Relevant bibliographies by topics / Wiggles

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  2. Dissertations / Theses
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Academic literature on the topic 'Wiggles'

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Published: 4 June 2021
Last updated: 5 February 2022

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Journal articles on the topic "Wiggles"

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Geel, Bas Van, and Willem G. Mook. "High-Resolution 14C Dating of Organic Deposits Using Natural Atmospheric 14C Variations." Radiocarbon 31, no. 2 (1989): 151–55. http://dx.doi.org/10.1017/s0033822200044805.

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The occurrence of atmospheric 14C variations complicates calibration, ie, the translation of 14C ages into real calendar ages. The procedure of wiggle matching, however, allows very precise calibration, by matching known 14C variations with wiggles in the floating chronology. In principle, wiggle matching can also be applied to a series of 14C dates from organic (peat) deposits. Where, in general, 14C ages are required at short distances and on small samples, dating by 14C accelerator mass spectrometry (AMS) is required.
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Dretske, Fred. "The Metaphysics Of Freedom." Canadian Journal of Philosophy 22, no. 1 (March 1992): 1–13. http://dx.doi.org/10.1080/00455091.1992.10717268.

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I offer Jimmy a dollar to wiggle his ears. He wiggles them because he wants the dollar and, as a result of my offer, thinks he will earn it by wiggling his ears. So I cause him to believe something that explains, or helps to explain, why he wiggles his ears. If I push a button, and a bell, wired to the button, rings because the button is depressed, I cause the bell to ring. I make it ring. Indeed, I ring it. So why don’t I, by offering him a dollar, make Jimmy wiggle his ears? Why, indeed, don’t I wiggle them? If I ring a bell by pushing a button, why don’t I wiggle Jimmy’s ears by offering him a dollar?That is a question that has always vexed a compatibilist’s vision of human freedom. If an intentional act–say, wiggling one’s ears in order to earn a dollar–is caused by one’s beliefs and desires (the reasons one has for wiggling one’s ears), then, by the transitivity of the causal relation, it appears to follow that it is (also) caused by whatever causes one to have those beliefs and desires. But the causes of belief and desire are often (in fact, if we trace the causal chain far enough backward, always) factors over which one has no control. So intentional behavior is often (or always) something one is made (caused) to do by factors over which one has no control. This, however, robs intentional behaviorand, presumably, also voluntary action–of its autonomy. Deliberate acts–Jimmy wiggling his ears to earn a dollar–have the same causal structure as does a bell that rings because a button is pushed. The only difference is the switch.
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Georgescu, Iulia. "Waves and wiggles." Nature Physics 9, no. 8 (August 2013): 459. http://dx.doi.org/10.1038/nphys2720.

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Liu, Pei-Ling, Tseng-Hwa Song, and Tsung-Tsong Wu. "Application of System Identification to the Absolute Calibration of Acoustic Emission Signals." Journal of Vibration and Acoustics 116, no. 4 (October 1, 1994): 562–66. http://dx.doi.org/10.1115/1.2930464.

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This paper studies the absolute calibration of acoustic emission signals. The experiments were conducted on a thin plate. Fracture of a glass capillary was adopted to generate a vertical force with a unit-step source function, and an NBS conical transducer was used to record the surface response. It is found that the output of the conical transducer contains surplus wiggles and exhibits amplitude decay. The system identification method is introduced to determine the dynamic model of the system. Calibration using the system model successfully recovers the amplitude and greatly suppresses the surplus wiggles. The method is further improved by subtracting the characteristic curve of the wiggles from the experimental data before the system identification approach is carried out.
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Siddiqi, Kaleem, Benjamin B. Kimia, Allen Tannenbaum, and Steven W. Zucker. "Shapes, shocks and wiggles." Image and Vision Computing 17, no. 5-6 (April 1999): 365–73. http://dx.doi.org/10.1016/s0262-8856(98)00130-9.

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Giuffre, Liz. "Top of the Tots: The Wiggles as Australia's Most Successful (Under-Acknowledged) Sound Media Export." Media International Australia 148, no. 1 (August 2013): 145–54. http://dx.doi.org/10.1177/1329878x1314800116.

