motion, that is to say, the shoulder flexion was decreased significantly when the shoulder was adducted or abducted. Second, new approximate algorithms generating reach volumes were suggested, in which range of two degrees of freedom motion was used as input data. Depending upon the body segment included such as trunk, arm and leg, three types of reach volume were provided, in which the human body was modeled as a multilink system based on the robot kinematics and the sweeping method was employed. Reach volume generated analytically in this study showed statistically reasonable results when compared with that obtained from direct measurement.

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Under-Developed and Under-Utilized Eclipsing Binary Model Capabilities

  • Wilson, R.E.
    • Journal of Astronomy and Space Sciences
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    • v.29 no.2
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    • pp.115-121
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    • 2012
  • Existing but largely unused binary star model capabilities are examined. An easily implemented scheme is parameterization of starspot growth and decay that can stimulate work on outer convection zones and their dynamos. Improved precision in spot computation now enhances analysis of very precise data. An existing computational model for blended spectral line profiles is accurate for binary system effects but needs to include damping, thermal Doppler, and other intrinsic broadening effects. Binary star ephemerides had been found exclusively from eclipse timings until recently, but now come also from whole light and radial velocity curves. A logical further development will be to expand these whole curve solutions to include eclipse timings. An attenuation model for circumstellar clouds, with several absorption and scattering mechanisms, has been applied only once, perhaps because the model clouds have fixed locations. However the clouds could be made to move dynamically and be combined into moving streams and disks. An area of potential interest is polarization curve analysis, where incentive for modeling could follow from publication of observed polarization curves. Other recent advances include direct single step solutions for temperatures of both stars of an eclipsing binary and third body kinematics from combined light and velocity curves.

INFLOWS IN MASSIVE STAR FORMATION REGIONS

  • WU, YUEFANG;LIU, TIE;QIN, SHENGLI
    • Publications of The Korean Astronomical Society
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    • v.30 no.2
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    • pp.93-97
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    • 2015
  • How high-mass stars form is currently unclear. Calculations suggest that the radiation pressure of a forming star can halt spherical infall, preventing further growth when it reaches $10M_{\odot}$. Two major theoretical models on the further growth of stellar mass have been proposed. One model suggests the merging of less massive stellar objects, and the other is through accretion, but with the help of a disk. Inflow motions are key evidence for how forming stars gain further mass to build up massive stars. Recent developments in technology have boosted the search for inflow motion. A number of high-mass collapse candidates were obtained with single dish observations, and mostly showed blue profiles. Infalling signatures seem to be more common in regions which have developed radiation pressure than in younger cores, which is the opposite of the theoretical prediction and is also very different from observations of low mass star formation. Interferometer studies so far confirm this tendency with more obvious blue profiles or inverse P Cygni profiles. Results seem to favor the accretion model. However, the evolution of the infall motion in massive star forming cores needs to be further explored. Direct evidence for monolithic or competitive collapse processes is still lacking. ALMA will enable us to probe more detail of the gravitional processes.

A class of actuated deployable and reconfigurable multilink structures

  • Phocas, Marios C.;Georgiou, Niki;Christoforou, Eftychios G.
    • Advances in Computational Design
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    • v.7 no.3
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    • pp.189-210
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    • 2022
  • Deployable structures have the ability to shift from a compact state to an expanded functional configuration. By extension, reconfigurability is another function that relies on embedded computation and actuators. Linkage-based mechanisms constitute promising systems in the development of deployable and reconfigurable structures with high flexibility and controllability. The present paper investigates the deployment and reconfigurability of modular linkage structures with a pin and a sliding support, the latter connected to a linear motion actuator. An appropriate control sequence consists of stepwise reconfigurations that involve the selective releasing of one intermediate joint in each closed-loop linkage, effectively reducing it to a 1-DOF "effective crank-slider" mechanism. This approach enables low self-weight and reduced energy consumption. A kinematics and finite-element analysis of different linkage systems, in all intermediate reconfiguration steps of a sequence, have been conducted for different lengths and geometrical characteristics of the members, as well as different actuation methods, i.e., direct and cable-driven actuation. The study provides insight into the impact of various structural typological and geometrical factors on the systems' behavior.

Study for Real-World Accident Database and Occupant Behavior Analysis in Far-Side Collisions (Far-Side 실사고 분석과 승객거동해석 연구)

  • Jaeho, Shin;Chang Min, Baek
    • Journal of Auto-vehicle Safety Association
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    • v.14 no.4
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    • pp.77-83
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    • 2022
  • Occupant behaviors and body contact with vehicle interior parts are main injury mechanism in far-side collisions. In vehicle side impact accident where the crash accident occurs on the opposite side of the vehicle from the a particular occupant, it is exposed in terms of relatively larger lateral motion to interact with the opposite side of the vehicle structure. The challenge of minimizing motions of upper body and injury risk according to a direct contact is a primary occupant protection research. This study has performed a data analysis of real-world accident database extracted from the 2016~2020 CISS database and a parametric investigation of impact angles and occupant kinematics in far-side lateral and oblique impact simulations. A detailed data analysis was conducted to reveal the relationship among the accident and injury data. Database analysis and computational far-side impact results proposed the fundamental vehicle design for safety improvement in far-side collisions.