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1

Nagle, David P., and W. van Iterson. "Inner Structures of Bacteria." Transactions of the American Microscopical Society 104, no. 3 (July 1985): 310. http://dx.doi.org/10.2307/3226448.

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2

Huang, Ganglei, Wufei Si, and Cunbiao Lee. "Inner structures of Görtler streaks." Physics of Fluids 33, no. 3 (March 1, 2021): 034116. http://dx.doi.org/10.1063/5.0042769.

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3

Ivrii, Oleg. "Critical structures of inner functions." Journal of Functional Analysis 281, no. 8 (October 2021): 109138. http://dx.doi.org/10.1016/j.jfa.2021.109138.

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4

Berry, Jim, and Stanley McGreal. "Community and inter-agency structures in the regeneration of inner-city Belfast." Town Planning Review 66, no. 2 (April 1995): 129. http://dx.doi.org/10.3828/tpr.66.2.g5l52757r47x7662.

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5

Faraci, Carla, and Yong Liu. "ANALYSIS OF WAVE FORCES ACTING ON COMBINED CAISSONS WITH INNER SLOPE RUBBLE MOUND." Coastal Engineering Proceedings 1, no. 34 (October 28, 2014): 51. http://dx.doi.org/10.9753/icce.v34.structures.51.

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6

Auriault, Jean-Louis. "Inner thermal resonance in thermoelastic geological structures." Acta Geophysica 62, no. 5 (May 19, 2014): 993–1004. http://dx.doi.org/10.2478/s11600-014-0209-6.

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7

Stansby, D., and T. S. Horbury. "Number density structures in the inner heliosphere." Astronomy & Astrophysics 613 (May 2018): A62. http://dx.doi.org/10.1051/0004-6361/201732567.

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Aims. The origins and generation mechanisms of the slow solar wind are still unclear. Part of the slow solar wind is populated by number density structures, discrete patches of increased number density that are frozen in to and move with the bulk solar wind. In this paper we aimed to provide the first in-situ statistical study of number density structures in the inner heliosphere. Methods. We reprocessed in-situ ion distribution functions measured by Helios in the inner heliosphere to provide a new reliable set of proton plasma moments for the entire mission. From this new data set we looked for number density structures measured within 0.5 AU of the Sun and studied their properties. Results. We identified 140 discrete areas of enhanced number density. The structures occurred exclusively in the slow solar wind and spanned a wide range of length scales from 50 Mm to 2000 Mm, which includes smaller scales than have been previously observed. They were also consistently denser and hotter that the surrounding plasma, but had lower magnetic field strengths, and therefore remained in pressure balance. Conclusions. Our observations show that these structures are present in the slow solar wind at a wide range of scales, some of which are too small to be detected by remote sensing instruments. These structures are rare, accounting for only 1% of the slow solar wind measured by Helios, and are not a significant contribution to the mass flux of the solar wind.
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Kama, M., M. Min, and C. Dominik. "The inner rim structures of protoplanetary discs." Astronomy & Astrophysics 506, no. 3 (August 18, 2009): 1199–213. http://dx.doi.org/10.1051/0004-6361/200912068.

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9

Duyunova, Anna, Valentin Lychagin, and Sergey Tychkov. "Continuum mechanics of media with inner structures." Differential Geometry and its Applications 74 (February 2021): 101703. http://dx.doi.org/10.1016/j.difgeo.2020.101703.

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10

Mazėtis, E. "On inner tensor structures in Cartan spaces." Lithuanian Mathematical Journal 40, no. 2 (April 2000): 148–55. http://dx.doi.org/10.1007/bf02467154.

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11

Kobayashi, Keisuke, Takeshi Ota, Kenzo Maehashi, Hisao Nakashima, Yoichi Ishiwata, and Shik Shin. "Photoluminescence inner core excitation in semiconductor quantum structures." Physica E: Low-dimensional Systems and Nanostructures 7, no. 3-4 (May 2000): 595–99. http://dx.doi.org/10.1016/s1386-9477(99)00391-4.