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The Wiggles produce hugely successful CDs, DVDs and interactive entertainment for pre-school children. They are Top of the Tots, as their 2004 album of the same name proclaims. However, the artists have been largely overlooked by the popular music and media academies. I argue that this omission can be attributed to problems of categorisation, particularly existing frameworks in television studies that limit how we gauge ‘quality entertainment’ and its audience; and in popular music and sound studies traditions that are yet to formally engage with listeners who are of pre-school age. The Wiggles are artists whose target audience historically has been overlooked by sophisticated, diverse and evolving academic traditions. As a result, their pioneering cross-media and international successes have largely been ignored. In this article, I seek to explore The Wiggles in terms that go beyond the narrow parameters of ‘children's entertainment’, offering more ‘grown-up’ ways to understand the group's success.
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Li HUANG, Huei, and Hsiao-Ping TSENG. "WIGGLES IN THIN FILM HEADS." Journal of the Magnetics Society of Japan 15, S_2_PMRC_91 (1991): S2_191–195. http://dx.doi.org/10.3379/jmsjmag.15.s2_191.

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Carlin, J. L., H. J. Newberg, L. Deng, J. Delaunay, D. Gole, K. Grabowski, C. Liu, Y. Xu, F. Yang, and H. Zhang. "Nearby kinematic wiggles from LEGUE." Proceedings of the International Astronomical Union 9, S298 (May 2013): 397. http://dx.doi.org/10.1017/s1743921313006649.

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In its first two observing seasons, the LEGUE (LAMOST Experiment for Galactic Understanding and Exploration; Deng et al., Zhao et al. 2012) survey has obtained ~1.7 million science-quality spectra. We apply corrections to the PPMXL proper motions (PMs; Roeser et al. 2010) as a function of position, as determined from the measured PMs of extragalactic objects discovered in LAMOST spectra (see Fig. 1, left and center panels). LAMOST radial velocities and corrected PMs are used to derive 3D space velocities for ~480,000 F-stars (assuming MV=4 to derive distances). The right panel of Fig. 1 shows the radial component of Galactic cylindrical velocities (VR) for stars between 7.8<RGC<9.8 kpc (with R⊙,GC=7.8 kpc) as a function of height (Z) and angle (θ) from the Galactic X-axis. Each dot represents the average position of stars in a 200x200 pc box, color-coded by the mean VR of those stars. Assuming circularrotation, VR should be zero. This is true on average for θ>0° (3rd Galactic quadrant), but not for θ<0°. The velocities are also asymmetric across the Galactic plane for θ<0° (2nd quadrant), with most positions 〈 VR 〉> 0 above the disk (radially outward), and 〈 VR 〉 < 0 below the disk. Similar structure to this apparent “shearing” motion has been seen in RAVE (e.g., Williams et al. 2013; Siebert et al. 2012), and SDSS (Widrow et al. 2012).
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Dio, Enea Di. "Lensing smoothing of BAO wiggles." Journal of Cosmology and Astroparticle Physics 2017, no. 03 (March 9, 2017): 016. http://dx.doi.org/10.1088/1475-7516/2017/03/016.

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TRUSKINOVSKY, L., and G. ZANZOTTO. "Ericksen's bar revisited : Energy wiggles." Journal of the Mechanics and Physics of Solids 44, no. 8 (August 1996): 1371–408. http://dx.doi.org/10.1016/0022-5096(96)00020-8.

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Dissertations / Theses on the topic "Wiggles"

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Lehmann, Sharon Fincher. ""Wiggles and Volcanos": an Investigation of Children's Graphing Responses to Music." Thesis, University of North Texas, 1993. https://digital.library.unt.edu/ark:/67531/metadc278601/.

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The purpose of this study was to investigate changes in selected children's Graphing Response Patterns to elemental changes in compositions in theme and variation form. The research problems were (1) to determine points and degrees of elemental change in the compositional structure of the musical examples; (2) to determine number, degree, and nature of changes in subjects' graphing response pattern to aurally presented musical examples; (3) to determine percentages of agreement between changes in graphing response patterns and points of elemental change within the compositional structures; (4) to determine the relationship of changes in subjects' graphing response pattern to the quality and magnitude of elemental change within the compositional structure. Twenty second- and fourth-grade children were individually videotaped as they listened to and graphed a series of aurally-presented musical examples. Each musical example was analysed according to such parameters as timbre, range/interval size, texture, tempo/meter, attack/rhythmic density, key/mode, dynamic level, and melodic presentation. Change in each parameter was scored using an interval scale reflecting change/no change and degree of change. Changes in graphing response pattern were determined by an interval scale which reflected the presence of change/no change and amount of change, using as analytical units speed, size, shape, type, and pause. The following conclusions were made: findings showed an observable, quantifiable relationship between changes in children's graphing response patterns and elemental changes in music parameters. This relationship encompassed not only change/no change judgements but also magnitude of response. Overall, frequency and magnitude/degree of student response was proportionate to the frequency and magnitude of change in the music parameter/s. Results indicated the existence of high-ranking correlations between student response and certain parameters regardless of the degree-of-change/points-of-change ratio. Findings showed that one degree of change in a single music parameter was not sufficient to cause an observable change in the attention of the young listener.
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Orban, Christopher M. "Powerlaws, Bumps and Wiggles: Self-Similar Models in the Era of Precision Cosmology." The Ohio State University, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=osu1299614704.

