2,204 research outputs found

    A cascade MPC control structure for PMSM with speed ripple minimization

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    This paper addresses the problem of reducing the impact of periodic disturbances arising from the current sensor offset error on the speed control of a PMSM. The new results are based on a cascade model predictive control scheme with embedded disturbance model, where the per unit model is utilized to improve the numerical condition of the scheme. Results from an experimental application are given to support the design

    Optimal control of wave linear repetitive processes

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    This paper gives new results on optimal control of the so-called wave discrete linear repetitive processes which find novel application in the modelling of physical examples. These processes have dynamics which are not restricted to the upper right quadrant of the 2D plane and hence the current control results for repetitive processes or 2D systems are not applicabl

    Dissipative stability theory for linear repetitive processes with application in iterative learning control

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    This paper develops a new set of necessary and sufficient conditions for the stability of linear repetitive processes, based on a dissipative setting for analysis. These conditions reduce the problem of determining whether a linear repetitive process is stable or not to that of checking for the existence of a solution to a set of linear matrix inequalities (LMIs). Testing the resulting conditions only requires compu- tations with matrices whose entries are constant in comparison to alternatives where frequency response computations are required

    Probabilistic Mass-Radius Relationship for Sub-Neptune-Sized Planets

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    The Kepler Mission has discovered thousands of planets with radii $<4\ R_\oplus,pavingthewayforthefirststatisticalstudiesofthedynamics,formation,andevolutionofthesesubNeptunesandsuperEarths.Planetarymassesareanimportantphysicalpropertyforthesestudies,andyetthevastmajorityofKeplerplanetcandidatesdonothavetheirsmeasured.AkeyconcernisthereforehowtomapthemeasuredradiitomassestimatesinthisEarthtoNeptunesizerangewheretherearenoSolarSystemanalogs.Previousworkshavederiveddeterministic,onetoonerelationshipsbetweenradiusandmass.However,iftheseplanetsspanarangeofcompositionsasexpected,thenanintrinsicscatteraboutthisrelationshipmustexistinthepopulation.Herewepresentthefirstprobabilisticmassradiusrelationship(MRrelation)evaluatedwithinaBayesianframework,whichbothquantifiesthisintrinsicdispersionandtheuncertaintiesontheMRrelationparameters.Weanalyzehowtheresultsdependontheradiusrangeofthesample,andonhowthemassesweremeasured.AssumingthattheMRrelationcanbedescribedasapowerlawwithadispersionthatisconstantandnormallydistributed,wefindthat, paving the way for the first statistical studies of the dynamics, formation, and evolution of these sub-Neptunes and super-Earths. Planetary masses are an important physical property for these studies, and yet the vast majority of Kepler planet candidates do not have theirs measured. A key concern is therefore how to map the measured radii to mass estimates in this Earth-to-Neptune size range where there are no Solar System analogs. Previous works have derived deterministic, one-to-one relationships between radius and mass. However, if these planets span a range of compositions as expected, then an intrinsic scatter about this relationship must exist in the population. Here we present the first probabilistic mass-radius relationship (M-R relation) evaluated within a Bayesian framework, which both quantifies this intrinsic dispersion and the uncertainties on the M-R relation parameters. We analyze how the results depend on the radius range of the sample, and on how the masses were measured. Assuming that the M-R relation can be described as a power law with a dispersion that is constant and normally distributed, we find that M/M_\oplus=2.7(R/R_\oplus)^{1.3},ascatterinmassof, a scatter in mass of 1.9\ M_\oplus,andamassconstrainttophysicallyplausibledensities,isthe"bestfit"probabilisticMRrelationforthesampleofRVmeasuredtransitingsubNeptunes(, and a mass constraint to physically plausible densities, is the "best-fit" probabilistic M-R relation for the sample of RV-measured transiting sub-Neptunes (R_{pl}<4\ R_\oplus$). More broadly, this work provides a framework for further analyses of the M-R relation and its probable dependencies on period and stellar properties.Comment: 14 pages, 5 figures, 2 tables. Accepted to the Astrophysical Journal on April 28, 2016. Select posterior samples and code to use them to compute the posterior predictive mass distribution are available at https://github.com/dawolfgang/MRrelatio

    Decoupling and iterative approaches to the control of discrete linear repetitive processes

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    This paper reports new results on the analysis and control of discrete linear repetitive processes which are a distinct class of 2D discrete linear systems of both systems theoretic and applications interest. In particular, we first propose an extension to the basic state-space model to include a coupling term previously neglected but which arises in some applications and then proceed to show how computationally efficient control laws can be designed for this new model

    Experimentally validated continuous-time repetitive control of non-minimum phase plants with a prescribed degree of stability

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    This paper considers the application of continuous-time repetitive control to non-minimum phase plants in a continuous-time model predictive control setting. In particular, it is shown how some critical performance problems associated with repetitive control of such plants can be avoided by use of predictive control with a prescribed degree of stability. The results developed are first illustrated by simulation studies and then through experimental tests on a non-minimum phase electro-mechanical system

    The Ambient Horn: Designing a novel audio-based learning experience

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    The Ambient Horn is a novel handheld device designed to support children learning about habitat distributions and interdependencies in an outdoor woodland environment. The horn was designed to emit non-speech audio sounds representing ecological processes. Both symbolic and arbitrary mappings were used to represent the processes. The sounds are triggered in response to the children’s location in certain parts of the woodland. A main objective was to provoke children into interpreting and reflecting upon the significance of the sounds in the context in which they occur. Our study of the horn being used showed the sounds to be provocative, generating much discussion about what they signified in relation to what the children saw in the woodland. In addition, the children appropriated the horn in creative ways, trying to ‘scoop’ up new sounds as they walked in different parts of the woodland

    Ten Years of Inter Partes Patent Reexamination Appeals: An Empirical View

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    An empirical analysis of the first ten years of decisions by the Board Patent Appeals and Interferences regarding inter partes patent reexamination appeals was conducted. The analysis of 101 cases focused on answering three broad questions: (1) How accurate are the specialist patent examiners of the Central Reexamination Unit of the U.S. Patent and Trademark Office? (2) Do patent owners or third party requestors fare better in appeals of decisions in inter partes reexamination proceedings? (3) Which types of appeals are more likely to be successful? The examiners’ determinations were upheld more than three fourths of the time; third party requestors tended to be more successful than patent owners at winning appeals; and appeals solely by third party requestors of unadopted grounds of rejection were the most successful type of appeal. These historical observations can be used to predict the success rate for appeals of Patent Trial and Appeal Board decisions in Inter Partes Review (IPR) proceedings, which was implemented in September 2012. Appeals of IPR decisions by third party requestors are predicted to have a better success rate at maintaining patent claim rejections and adding new grounds of rejection than appeals by patent owners will have at receiving reversal of patent claim rejections
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