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12

NAKAHARA, Hiroshi. "Surface Patterns and Inner Structures of Mollusc Shells." Hyomen Kagaku 15, no. 3 (1994): 184–88. http://dx.doi.org/10.1380/jsssj.15.184.

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13

Malaspina, D. M., L. Andersson, R. E. Ergun, J. R. Wygant, J. W. Bonnell, C. Kletzing, G. D. Reeves, R. M. Skoug, and B. A. Larsen. "Nonlinear electric field structures in the inner magnetosphere." Geophysical Research Letters 41, no. 16 (August 19, 2014): 5693–701. http://dx.doi.org/10.1002/2014gl061109.

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14

Glagolevskij, Yu V., and A. F. Nazarenko. "Probable Inner Magnetic Structures of Magnetic Stars. I." Astrophysical Bulletin 73, no. 2 (April 2018): 201–10. http://dx.doi.org/10.1134/s1990341318020062.

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15

Glagolevskij, Yu V., and A. F. Nazarenko. "Probable Inner Magnetic Structures of Magnetic Stars. II." Astrophysical Bulletin 75, no. 4 (October 2020): 440–46. http://dx.doi.org/10.1134/s1990341320040070.

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16

Daliri, Mohammad, Fabio Dentale, Daniela Salerno, and Mariano Buccino. "A CFD STUDY ON THE STRUCTURAL RESPONSE OF A SLOPING TOP CAISSON." Coastal Engineering Proceedings, no. 35 (June 23, 2017): 41. http://dx.doi.org/10.9753/icce.v35.structures.41.

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The paper discusses preliminary results of a CFD study on the structural response of a Sloping Top Breakwater subject to wave overtopping. The analysis showed that the transmitted wave field act to increase both the landward and the seaward forces and that the conventional design methods may be not adequate to guarantee an appropriate degree of safety to the structure. The study also confirmed the previous finding by Walkden et al. (2001), which noticed the existence of strong impulsive loadings on the inner face of the wall, due to violent overtopping events.
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17

Ciuman, R. R. "Stria vascularis and vestibular dark cells: characterisation of main structures responsible for inner-ear homeostasis, and their pathophysiological relations." Journal of Laryngology & Otology 123, no. 2 (June 23, 2008): 151–62. http://dx.doi.org/10.1017/s0022215108002624.

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AbstractThe regulation of inner-ear fluid homeostasis, with its parameters volume, concentration, osmolarity and pressure, is the basis for adequate response to stimulation. Many structures are involved in the complex process of inner-ear homeostasis. The stria vascularis and vestibular dark cells are the two main structures responsible for endolymph secretion, and possess many similarities. The characteristics of these structures are the basis for regulation of inner-ear homeostasis, while impaired function is related to various diseases. Their distinct morphology and function are described, and related to current knowledge of associated inner-ear diseases. Further research on the distinct function and regulation of these structures is necessary in order to develop future clinical interventions.
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18

Fernandez, Julia, Sol Alonso, Valeria Mesa, Fernanda Duplancic, and Georgina Coldwell. "Properties of galaxies with ring structures." Astronomy & Astrophysics 653 (September 2021): A71. http://dx.doi.org/10.1051/0004-6361/202141208.