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Abualrob, Hadil. "Construction et études de wigglers à SOLEIL : W164 et wiggler Robinson." Thesis, Paris 11, 2015. http://www.theses.fr/2015PA112213.

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Es centres de rayonnement synchrotron sont des accélérateurs de particules qui génèrentun faisceau de lumière bien intense et collimaté en courbant la trajectoire d'un faisceau d´électronrelativiste. Le champ le plus simple utilisé pour courber la trajectoire d'un électron est unchamps magnétique constant généré par un dipôle. Des rayonnements plus intense peuventêtre émis dans une insertion. Une insertion est composée d'une séries de dipôle de polaritésinverses. Les insertions comprennent en général deux types : onduleurs et wigglers. Leswigglers sont très importants pour une source de rayonnement synchrotron. Ils peuvent êtreutilisé pour objectives différents, comme moduler le structure temporel de paquets d´électron,la production de faisceau de photon de haut énergie et réduire la taille transverse de faisceau.Ce travail est consacré pour l´étude de deux wigglers différent pour deux objective différents :le wiggler W164 et wiggler Robinson. Le W164 a étéconstruit pour la production des impulsionsde courte durée (femtosecond ) en utilisant le principe de femtoslicing. Dans le principede femtoslicing, si un faisceau d´électron se propage avec un faisceau de laser de durée defemtosecond dans le wiggler, ce dernier fait le rôle d'un modulateur qui extrait un “ slice “du paquet de durée de femtosecond qui émet à son tour un rayonnement X de durée de femtosecond.En plus, W164 fait un autre rôle d' une source rayonnement de photon des hautsénergies pour une autre ligne de lumière. La deuxième partie de ce travail est dédiée à l´étude d'unwiggler Robinson pour réduire l´emittance horizontal. L'effet Robinson à été étudié et observéexpérimentalement à SOLEIL avant la construction de wiggler. Les résultats sont présentés.Un pré-design a été aussi proposé
Synchrotron light sources are particle accelerators that generate intense and highly collimatedradiation by bending the trajectory of a relativistic electron beam. The most commonsimple field used to deflect a relativistic electron beam trajectory is a constant magnetic fieldgenerated by bending magnet. More intense radiation can produced through insertion devices.An insertion device is made by combining short bending magnets of opposite polarities. Theyinclude in general two types: undulators and wigglers. Wigglers play an important role ina synchrotron radiation source, since they can be employed for different objectives such asmodulating the time structure of the electron bunch, generating high energy photons, andreducing the transverse beam size. This work studies two different wigglers for different purposes:W164 and Robinson wiggler. The wiggler W164 was constructed for the production offemtosecond light pulses based on the femtoslicing principle. Femtoslicing implies that if anelectron beam co-propagates through the wiggler with a femtosecond laser pulse, the wiggleracts on the electron beam as a modulator and extracts a femtosecond slice of the bunch thatcreates in turn a femtosecond X-ray pulse. Moreover, the W164 plays another role of being ahigh energy photon source for another beamline. The second topic studied here is reducing thehorizontal emittance by using Robinson wiggler. Robinson effect was studied and observedexperimentally at SOLEIL before the wiggler construction. A preliminary wiggler design isproposed
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Tuček, Marek. "Frekvenční rapid-scan EPR na organických radikálech." Master's thesis, Vysoké učení technické v Brně. Fakulta strojního inženýrství, 2018. http://www.nusl.cz/ntk/nusl-382258.

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Tato práce popisuje historicky první multi-frekvenční rapid-scan EPR. Při zavedení mikrovlnného záření z oblasti 200 GHz a následnou sinusovou modulací bylo dosaženo rychlostí změn frekvence až 61 500 THz/s a zkreslení spekter, známé jako ”wiggles”, bylo pozorováno u obou studovaných vzorků organických radikálů – BDPA v polystyrenové matici a LiPc. Tato práce představuje flexibilní metodu provádění rapid-scan EPR experimentů za použití napětím ovládaného oscilátoru (Voltage Controlled Oscillator; VCO) jako zdroje a zero-bias detektoru (ZBD) pro detekci, čímž se otevírá možnost postupu dále do oblastí vyšších polí / vyšších frekvencí. Dále je popsán postup získání ustáleného spektra z rapid-scan výsledků, známý jako Fourierovská dekonvoluce, a dále je zjistěn spinový dekoherenční čas vzorků pomocí srovnání experimentálních spekter s výsledky numericky vyřešených Blochových rovnic. Výsledné hodnoty jsou 50 ns pro BDPA a 12 ns pro LiPc.
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Kneip, Stefan. "Laser plasma accelerator and wiggler." Thesis, Imperial College London, 2010. http://hdl.handle.net/10044/1/5671.

