50 results on '"I., Arregui"'
Search Results
2. Pápula pedunculada en región plantar
- Author
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I. Arregui, C. Ñanco, and F. Mardones
- Subjects
Dermatology ,RL1-803 ,Internal medicine ,RC31-1245 - Published
- 2023
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3. Pápula pedunculada en región plantar
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L, I Arregui, primary, M, C Ñanco, additional, and V, F Mardones, additional
- Published
- 2023
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4. Fracture Assessment From Well-Centered and Reservoir Scale Coupled Geomechanical Models
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J. M. Segura, R. C. Bezerra de Melo, A. Martínez, J. Alvarellos, M. Morón, S. Fontenla, E. Vargas, C. Rojas, and J. I. Arregui
- Abstract
Abstract An integrated and multiscale analysis has been performed to ensure safe reinjection of formation water into a sandstone saline aquifer during the lifecycle of an onshore field. The study includes well centered models to evaluate the possibility of creation and propagation of hydraulic fractures, paying special attention to vertical fracture containment within the target zone. The hydraulic fracture models are fed by geomechanical models that provide estimations of stresses and rock mechanical properties, and which include lithological and stress contrasts that replicate the drilling experience of the two injection wells. A 3D reservoir scale coupled geomechanical and fluid-flow model has been generated for integrity analysis of the target and seal formations, and faults, also analyzing the effect that injection operations could have on surface uplift. The most critical assumptions are considered in the assessment, like lower than expected fracture gradient, higher than expected injection rates, and mechanical and fluid flow parameters that favor hydraulic fracture propagation. The analyzed cases show how eventual fractures would be confined in height, only propagating laterally with a tendency of stabilizing and without affecting the integrity of nearby wells. No other type of rock failure nor fault reactivation is observed anywhere in the model. Introduction Reinjection of formation water that has been extracted along with hydrocarbons must be performed in a secure and safe manner. Geomechanics analysis can help in predicting the effect of pore-pressure increase associated to injection operations on the deformation and failure of rock (in target formation and in surrounding formations) as well as on the reactivation of faults, being both relevant aspects in ensuring safe operations during the field lifecycle.
- Published
- 2022
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5. Construction of coronal hole and active region magnetohydrostatic solutions in two dimensions: Force and energy balance
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J., Terradas, R., Soler, R., Oliver, P., Antolin, I., Arregui, M., Luna, I., Piantschitsch, E., Soubrié, L, Ballester J., J., Terradas, R., Soler, R., Oliver, P., Antolin, I., Arregui, M., Luna, I., Piantschitsch, E., Soubrié, and L, Ballester J.
- Abstract
Coronal holes and active regions are typical magnetic structures found in the solar atmosphere. We propose several magnetohydrostatic equilibrium solutions that are representative of these structures in two dimensions. Our models include the effect of a finite plasma-$\beta$ and gravity, but the distinctive feature is that we incorporate a thermal structure with properties similar to those reported by observations. We developed a semi-analytical method to compute the equilibrium configuration. Using this method, we obtain cold and under-dense plasma structures in open magnetic fields representing coronal holes, while in closed magnetic configurations, we achieve the characteristic hot and over-dense plasma arrangements of active regions. Although coronal holes and active regions seem to be antagonistic structures, we find that they can be described using a common thermal structure that depends on the flux function. In addition to the force balance, the energy balance is included in the constructed models using an a posteriori approach. From the two-dimensional computation of thermal conduction and radiative losses in our models, we infer the required heating function to achieve energy equilibrium. We find that the temperature dependence on height is an important parameter that may prevent the system from accomplishing thermal balance at certain spatial locations. The implications of these results are discussed in detail., Comment: Accepted for publication in A&A
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- 2022
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6. High-yield waveguide diplexer for low-cost E-band 5G point-to-point radio links
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F. Teberio, I. Calero, I. Arregui, P. Martin-Iglesias, J. Teniente, M. A. G. Laso, Universidad Pública de Navarra. Departamento de Ingeniería Eléctrica, Electrónica y de Comunicación, Universidad Pública de Navarra / Nafarroako Unibertsitate Publikoa. Institute of Smart Cities - ISC, and Nafarroako Unibertsitate Publikoa. Ingeniaritza Elektrikoa, Elektronikoa eta Telekomunikazio Ingeniaritza Saila
- Subjects
Diplexer ,Waveguide ,E-band ,Point-to-point radio-link ,5G - Abstract
This paper presents the design and realization of a high-yield tuning-less waveguide diplexer and a high-gain lens horn antenna for 5G point-to-point fixed-beam communications at the frequency ranges of 71/76 GHz and 81/86 GHz (E-band). The diplexer is composed of two bandpass filters based on the combination of a low-pass filtering function and a high-pass structure. The diplexer provides very relaxed fabrication tolerances. A prototype has been fabricated and measured showing return loss better than 20 dB and attenuation levels higher than 60 dB. The insertion loss is better than 1 dB. A lens horn antenna which provides more than 38 dBi gain is utilized to provide high directivity at the same frequencies. The proposed sub-system combines the advantages of high-performance and simple mechanical assembly finding, it especially attractive for 5G applications due to the reduced fabrication cost. This work was supported by the Spanish Ministerio de Ciencia, Innovación y Universidades–Agencia Estatal de Investigación under Project TEC2017-85529-C3-2-R (AEI, FEDER-EU).