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Aims. We present a statistical analysis of different characteristics of ringed spiral galaxies with the aim of assessing the effects of rings on disk galaxy properties. Methods. We built a catalog of ringed galaxies from the Sloan Digital Sky Survey Data Release 14 (SDSS-DR14). Via visual inspection of SDSS images, we classified the face-on spiral galaxies brighter than g < 16.0 mag into galaxies with: an inner ring, an outer ring, a nuclear ring, both an inner and an outer ring, and a pseudo-ring. In addition to rings, we recorded morphological types and the existence of bars, lenses, and galaxy pair companions with or without interaction. With the goal of providing an appropriate quantification of the influence of rings on galaxy properties, we also constructed a suitable control sample of non-ringed galaxies with similar redshift, magnitude, morphology, and local density environment distributions to those of ringed ones. Results. We found 1868 ringed galaxies, accounting for 22% of the full sample of spiral galaxies. In addition, within galaxies with ringed structures, 46% have an inner ring, 10% an outer ring, 20% both an inner and an outer ring, 6% a nuclear ring, and 18% a partial ring. Moreover, 64% of the ringed galaxies present bars. We also found that ringed galaxies have both a lower efficiency of star formation activity and older stellar populations (as derived with the Dn(4000) spectral index) with respect to non-ringed disk objects from the control sample. Moreover, there is a significant excess of ringed galaxies with red colors. These effects are more important for ringed galaxies that have inner rings and bars with respect to their counterparts that have some other types of rings and are non-barred. The color-magnitude and color-color diagrams show that ringed galaxies are mostly concentrated in the red region, while non-ringed spiral objects are more extended to the blue zone. Galaxies with ringed structures present an excess of high metallicity values compared to non-ringed ones, which show a 12 + Log(O/H) distribution toward lower values. These findings seem to indicate that rings are peculiar structures that produce an accelerating galactic evolution, strongly altering the physical properties of their host galaxies.
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19

TAKANO, Seiji. "Changing Spatial Structures of the Inner Cities in Japan." Kikan Chirigaku 56, no. 4 (2004): 225–40. http://dx.doi.org/10.5190/tga.56.225.

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20

Adunka, Oliver. "Preservation of Inner Ear Structures with a Promontory Cochleostomy." Otolaryngology–Head and Neck Surgery 131, no. 2 (August 2004): P266. http://dx.doi.org/10.1016/j.otohns.2004.06.553.

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21

Löhle, E., Ch Beck, J. Schölmerich, and U. Baumgartner. "The Influence of Portocaval Shunting on Inner Ear Structures." Pathology - Research and Practice 186, no. 1 (February 1990): 180–86. http://dx.doi.org/10.1016/s0344-0338(11)81028-9.

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22

Francis, J. T., and A. P. Hitchcock. "Distinguishing Keto and Enol Structures by Inner-Shell Spectroscopy." Journal of Physical Chemistry 98, no. 14 (April 1994): 3650–57. http://dx.doi.org/10.1021/j100065a018.

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23

Mosenkov, Aleksandr V., Anton A. Smirnov, Olga K. Sil’chenko, R. Michael Rich, Vladimir P. Reshetnikov, and John Kormendy. "Tilted outer and inner structures in edge-on galaxies?" Monthly Notices of the Royal Astronomical Society 497, no. 2 (July 3, 2020): 2039–56. http://dx.doi.org/10.1093/mnras/staa1885.

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ABSTRACT Tilted and warped discs inside tilted dark matter haloes are predicted from numerical and semi-analytical studies. In this paper, we use deep imaging to demonstrate the likely existence of tilted outer structures in real galaxies. We consider two SB0 edge-on galaxies, NGC 4469 and NGC 4452, which exhibit apparent tilted outer discs with respect to the inner structure. In NGC 4469, this structure has a boxy shape, inclined by ΔPA ≈ 3° with respect to the inner disc, whereas NGC 4452 harbours a discy outer structure with ΔPA ≈ 6°. In spite of the different shapes, both structures have surface brightness profiles close to exponential and make a large contribution (∼30 per cent) to the total galaxy luminosity. In the case of NGC 4452, we propose that its tilted disc likely originates from a former fast tidal encounter (probably with IC 3381). For NGC 4469, a plausible explanation may also be galaxy harassment, which resulted in a tilted or even a tumbling dark matter halo. A less likely possibility is accretion of gas-rich satellites several Gyr ago. New deep observations may potentially reveal more such galaxies with tilted outer structures, especially in clusters. We also consider galaxies, mentioned in the literature, where a central component (a bar or a bulge) is tilted with respect to the stellar disc. According to our numerical simulations, one of the plausible explanations of such observed ‘tilts’ of the bulge/bar is a projection effect due to a not exactly edge-on orientation of the galaxy coupled with a skew angle of the triaxial bulge/bar.
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24