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This thesis details experimental research of laser-driven electron acceleration from underdense plasmas and the characterisation of the x-ray radiation owing to the transverse oscillatory motion that electrons perform during the acceleration process. Acceleration of monoenergetic electron beams to the GeV level was achieved for the first time in a self-guiding, self-injecting wakefield accelerator in the nonlinear regime, driven by the 200 TW Astra Gemini laser. The laser pulse was shown to be self-guided for 1 cm or more than ten times its Rayleigh range, by measurement of a single filament containing > 30% of the initial laser energy at this distance. The intensity in the guided filament is amplified beyond its initial value, as suggested by the GeV electron energy gain. Three dimensional numerical modeling is in excellent agreement with the experimental findings. In this regime, a beam of tens of keV x-rays emanating from a micrometer source with milliradian divergence, spatial coherence and a peak brightness comparable to third generation light sources was measured on experiments with the 100 TW Hercules laser. The measurements show that, due to their small transverse oscillations, the electron trajectories and their radiation properties resemble the scenario of an electron in a wiggler-type insertion device, with a strength parameter K close to 1. The experimental findings are supported by three dimensional modeling of the electron and x-ray beam. Betatron radiation was also measured with ten times longer and more intense pulses from the Vulcan Petawatt laser. In this case, electron acceleration is strongly driven transversely by the laser and a betatron resonance leads to a tenfold increase in oscillation amplitude. This alters the characteristics of the emitted synchrotron radiation fundamentally, increasing 50-fold the strength parameter and divergence, 10-fold the source size and up to 5-fold the x-ray energy, thereby broadening the electron energy distribution and converting up to 5% of their energy into x-rays. The studies provide evidence for the scalability of self-guided laser wakefield accelerators from 0.1 to 1 GeV. Furthermore the work demonstrates that betatron radiation can help to understand the acceleration process and has characteristics comparable to conventional synchrotron light.
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Garcia, Perez Oscar Armando. "Condicionamento espectral da luz de um Wiggler." [s.n.], 1995. http://repositorio.unicamp.br/jspui/handle/REPOSIP/277361.

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Orientador: Antonio Rubens Britto de Castro
Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Fisica "Gleb Wataglin"
Made available in DSpace on 2018-07-20T21:46:26Z (GMT). No. of bitstreams: 1 GarciaPerez_OscarArmando_M.pdf: 1340646 bytes, checksum: 9bc8d75a0d4a71f3107692ab482e7e67 (MD5) Previous issue date: 1995
Resumo: Esta tese descreve o projeto de um sistema de filtros de carbono, a ser instalado nas linhas de wiggler do Laboratório Nacional de Luz Sincrotron (LNLS). O sistema compõe-se de seis películas, com uma densidade superficial total x=61627mg/cm2, tendo uma transmissão de 75% em 8 K e V. Analisou-se a influência das impurezas e demostrou-se que seu efeito é desprezível. Foram realizadas simulações com o programa de elementos finitos MODULEF, para predizer o comportamento termo-mecânico das películas, a tensão máxima está perto do limiar de segurança. O sistema de filtros será montado alterando um componente padrão dos "front-ends" nas linhas de luz, a chamada máscara refrigerada
Abstract: This thesis describes a project of carbon filters system, which will be installed in the wiggler ljnes of the National Laboratory of Sinchrotron Light (LNLS). The system consist of six films, with a total surface density of x = 61627 m g / cm2 , possessing a transmition of 75% at 8 K e V. The influence of impurities was analyzed showing that its effect is inmaterial. Simulations were carried out with the program of finit elements MODULEF to predict the thermo-mechanical behaviour of the films the maximum tension lay close to the security threshold. The filters system will be assembled changing one standard compound of the front-ends in the beamlines, a so-called refrigerated mask
Mestrado
Física
Mestre em Física
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Chen, Sijia. "FEL theory in the ion channel wiggler." Thesis, University of Strathclyde, 2016. http://digitool.lib.strath.ac.uk:80/R/?func=dbin-jump-full&object_id=27544.