- Published
- 2022
7. Some young adults with cystic fibrosis‐related diabetes may safely stop insulin without any adverse clinical sequelae
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I. Arregui‐Fresneda, T. Daniels, C. Ogbolu, and R. I. G. Holt
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Glycated Hemoglobin ,Male ,Pediatrics ,medicine.medical_specialty ,Adolescent ,Cystic Fibrosis ,business.industry ,Endocrinology, Diabetes and Metabolism ,Insulin ,medicine.medical_treatment ,Cystic fibrosis-related diabetes ,medicine.disease ,Young Adult ,Deprescriptions ,Endocrinology ,Insulin Secretion ,Diabetes Mellitus ,Internal Medicine ,medicine ,Humans ,Hypoglycemic Agents ,Female ,Young adult ,business - Published
- 2020
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8. [Cryptosporidiosis in immunosuppressed renal transplant patient]
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C Ezpeleta Baquedano, A Aguinaga Pérez, M Elía Lòpez, J Manrique Escola, and I Arregui Garcia
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Microbiology (medical) ,Pharmacology ,medicine.medical_specialty ,business.industry ,Cryptosporidiosis ,General Medicine ,Gastroenterology ,Kidney Transplantation ,Feces ,Immunocompromised Host ,Renal transplant ,Internal medicine ,Carta al Director ,Medicine ,Humans ,business - Published
- 2021
9. The Impact of Plasma 25-Hydroxyvitamin D on Lung Function in Patients with Cystic Fibrosis
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A J Causer, Z L Saynor, I Arregui-Fresneda, G Connett, M I Allenby, T Daniels, M P Carroll, D S Urquhart, and R Revuelta Iniesta
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- 2020
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10. Prominence seismology using ground- and space-based observations
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Roberto Soler, I. Arregui, Oddbjørn Engvold, L. Rouppe van der Voort, Jose Luis Ballester, O. Langagen, J. Terradas, Y. Lin, and Ramon Oliver
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Physics ,Physics::Plasma Physics ,Space and Planetary Science ,Physics::Space Physics ,General Engineering ,Astrophysics::Solar and Stellar Astrophysics ,Astronomy and Astrophysics ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,Space (mathematics) ,Measure (mathematics) ,Seismology ,Solar prominence - Abstract
Ground- and space-based observations have confirmed the presence of oscillatory motions in prominences and they have been interpreted in terms of magnetohydrodynamic (MHD) waves. This interpretation opens the door to perform prominence seismology, whose main aim is to determine physical parameters in magnetic and plasma structures (prominences) that are difficult to measure by direct means. Here, two prominence seismology applications are presented.
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- 2012
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11. No unique solution to the seismological problem of standing kink magnetohydrodynamic waves
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M. Goossens and I. Arregui
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corona [Sun] ,010504 meteorology & atmospheric sciences ,statistical [methods] ,SURFACE-WAVES ,Astrophysics ,Astronomy & Astrophysics ,magnetohydrodynamics (MHD) ,FLUX TUBES ,01 natural sciences ,Physics::Geophysics ,Methods statistical ,EXCITATION ,0103 physical sciences ,RESONANT ABSORPTION ,Astrophysics::Solar and Stellar Astrophysics ,waves ,Magnetohydrodynamic drive ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Physics ,Science & Technology ,oscillations [Sun] ,Astronomy and Astrophysics ,Computational physics ,PERIOD MAGNETIC PULSATIONS ,MHD WAVES ,Space and Planetary Science ,Physical Sciences ,MODES ,ALFVEN WAVES ,CORONAL LOOP OSCILLATIONS ,BEHAVIOR - Abstract
© ESO 2019. The aim of this paper is to point out that the classic seismological problem using observations and theoretical expressions for the periods and damping times of transverse standing magnetohydrodynamic waves in coronal loops is better referred to as a reduced seismological problem. "Reduced" emphasises the fact that only a small number of characteristic quantities of the equilibrium profiles can be determined. Reduced also implies that there is no unique solution to the full seismological problem. Even the reduced seismological problem does not allow a unique solution. Bayesian inference results support our mathematical arguments and offer insight into the relationship between the algebraic and the probabilistic inversions. ispartof: ASTRONOMY & ASTROPHYSICS vol:622 status: published
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- 2019
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12. Visual Perception of Portion Size
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A. Wise, L. Duncan, G. Moalosi, and I. Arregui-Fresneda
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Visual perception ,Ecology ,French fries ,Statistics ,Medicine (miscellaneous) ,General Medicine ,Food science ,Portion size ,Food Science ,Mathematics - Abstract
Three studies were made in which chips (French fries) of different thickness and peas of different sizes were used. In each study, subjects were asked to serve the food in an attempt to match a standard amount of food placed on the table. Subjects served significantly (P < 0.001) smaller amounts of thin chips compared to thick chips, whether the standard was rice or chips, but for peas there was no effect of size of pea on the amount served. When chips were cut into cubes, results were more similar to those found with peas rather than with the original chips.