Olsson, Johan D. M., and Stefan Oscarson. "Synthesis of phosphorylated Neisseria meningitidis inner core lipopolysaccharide structures." Tetrahedron: Asymmetry 20, no. 6-8 (May 2009): 875–82. http://dx.doi.org/10.1016/j.tetasy.2009.02.017.

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25

Ruan, Zhongyuan, Ming Tang, Changgui Gu, and Jinshan Xu. "Epidemic spreading between two coupled subpopulations with inner structures." Chaos: An Interdisciplinary Journal of Nonlinear Science 27, no. 10 (October 2017): 103104. http://dx.doi.org/10.1063/1.4990592.

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26

Adunka, Oliver, Wolfgang Gstoettner, Markus Hambek, Marc H. Unkelbach, Andreas Radeloff, and Jan Kiefer. "Preservation of Basal Inner Ear Structures in Cochlear Implantation." ORL 66, no. 6 (2004): 306–12. http://dx.doi.org/10.1159/000081887.

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27

Sula, Altin, Ambrose R. Cole, Corin Yeats, Christine Orengo, and Nicholas H. Keep. "Crystal structures of the human Dysferlin inner DysF domain." BMC Structural Biology 14, no. 1 (2014): 3. http://dx.doi.org/10.1186/1472-6807-14-3.

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28

Geneci, Ferhat, Muhammet Bora Uzuner, Burak Bilecenoğlu, Bilge İpek Torun, Kaan Orhan, and Mert Ocak. "Examination of inner ear structures: a micro-CT study." Acta Oto-Laryngologica 142, no. 1 (January 2, 2022): 1–5. http://dx.doi.org/10.1080/00016489.2021.2015078.

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29

Kelly, S. Graham. "Free and Forced Vibrations of Elastically Connected Structures." Advances in Acoustics and Vibration 2010 (January 2, 2010): 1–11. http://dx.doi.org/10.1155/2010/984361.

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A general theory for the free and forced responses of elastically connected parallel structures is developed. It is shown that if the stiffness operator for an individual structure is self-adjoint with respect to an inner product defined for , then the stiffness operator for the set of elastically connected structures is self-adjoint with respect to an inner product defined on . This leads to the definition of energy inner products defined on . When a normal mode solution is used to develop the free response, it is shown that the natural frequencies are the square roots of the eigenvalues of an operator that is self-adjoint with respect to the energy inner product. The completeness of the eigenvectors in is used to develop a forced response. Special cases are considered. When the individual stiffness operators are proportional, the problem for the natural frequencies and mode shapes reduces to a matrix eigenvalue problem, and it is shown that for each spatial mode there is a set of intramodal mode shapes. When the structures are identical, uniform, or nonuniform, the differential equations are uncoupled through diagonalization of a coupling stiffness matrix. The most general case requires an iterative solution.
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30

Rebielak, Janusz. "Space Structures — Proposals for Shaping." International Journal of Space Structures 7, no. 3 (September 1992): 175–90. http://dx.doi.org/10.1177/026635119200700301.