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The ion channel laser (ICL) is an ultra-compact version of the free-electron laser (FEL),with the wiggler replaced by an ion channel. Given its small size and the large wiggler field that can be created within a small volume, it has enormous potential for generating high-frequency coherent radiation. Previous studies of the ICL [1,5], however, have assumed transverse momentum amplitudes that are unrealistically small for experiments, and thus concluded that high-gain high-frequency coherent radiation generation using the ICL is infeasible. In contrast, this thesis shows that this restriction can be removed by correctly taking into account the dependence of the resonance between oscillations and emitted field on the betatron amplitude, which must be treated as variable. The ICL model with this essential addition is described using the well-known formalism for the FEL [3]. Both steady-state and spatio-temporal analyses of the resulting scaled equations show a realistic prospect of building a compact ICL source for fundamental wavelengths down to the UV, with harmonics potentially extending to X-rays. The gain parameter ρ can attain values of the order of 0.01-0.1, which permits driving an ICL with electron bunches with realistic emittance and achieving a radiation power gain comparable to FEL over a small distance. In addition, we present the first results of superradiant simulations for the ICL, also within the framework of the scaled formalism for the FEL, taking into account propagation effects, as well as a full SASE simulation using shot noise as the startup.
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Schoerling, Daniel. "Superconducting wiggler magnets for beam-emittance damping rings." Doctoral thesis, Technische Universitaet Bergakademie Freiberg Universitaetsbibliothek "Georgius Agricola", 2012. http://nbn-resolving.de/urn:nbn:de:bsz:105-qucosa-85819.

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Elektronen- und Positronenstrahlen mit niedrigsten Emittanzen und hohen Strömen werden in zukünftigen Linearbeschleunigern, wie zum Beispiel dem Compact Linear Collider (CLIC), benötigt, um die geforderte Leuchtkraft für physikalische Experimente bereit zu stellen. Diese Strahlen können in Dämpfungsringen, ausgestattet mit starken, supraleitenden Dämpfungswigglermagneten, erzeugt werden. In dieser Arbeit sind Designkonzepte verschiedener supraleitender Dämpfungswigglermagnete entwickelt worden. Testspulen sowie Modelle sind gebaut und getestet, elektrische Verbindungstechniken entwickelt worden. Eine Wärmelastrechnung für den Betrieb in Dämpfungsringen und ein Designkonzept für den kryogenen Betrieb bei 4.2 K ist erstellt worden. Es konnte theoretisch und experimentell gezeigt werden, dass supraleitende Dämpfungswigglermagnete mit Nb-Ti und Nb3Sn Niedertemperatursupraleitern die magnetischen, mechanischen, elektrischen und thermischen Anforderungen erfüllen und in Dämpfungsringen betrieben werden können.
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Al-Shamma'a, Ahmed Ibrahim. "Wiggler system for an industrial free electron laser." Thesis, University of Liverpool, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.318234.

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Tydecks, Tobias. "A Robinson Wiggler for the Metrology Light Source." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät, 2016. http://dx.doi.org/10.18452/17639.

