radial motion
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2021 ◽  
Vol 57 (11) ◽  
Author(s):  
D. A. Nesterenko ◽  
T. Eronen ◽  
Z. Ge ◽  
A. Kankainen ◽  
M. Vilen

AbstractPhase-imaging ion-cyclotron-resonance technique has been implemented at the Penning-trap mass spectrometer JYFLTRAP and is routinely employed for mass measurements of stable and short-lived nuclides produced at IGISOL facility. Systematic uncertainties that impose limitations on the accuracy of measurements are discussed. It was found out that the phase evolution of the radial motion of ions in a Penning trap during the application of radio-frequency fields leads to a systematic cyclotron frequency shift when more than one ion species is present in the trap during the cyclotron frequency measurement. An analytic expression was derived to correctly account for the shift. Cross-reference mass measurements with carbon-cluster ions have been performed providing the mass-dependent and residual uncertainties.


2021 ◽  
Vol 143 (12) ◽  
Author(s):  
Feng Wang ◽  
Zhenxing Sun ◽  
Wieslaw Fiebig ◽  
Bing Xu ◽  
Kim A. Stelson

Abstract A mathematical modeling approach to determine fluid film thickness on the vane tip in a vane pump transmission is developed. The transmission is based on a double-acting vane pump with an additional output shaft coupled to a floating ring. Owing to the floating ring design, the internal viscous friction helps to drive the output shaft, whereas the friction is turned into heat in a conventional vane pump. To study the mechanical efficiency, it is crucial to investigate the fluid film thickness between the vane tip and the ring inner surface. The modeling approach in this study takes the interactions between vane radial motion and chamber pressure dynamics into consideration, without using a computational fluid dynamics approach. The lubrication on the vane tip is considered as elasto-hydrodynamic lubrication and the fluid film thickness calculation is based on the Hooke lubrication diagram. Results show that the developed simulation model is capable of revealing the fluid film thickness change and vane radial motion in different operation regions. Sensitivity studies of several parameters on the minimum fluid film thickness are also presented.


2020 ◽  
Vol 46 (12) ◽  
pp. 3413-3425
Author(s):  
Xiaomin Liu ◽  
Yinong Wang ◽  
Peizhen Zhang ◽  
Qing Wang ◽  
Qianjin Feng ◽  
...  

2020 ◽  
Vol 222 (3) ◽  
pp. 1686-1703
Author(s):  
Colin M Hardy ◽  
Philip W Livermore ◽  
Jitse Niesen

SUMMARY Mounting evidence from both seismology and numerical experiments on core composition suggests the existence of a layer of stably stratified fluid at the top of Earth’s outer core. In such a layer, a magnetostrophic force balance and suppressed radial motion lead to stringent constraints on the magnetic field, named Malkus constraints, which are a much more restrictive extension of the well known Taylor constraints. Here, we explore the consequences of such constraints for the structure of the core’s internal magnetic field. We provide a new simple derivation of these Malkus constraints, and show solutions exist which can be matched to any external potential field with arbitrary depth of stratified layer. From considerations of these magnetostatic Malkus constraints alone, it is therefore not possible to uniquely infer the depth of the stratified layer from external geomagnetic observations. We examine two models of the geomagnetic field defined within a spherical core, which obey the Taylor constraints in an inner convective region and the Malkus constraints in an outer stratified layer. When matched to a single-epoch geomagnetic potential field model, both models show that the toroidal magnetic field within the outer layer is about 100 times stronger compared to that in the inner region, taking a maximum value of 8 mT at a depth of 70 km. The dynamic regime of such a layer, modulated by suppressed radial motion but also a locally enhanced magnetic field, may therefore be quite distinct from that of any interior dynamo.


2020 ◽  
Vol 34 (01) ◽  
pp. 1218-1225
Author(s):  
Chengqian Zhao ◽  
Cheng Feng ◽  
Dengwang Li ◽  
Shuo Li

Comprehensively analyzing the carotid artery is critically significant to diagnosing and treating cardiovascular diseases. The object of this work is to simultaneously achieve direct quantitative measurement and automated segmentation of the lumen diameter and intima-media thickness as well as the motion estimation of the carotid wall. No work has simultaneously achieved the comprehensive analysis of carotid artery due to three intractable challenges: 1) Tiny intima-media is more challenging to measure and segment; 2) Artifact generated by radial motion restrict the accuracy of measurement and segmentation; 3) Occlusions on diseased carotid walls generate dynamic complexity and indeterminacy. In this paper, we propose a novel optical flow-auxiliary multi-task regression network named OF-MSRN to overcome these challenges. We concatenate multi-scale features to a regression network to simultaneously achieve measurement and segmentation, which makes full use of the potential correlation between the two tasks. More importantly, we creatively explore an optical flow auxiliary module to take advantage of the co-promotion of segmentation and motion estimation to overcome the restrictions of the radial motion. Besides, we evaluate consistency between forward and backward optical flow to improve the accuracy of motion estimation of the diseased carotid wall. Extensive experiments on US sequences of 101 patients demonstrate the superior performance of OF-MSRN on the comprehensive analysis of the carotid artery by utilizing the dual optimization of the optical flow auxiliary module.


Nonlinearity ◽  
2020 ◽  
Vol 33 (5) ◽  
pp. 1987-2034 ◽  
Author(s):  
L Angela Mihai ◽  
Thomas E Woolley ◽  
Alain Goriely
Keyword(s):  

2020 ◽  
Author(s):  
Wiremu Hohaia ◽  
Blake W. Saurels ◽  
Alan Johnston ◽  
Kielan Yarrow ◽  
Derek H. Arnold

AbstractOne of the seminal findings of cognitive neuroscience is that the power of alpha-band (∼10 Hz) brain waves, in occipital regions, increases when people close their eyes. This has encouraged the view that alpha oscillations are a default dynamic, to which the visual brain returns in the absence of input. Accordingly, we might be unable to increase the power of alpha oscillations when the eyes are closed, above the level that would usually ensue. Here we report counter evidence. We used electroencephalography (EEG) to record brain activity when people had their eyes open and closed, before and after they had adapted to radial motion. The increase in the power of alpha oscillations when people closed their eyes was enhanced by adaptation to a broad range of radial motion speeds. This effect was greatest for 10Hz motion, but robust for other frequencies, and specifically for 7.5Hz. This last observation is important, as it rules against an ongoing entrainment of activity, at the adaptation frequency, as an explanation for our results. Instead, our data show that visual processes remain active when people close their eyes, and these can be modulated by adaptation to increase the power of alpha oscillations in occipital brain regions.


Measurement ◽  
2019 ◽  
Vol 137 ◽  
pp. 624-635 ◽  
Author(s):  
Hailong Cui ◽  
Dajiang Lei ◽  
Xinjiang Zhang ◽  
He Lan ◽  
Zhengyi Jiang ◽  
...  

2019 ◽  
Vol 27 (9) ◽  
pp. 2053-2061
Author(s):  
娄志峰 LOU Zhi-feng ◽  
郝秀朋 HAO Xiu-peng ◽  
刘 力 LIU Li ◽  
王晓东 WANG Xiao-dong

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