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The tendency to the individual shaping of an architectural view of space structures leads sometimes to the search for new arrangements of component parts of these structures and their reciprocal juxtapositions. The merger procedure of these elements determines a geometric form of the inner construction of a given space structure and technical conditions connected with its application. This paper presents, having in mind architectural advantages, some examples of geometrical shaping of the inner construction of multi-layer space structures and some proposals of their application as structures for large span covers. The systems presented of the proposed space frameworks were obtained by help of modification of a bar arrangement within chosen symmetric modular sets of a certain group of space structures. The application proposals of the presented group of space structures were shown mainly on examples of spherical covers.
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31

Hasse, A., I. Zuest, and L. F. Campanile. "Modal synthesis of belt-rib structures." Proceedings of the Institution of Mechanical Engineers, Part C: Journal of Mechanical Engineering Science 225, no. 3 (September 10, 2010): 722–32. http://dx.doi.org/10.1243/09544062jmes2329.

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In contrast to conventional mechanisms, compliant mechanisms exploit structural flexibility to produce controllable large deformations. Belt-rib airfoils are shape-adaptable lightweight structures based on this idea. A belt-rib structure originally consists of a deformable closed shell (belt) whose kinematic degrees of freedom are constrained by inner stiffeners called spokes. Using standard spoke elements, the possible profile changes of the airfoil are limited. The purpose of the work reported in the current article is to define an inner stiffening structure based on numerical topology optimization in order to realize arbitrary profile changes. A ground structure with moveable connection points within the external belt represents the set of possible topologies and shapes. A new modal objective function for the synthesis of compliant mechanisms with selective compliance is introduced. The optimization problem is approached by using genetic algorithms. The applicability of the current procedure is validated by a profile shape adaptation example. For this purpose, an initial profile shape and a target profile shape are defined. The outcome of the procedure is a complex inner stiffening structure, which fulfils the imposed requirements. The solution is validated by modal analysis based on an finite-element model. Furthermore, the structural behaviour is experimentally investigated.
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32

Ulug, T. "Using the processus cochleariformis as a multipurpose landmark in middle cranial fossa surgery." Journal of Laryngology & Otology 123, no. 2 (May 20, 2008): 163–69. http://dx.doi.org/10.1017/s0022215108002697.

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AbstractObjective:To demonstrate that the anatomical structure known as the processus cochleariformis, with its intimate and constant relationships to inner-ear structures, can be used as a reliable landmark during middle cranial fossa surgery, alone or in conjunction with other landmarks.Study design:An anatomical study using cadaveric temporal bones to define six reproducible measurements that relate the processus cochleariformis to inner-ear structures, and to define 14 other measurements that relate inner-ear structures to adjacent structures within the intact bone.Method:Using 10 cadaver specimens, 20 reproducible measurements were defined. The first six of these defined the relation of the processus cochleariformis to inner-ear structures in the middle cranial fossa approach. The other measurements defined the exact location of the inner-ear structures and adjacent structures within the intact bone.Results:The vertical crest lies at a 20° angle from the processus cochleariformis to the coronal plane, and at a distance of 5 to 6 mm from the processus cochleariformis. The point at which the medial margin of the basal turn of the cochlea crosses the labyrinthine segment of the facial nerve lies at a 0° angle from the processus cochleariformis to the coronal plane, and at a distance of 6.5 to 7.5 mm from the processus cochleariformis. The superior semicircular canal lies at a 45° angle from the processus cochleariformis to the coronal plane. The other measurements obtained give important clues about the position of the cochlea, vestibulum, greater superficial petrosal nerve and labyrinthine segment of the facial nerve.Conclusions:If the classical landmarks are indiscernible during middle cranial fossa surgery, then the processus cochleariformis, with its intimate and constant relationships to inner-ear structures, is a safe and constant landmark.
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33

Ringel, Aron, and Johannes Lohmar. "Optimization of the Surface Geometry in Structured Cold Rolling for Interlocking of Formed and Die-Cast Metal Components." Defect and Diffusion Forum 414 (February 24, 2022): 89–94. http://dx.doi.org/10.4028/p-z54p05.