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Im Jahre 1958, schlug Kenneth W. Robinson die Nutzung eines Korrektormagneten vor um den entdämpften radialen Betatronoszillationen im Cambridge electron accelerator entgegen zu wirken. Dieser Korrektormagnet sollte aus kurzen, alternierenden Dipolen mit einem starken Gradienten bestehen, sodass die Verluste durch Synchrotronstrahlung mit zunehmendem Trajektorienradius abnehmen. Diese Transversal-Gradienten-Wiggler werden auch "Robinson Wiggler" (RW) genannt. Die Metrology Light Source (MLS), welche Eigentum der Physikalisch-Technischen Bundesanstalt (PTB) ist und vom Helmholtz-Zentrum Berlin (HZB) entworfen und betrieben wird, ist ein Elektronen-Synchrotron, optimiert für die Produktion von Synchrotronstrahlung im Spektralbereich zwischen THz und EUV. Da die MLS eine gerampte Maschine ist, nimmt der gespeicherte Elektronenstrom mit der Zeit ab und die Strahllebensdauer ist von Bedeutung für die Nutzer der Synchrotronstrahlung. Es wird vorgeschlagen einen RW bei der MLS zu installieren um die Strahllebensdauer zu erhöhen. Mit RW wäre es möglich, Dämpfung aus der longitudinalen in die horizontale Ebene zu verschieben sodass sich die Energiebreite um einen Faktor 3 erhöht und die Emittanz sich um ungefähr einen Faktor 2 reduziert. Die Länge der Elektronenpakete wird dadurch stärker verlängert als die mittlere horizontale Paketbreite reduziert wird. So nimmt die Elektronendichte im Paket ab und die Verlustrate sinkt. Dies hat zu Folge dass sich die Lebensdauer verbessert und die Aktivierung von Komponenten reduziert wird. Mit erhöhter Energiebreite und verringerter Emittanz, wird der Beitrag der Dispersion zur horizontalen Quellgröße stärker. Durch geeignete Wahl der Magnetoptik kann die Brillianz am Quellpunkt erhöht werden bei gleichzeitiger Verbesserung der Lebensdauer. Simulationen zeigen dass die Lebensdauer an der MLS durch die Installation eines solchen RW um einen Faktor 2.3 ansteigt, was einem Zugewinn an integriertem Photonenfluss von 30 % entspricht.
In 1958, Kenneth W. Robinson proposed the usage of a magnetic correction device to reduce the antidamping of radial betatron oscillations in the Cambridge electron accelerator. The essence of this correction device are short, alternating dipoles with a strong gradient, such that the radiation loss decreases with increasing radius of trajectory. These transverse gradient wigglers are also called "Robinson Wigglers" (RW). The Metrology Light Source (MLS), owned by the Physikalisch-Technische Bundesanstalt (PTB) and designed and operated by Helmholtz-Zentrum Berlin (HZB), is an electron synchrotron, optimized for the production of synchrotron radiation in the THz to the EUV spectral region. Being a ramped machine, Top-Up operation is not possible. With a decaying beam current, the lifetime of the stored beam is of importance for the user community, for reasons of temporal stability and integrated photon flux. It is proposed to install a RW at the MLS in order to improve the beam lifetime. With a RW, it is possible to transfer damping from the longitundinal to the horizontal plane in a way, that the energy spread increases by a factor of 3 and the emittance reduces by a factor of 2. Doing so, the bunch length is increased by a larger fraction than the average bunch width is decreased. Thereby the electron density is reduced which results in a lower loss rate of electrons. This improves the beam lifetime and reduces induced radioactivity of accelerator components and shielding. With an increased energy spread and a reduced emittance, the contribution of the dispersion to source size becomes more important. By carefully choosing the magnet optics, the brilliance at the source point can be improved simultaneously to increasing the lifetime. Simulations indicate that a RW is able to increase the lifetime in the standard user operation mode at the MLS by a factor of 2.3, corresponding to an increase in photon flux for one standard user run of approximately 30 %.
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Books on the topic "Wiggles"

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group), Wiggles (Musical, ed. The wiggles: Wiggly colors. New York: Modern Pub., 2004.

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Loupy, Christophe. Wiggles. New York: North-South Books, 2005.

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translator, Franceschelli Christopher, ed. Wiggles. San Francisco, CA: Chronicle Books LLC, 2018.

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ill, Unada, ed. Wiggles. St Petersburg, Fla: Willowisp Press, 1995.

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Rehabilitating Mr. Wiggles. New York: Nantier, Beall, Minoustchine, 2005.

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Rehabilitating Mr. Wiggles. Brooklyn, N.Y: N. Swaab, 2002.

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Anderson, Derek. Blue Burt and Wiggles. New York: Simon & Schuster Books for Young Readers, 2006.

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Wiggles, The: Wiggly Safari (Wiggles). Grosset & Dunlap, 2003.

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Wiggly ABCs (The Wiggles). Modern Publishing, 2004.

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Wiggly Party! (The Wiggles). Grosset & Dunlap, 2005.

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Book chapters on the topic "Wiggles"

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Di Lorenzo, Renato. "Wiggles." In Perspectives in Business Culture, 143–45. Milano: Springer Milan, 2012. http://dx.doi.org/10.1007/978-88-470-2534-9_31.

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Xue, Tianfan, Michael Rubinstein, Neal Wadhwa, Anat Levin, Fredo Durand, and William T. Freeman. "Refraction Wiggles for Measuring Fluid Depth and Velocity from Video." In Computer Vision – ECCV 2014, 767–82. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-10578-9_50.

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Freund, H. P., and T. M. Antonsen. "Wiggler Imperfections." In Principles of Free Electron Lasers, 555–65. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-75106-1_11.

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Dempsey, Jessica, and Geraldine Pratt. "Wiggle Room." In Keywords in Radical Geography: Antipode at 50, 274–79. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2019. http://dx.doi.org/10.1002/9781119558071.ch51.

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Freund, H. P., and T. M. Antonsen. "Electromagnetic-Wave Wigglers." In Principles of Free Electron Lasers, 635–50. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-75106-1_14.

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Wille, Klaus. "Wiggler und Undulatoren." In Physik der Teilchenbeschleuniger und Synchrotronstrahlungsquellen, 249–65. Wiesbaden: Vieweg+Teubner Verlag, 1992. http://dx.doi.org/10.1007/978-3-663-11850-3_8.

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Bärtschi, Ralph, Michael Knauss, Tobias Bonwetsch, Fabio Gramazio, and Matthias Kohler. "Wiggled Brick Bond." In Advances in Architectural Geometry 2010, 137–47. Vienna: Springer Vienna, 2010. http://dx.doi.org/10.1007/978-3-7091-0309-8_10.

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Wille, Klaus. "Wiggler und Undulatoren." In Teubner Studienbücher Physik, 249–65. Wiesbaden: Vieweg+Teubner Verlag, 1996. http://dx.doi.org/10.1007/978-3-663-11039-2_8.

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Freund, H. P., and T. M. Antonsen. "Electromagnetic-wave Wigglers." In Principles of Free-Electron Lasers, 406–20. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2316-7_10.

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Le Kim, Phan, Nguyen Phu Thuy, Phuong LeMinh, and Dinh Hung Manh. "A study on narrow-range angle sensors based on wiggles in angular dependence of pseudo-Hall effect in permalloy thin films." In Transducers ’01 Eurosensors XV, 168–71. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-59497-7_39.

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Conference papers on the topic "Wiggles"

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Pan, Jun, Carlo Luciano Bianco, and She-Sheng Xue. "Rescaled bispectrum and the baryonic wiggles in bispectrum." In RELATIVISTIC ASTROPHYSICS: 4th Italian-Sino Workshop. AIP, 2008. http://dx.doi.org/10.1063/1.2836979.

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Manbachi, Amir, Yiemeng Hoi, and David A. Steinman. "Characterization of Common Carotid Artery Curvature and Its Impact on Velocity Profile Shape." In ASME 2010 Summer Bioengineering Conference. American Society of Mechanical Engineers, 2010. http://dx.doi.org/10.1115/sbc2010-19056.

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Clinical and engineering studies of carotid artery disease typically assume that the common carotid artery (CCA), proximal to the bifurcation, is relatively straight, at least enough to assume the velocity profile is fully-developed (i.e., Poiseuille or Womersley profile) or at least axisymmetric. However, a recent study from our group has shown the surprising presence, in vivo, of strongly skewed velocity profiles in what appeared to be only mildly curved CCAs [1]. A computational fluid dynamics (CFD) study from our group also demonstrated strong velocity profile skewing in an idealized geometry possessing subtle wiggles similar to those observed in the CCA [2].
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Terashima, Hiroshi, Soshi Kawai, and Mitsuo Koshi. "Approach to Prevent Spurious Oscillations in Compressible Multicomponent Flows Using High-Order Methods." In ASME 2012 Fluids Engineering Division Summer Meeting collocated with the ASME 2012 Heat Transfer Summer Conference and the ASME 2012 10th International Conference on Nanochannels, Microchannels, and Minichannels. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/fedsm2012-72246.

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We present an interface-capturing method for fluid interfaces in compressible multicomponent flows using high-order central-difference-based schemes. Numerical diffusion terms are consistently designed so that the velocity, pressure, and temperature equilibriums are maintained at the fluid interfaces, while serving as an efficient interface-capturing. Advection problems of a contact discontinuity and a material interface shows that 1) the present method maintains the velocity, pressure, and temperature equilibriums at the fluid interfaces (oscillation-free property) and 2) the numerical diffusion terms effectively works for suppressing spurious wiggles of the density or temperature. Comparisons with a conventional fully-conservative approach demonstrates the superiority of the present method in avoiding spurious oscillations. A shock tube problem of two-component gases shows the capability for capturing the shock wave while the velocity and pressure equilibriums are successfully maintained at the contact discontinuity.
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Blakely, Richard J., Ray E. Wells, Lydia M. Staisch, Scott E. K. Bennett, and Brian L. Sherrod. "POTENTIAL-FIELD ANOMALIES ILLUMINATE CASCADIA TECTONIC HISTORY, FROM REGIONAL TO OUTCROP SCALE: WORMS, WIGGLES, AND A STRING OF PEARLS." In 115th Annual GSA Cordilleran Section Meeting - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019cd-329159.