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Modern lightweight design is often based on multi-material components. For example, structured sheet metals can be equipped with a die-cast light metal insert for structural support. To interlock sheet and insert, structures with undercuts are formed into the sheet in a multi-pass rolling process. In a first pass, structured rolls are used to create a structure of channels and ribs. Undercuts are formed in a consecutive pass by flat rolling those ribs. During die-casting, the melt flows into the channels and forms an interlocking connection once solidified. The joint strength is decisively determined by the undercut geometry. The undercuts formed by material displacement increase with the height reduction in the flat rolling pass. However, after a certain amount of material displacement, the channel side edge starts to fold over the channel bottom and forms an inner notch. Those inner notches can be prone to crack initiation and subsequently lead to component failure. To analyze the surface structure regarding channel depth, undercuts and inner notches as well as finally maximize the joint strength, a combined experimental and numerical study was laid out. The surface of 2.0 mm DC04 was structured with up to 0.5 mm deep channels and then flattened with different height reductions. The results from the 2D explicit FE-model suggest that a process optimum for those surface structures with high undercut width but without inner notch exists at 14% height reduction. However, in the experiments inner notches started to form at approx. 8% height reduction with approx. 20 µm wide undercuts for the given experimental setup. In contrast, maximum undercuts of approx. 50 µm form at 26% height reduction, but also cause inner notches with approx. 60 µm length.
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34

Li, Chuxin, Haoyu Dai, Can Gao, Ting Wang, Zhichao Dong, and Lei Jiang. "Bioinspired inner microstructured tube controlled capillary rise." Proceedings of the National Academy of Sciences 116, no. 26 (June 10, 2019): 12704–9. http://dx.doi.org/10.1073/pnas.1821493116.

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Effective, long-range, and self-propelled water elevation and transport are important in industrial, medical, and agricultural applications. Although research has grown rapidly, existing methods for water film elevation are still limited. Scaling up for practical applications in an energy-efficient way remains a challenge. Inspired by the continuous water cross-boundary transport on the peristome surface ofNepenthes alata, here we demonstrate the use of peristome-mimetic structures for controlled water elevation by bending biomimetic plates into tubes. The fabricated structures have unique advantages beyond those of natural pitcher plants: bulk water diode transport behavior is achieved with a high-speed passing state (several centimeters per second on a milliliter scale) and a gating state as a result of the synergistic effect between peristome-mimetic structures and tube curvature without external energy input. Significantly, on further bending the peristome-mimetic tube into a “candy cane”-shaped pipe, a self-siphon with liquid diode behavior is achieved. Such a transport mechanism should inspire the design of next generation water transport devices.
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35

Kuo, H.-C., L.-Y. Lin, C.-P. Chang, and R. T. Williams. "The Formation of Concentric Vorticity Structures in Typhoons." Journal of the Atmospheric Sciences 61, no. 22 (November 1, 2004): 2722–34. http://dx.doi.org/10.1175/jas3286.1.

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Abstract An important issue in the formation of concentric eyewalls in a tropical cyclone is the development of a symmetric structure from asymmetric convection. It is proposed herein, with the aid of a nondivergent barotropic model, that concentric vorticity structures result from the interaction between a small and strong inner vortex (the tropical cyclone core) and neighboring weak vortices (the vorticity induced by the moist convection outside the central vortex of a tropical cyclone). The results highlight the pivotal role of the vorticity strength of the inner core vortex in maintaining itself, and in stretching, organizing, and stabilizing the outer vorticity field. Specifically, the core vortex induces a differential rotation across the large and weak vortex to strain out the latter into a vorticity band surrounding the former. The straining out of a large, weak vortex into a concentric vorticity band can also result in the contraction of the outer tangential wind maximum. The stability of the outer band is related to the Fjørtoft sufficient condition for stability because the strong inner vortex can cause the wind at the inner edge to be stronger than the outer edge, which allows the vorticity band and therefore the concentric structure to be sustained. Moreover, the inner vortex must possess high vorticity not only to be maintained against any deformation field induced by the outer vortices but also to maintain a smaller enstrophy cascade and to resist the merger process into a monopole. The negative vorticity anomaly in the moat serves as a “shield” or a barrier to the farther inward mixing the outer vorticity field. The binary vortex experiments described in this paper suggest that the formation of a concentric vorticity structure requires 1) a very strong core vortex with a vorticity at least 6 times stronger than the neighboring vortices, 2) a large neighboring vorticity area that is larger than the core vortex, and 3) a separation distance between the neighboring vorticity field and the core vortex that is within 3 to 4 times the core vortex radius.
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36