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Marcouille, O., F. Marteau, S. Tripathi, A. Thiel, H. Tarawneh, K. Tavakoli, J. L. Marlats, et al. "Production of high energy photons with in vacuum wigglers: From SOLEIL wiggler to MAXIV wiggler." In PROCEEDINGS OF THE 13TH INTERNATIONAL CONFERENCE ON SYNCHROTRON RADIATION INSTRUMENTATION – SRI2018. Author(s), 2019. http://dx.doi.org/10.1063/1.5084590.

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Escobosa, A., S. Gallardo-Hernandez, A. Tavira, M. Lopez-Lopez, R. Cisneros Tamayo, and T. V. Torchinska. "On the gaps observed in high resolution x-ray diffraction scans and the wiggles in reciprocal space maps of high quality crystalline samples." In 2015 IEEE International Autumn Meeting on Power, Electronics and Computing (ROPEC). IEEE, 2015. http://dx.doi.org/10.1109/ropec.2015.7395134.

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Palmer, M. A., J. A. Crittenden, and J. Urban. "Design considerations and modeling results for ILC damping ring wigglers based on the CESR-C superconducting wiggler." In 2007 IEEE Particle Accelerator Conference (PAC). IEEE, 2007. http://dx.doi.org/10.1109/pac.2007.4440652.

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Taccetti, J. M., R. H. Jackson, H. P. Freund, D. E. Pershing, M. Blank, and V. L. Granatstein. "A CHI wiggler ubitron amplifier experiment: wiggler characterization." In International Conference on Plasma Science (papers in summary form only received). IEEE, 1995. http://dx.doi.org/10.1109/plasma.1995.531461.

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Jiang, Leiyong. "Combustor Cooling Wiggle Strip and Geometrical Simplification." In ASME 2008 International Mechanical Engineering Congress and Exposition. ASMEDC, 2008. http://dx.doi.org/10.1115/imece2008-68380.

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The flow fields of a combustor cooling wiggle strip and its corresponding simplified slot with conjugate heat transfer have been studied numerically. The effects of geometrical simplification on the flow fields have been analysed qualitatively and quantitatively. It is found that its effects on the flow velocity and temperature fields are limited to local regions near the cooling element, and are negligible in the far field. However, the simplification shows a considerable effect on the combustor liner temperature near the cooling element, about 8.5% of the average temperature across the cooling element. In short, using the simplified slot to replace the cooling wiggle strip in gas turbine combustor modeling is an acceptable practice if accurate liner temperature prediction is not required.
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Meot, F. "Low-frequency wiggler radiation." In Proceedings of the 1999 Particle Accelerator Conference (Cat. No.99CH36366). IEEE, 1999. http://dx.doi.org/10.1109/pac.1999.792719.

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Reports on the topic "Wiggles"

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Conte, M., and A. Luccio. Wiggler Snakes for RHIC. Office of Scientific and Technical Information (OSTI), September 1992. http://dx.doi.org/10.2172/1151273.

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Lai, B., A. Khounsary, and E. Gluskin. Wiggler A characteristics and specifications. Office of Scientific and Technical Information (OSTI), February 1993. http://dx.doi.org/10.2172/10135104.

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Forest, E., and K. Ohmi. Symplectic integration for complex wigglers. Office of Scientific and Technical Information (OSTI), August 1992. http://dx.doi.org/10.2172/10159952.

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Lai, B., A. Khounsary, and E. Gluskin. Wiggler A characteristics and specifications. Office of Scientific and Technical Information (OSTI), February 1993. http://dx.doi.org/10.2172/6947981.

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Safranek, James. Nonlinear Dynamics in Spear Wigglers. Office of Scientific and Technical Information (OSTI), August 2002. http://dx.doi.org/10.2172/800083.

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Forest, E., and K. Ohmi. Symplectic integration for complex wigglers. Office of Scientific and Technical Information (OSTI), August 1992. http://dx.doi.org/10.2172/7368543.

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Bonifacio, R., L. De Salvo, and P. Pierini. Harmonic generation with multiple wiggler schemes. Office of Scientific and Technical Information (OSTI), February 1995. http://dx.doi.org/10.2172/88778.

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Carr, Roger. A Superconducting Wiggler for the LCLS. Office of Scientific and Technical Information (OSTI), December 2002. http://dx.doi.org/10.2172/812620.

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Armendariz, J., J. Gallardo, T. Romano, and A. van Steenbergen. Fast excitation wiggler field measurement results. Office of Scientific and Technical Information (OSTI), August 1992. http://dx.doi.org/10.2172/10191258.

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Shen, S. S., J. R. Miller, J. R. Heim, and D. S. Slack. Design of a superconducting wiggler system. Office of Scientific and Technical Information (OSTI), October 1988. http://dx.doi.org/10.2172/7010137.

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