Sánchez-Arcilla, Agustín, Manuel Espino, Manel Grifoll, Cesar Mösso, Joan Pau Sierra, Marc Mestres, Stella Spyropoulou, et al. "QUAY DESIGN AND OPERATIONAL OCEANOGRAPHY. THE CASE OF BILBAO HARBOUR." Coastal Engineering Proceedings 1, no. 32 (February 1, 2011): 51. http://dx.doi.org/10.9753/icce.v32.structures.51.

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In this paper a harbour engineering application of an operational system to forecast circulation and transport fields is presented. It deals with the functional design of a quay in the Bilbao harbour (Bay of Biscay, North-Atlantic coast of Spain). The aim is to use physical oceanography “tools” to design the optimal quay alignment according to two criteria: i) Minimize the currents in order to guarantee the vessel maneuverability and quay operability for given safety levels and ii) Maximize the water renewal capacity of the harbour inner basins (beyond the studied quay) in order to reduce the risk of water quality degradation. The methodology and the results reveal a new procedure to enhance the harbour lay-out design from an environment point of view.
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37

Mutoh, Hideki. "3-D Wave Optical Simulation of Inner-Layer Lens Structures." Journal of the Institute of Image Information and Television Engineers 54, no. 2 (2000): 210–15. http://dx.doi.org/10.3169/itej.54.210.

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38

Chen, James. "An advanced kinetic theory for morphing continuum with inner structures." Reports on Mathematical Physics 80, no. 3 (December 2017): 317–32. http://dx.doi.org/10.1016/s0034-4877(18)30004-1.

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39

Heinrich, Lothar, Hendrik Schmidt, and Volker Schmidt. "Limit theorems for stationary tessellations with random inner cell structures." Advances in Applied Probability 37, no. 01 (March 2005): 25–47. http://dx.doi.org/10.1017/s0001867800000021.

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We consider stationary and ergodic tessellations X = Ξ n n≥1 in R d , where X is observed in a bounded and convex sampling window W p ⊂ R d . It is assumed that the cells Ξ n of X possess random inner structures, examples of which include point patterns, fibre systems, and tessellations. These inner cell structures are generated, both independently of each other and independently of the tessellation X, by generic stationary random sets that are related to a stationary random vector measure J 0 acting on R d . In particular, we study the asymptotic behaviour of a multivariate random functional, which is determined both by X and by the individual cell structures contained in W p , as W p ↑ R d . It turns out that this functional provides an unbiased estimator for the intensity vector associated with J 0. Furthermore, under natural restrictions, strong laws of large numbers and a multivariate central limit theorem of the normalized functional are proven. Finally, we discuss in detail some numerical examples and applications, for which the inner structures of the cells of X are induced by iterated Poisson-type tessellations.
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40

Manssour, Isabel H., Luiz Gustavo Fernandes, Carla Maria Freitas, Gustavo Serra, and Thiago Nunes. "High performance approach for inner structures visualisation in medical data." International Journal of Computer Applications in Technology 22, no. 1 (2005): 23. http://dx.doi.org/10.1504/ijcat.2005.006800.

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41

Di Giovannantonio, Marco, Xuelin Yao, Kristjan Eimre, José I. Urgel, Pascal Ruffieux, Carlo A. Pignedoli, Klaus Müllen, Roman Fasel, and Akimitsu Narita. "Large-Cavity Coronoids with Different Inner and Outer Edge Structures." Journal of the American Chemical Society 142, no. 28 (June 26, 2020): 12046–50. http://dx.doi.org/10.1021/jacs.0c05268.

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42

Vivas, A. K., R. Zinn, S. Duffau, and Y. Jaffé. "Sub-structures in the inner halo of the Milky Way." EPJ Web of Conferences 19 (2012): 02007. http://dx.doi.org/10.1051/epjconf/20121902007.

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43

Chuang, Ming-Tsung, I.-Chan Chiang, Gin-Chung Liu, and Wei-Chen Lin. "Multidetector row CT demonstration of inner and middle ear structures." Clinical Anatomy 19, no. 4 (2006): 337–44. http://dx.doi.org/10.1002/ca.20213.

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44

Jiang, Shulan, Tielin Shi, Zirong Tang, and Shuang Xi. "Cost-Effective Fabrication of Inner-Porous Micro/Nano Carbon Structures." Journal of Nanoscience and Nanotechnology 18, no. 3 (March 1, 2018): 2089–95. http://dx.doi.org/10.1166/jnn.2018.14256.

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45

Heinrich, Lothar, Hendrik Schmidt, and Volker Schmidt. "Limit theorems for stationary tessellations with random inner cell structures." Advances in Applied Probability 37, no. 1 (March 2005): 25–47. http://dx.doi.org/10.1239/aap/1113402398.

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Abstract:
We consider stationary and ergodic tessellations X = Ξnn≥1 in Rd, where X is observed in a bounded and convex sampling window Wp ⊂ Rd. It is assumed that the cells Ξn of X possess random inner structures, examples of which include point patterns, fibre systems, and tessellations. These inner cell structures are generated, both independently of each other and independently of the tessellation X, by generic stationary random sets that are related to a stationary random vector measure J0 acting on Rd. In particular, we study the asymptotic behaviour of a multivariate random functional, which is determined both by X and by the individual cell structures contained in Wp, as Wp ↑ Rd. It turns out that this functional provides an unbiased estimator for the intensity vector associated with J0. Furthermore, under natural restrictions, strong laws of large numbers and a multivariate central limit theorem of the normalized functional are proven. Finally, we discuss in detail some numerical examples and applications, for which the inner structures of the cells of X are induced by iterated Poisson-type tessellations.
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Pauna, Henrique F., Rafael C. Monsanto, Natsuko Kurata, Michael M. Paparella, and Sebahattin Cureoglu. "Changes in the inner ear structures in cystic fibrosis patients." International Journal of Pediatric Otorhinolaryngology 92 (January 2017): 108–14. http://dx.doi.org/10.1016/j.ijporl.2016.11.013.

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Cor, J. J., and T. F. Miller. "Theoretical analysis of hydrostatic implodable volumes with solid inner structures." Journal of Fluids and Structures 25, no. 2 (February 2009): 284–303. http://dx.doi.org/10.1016/j.jfluidstructs.2008.04.003.

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48

Chen, C. S., and L. M. Anderson. "The inner ear structures of the echidna—An SEM study." Experientia 41, no. 10 (October 1985): 1324–26. http://dx.doi.org/10.1007/bf01952077.

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49

Hamhalter, Jan, and Ekaterina Turilova. "Subspace Structures in Inner Product Spaces and von Neumann Algebras." International Journal of Theoretical Physics 50, no. 12 (January 19, 2011): 3812–20. http://dx.doi.org/10.1007/s10773-011-0665-6.

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Krasnoshchekov, Dmitry, Petr Kaazik, Elena Kozlovskaya, and Vladimir Ovtchinnikov. "Seismic Structures in the Earth’s Inner Core Below Southeastern Asia." Pure and Applied Geophysics 173, no. 5 (February 20, 2016): 1575–91. http://dx.doi.org/10.1007/s00024-015-1207-6.

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