- Published
- 2008
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13. Resonant absorption in multi-stranded coronal loops
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Ramon Oliver, Jose Luis Ballester, I. Arregui, and J. Terradas
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Physics ,Transverse plane ,Space and Planetary Science ,Energy transformation ,Astronomy and Astrophysics ,Astrophysics ,Coronal loop ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,Coronal radiative losses ,Excitation ,Nanoflares ,Computational physics - Abstract
We study the excitation and damping of transverse oscillations in a complex multi-stranded model of a coronal loop. By numerically solving the time-dependent magnetohydrodynamic (MHD) equations in two dimensions, we show how the global motion of the whole bundle of tubes, produced by an external disturbance, is converted into localised motions due to the process of resonant absorption. At any location in the structure two dominant frequencies are found, the frequency of the global mode (different from the kink frequency of the individual strands) and the local Alfvén frequency. The mechanism of mode conversion is not affected by the complicated geometry of the system and for certain configurations the energy conversion does not only take place at the external edge of the composite loop but also inside the structure.
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- 2007
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14. Damped oscillations of two interacting coronal loops
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J. Terradas, I. Arregui, Ramon Oliver, and Jose Luis Ballester
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Physics ,Antisymmetric relation ,Oscillation ,Astronomy and Astrophysics ,Mechanics ,Coronal loop ,Wave equation ,Nanoflares ,Classical mechanics ,Physics::Plasma Physics ,Space and Planetary Science ,Normal mode ,Slab ,Magnetohydrodynamics - Abstract
We present results on the oscillatory properties (periods, damping rates, and spatial distribution of perturbations) for resonantly damped oscillations in a system of two inhomogeneous coronal slabs and compare them to the properties found in single slab loop models. A system of two identical coronal loops is modelled, in Cartesian geometry, as being composed by two density enhancements. The linear magnetohydrodynamic (MHD) wave equations for oblique propagation of waves are solved and the damping due to resonant absorption is computed. Due to the interaction between the loops, the normal modes of oscillation present in a single slab split into symmetric and antisymmetric oscillations when a system of two identical slabs is considered. The frequencies of these solutions may differ from the single slab results when the distance between the loops is of the order of a few slab widths. Oblique propagation of waves weakens this interaction, since solutions become more confined to the edges of the slabs. The damping is strong for surface-like oscillations, while sausage body-like solutions are unaffected.
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- 2007
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15. Magnetohydrodynamic waves in a sheared potential coronal arcade
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Jose Luis Ballester, I. Arregui, and Ramon Oliver
- Subjects
Physics ,Continuous spectrum ,Astronomy and Astrophysics ,Plasma ,Astrophysics ,Wave equation ,Magnetic field ,Classical mechanics ,Space and Planetary Science ,Normal mode ,Quantum electrodynamics ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,Adiabatic process - Abstract
We study the effects of magnetic field shear (B y ¬= 0) and longitudinal propagation of perturbations (k y ¬= 0) on the linear and adiabatic magnetohydrodynamic (MHD) normal modes of oscillation of a potential coronal arcade. In a cold plasma, the inclusion of these two effects produces the linear coupling of discrete fast modes, characterised by a discrete spectrum of frequencies and a global velocity structure, and Alfven continuum modes, characterised by a continuous spectrum of frequencies and with a velocity perturbation confined to given magnetic surfaces in such a way that modes with mixed properties arise (Arregui et al. 2004). The wave equations governing the velocity perturbations have been solved numerically and our results show that the couplings between fast and Alfven modes are governed by some parity rules for the symmetry of the eigenfunctions of fast and Alfven modes in the direction along the equilibrium magnetic field. The nature of the coupling between fast and Alfven modes can be resonant or non-resonant depending on the location of the fast mode frequency within the different Alfven continua. Also, an important result is that in this kind of configurations coupled modes could be difficult to observe since when both magnetic field shear and longitudinal propagation are present the spatial distribution of the velocity may not be confined to low heights in the solar corona.
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- 2004
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16. Magnetohydrodynamic Waves in Sheared Coronal Arcades
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Jose Luis Ballester, I. Arregui, and Ramon Oliver
- Subjects
Physics ,Astronomy and Astrophysics ,Magnetic field ,Classical mechanics ,Singularity ,Space and Planetary Science ,Normal mode ,Quantum electrodynamics ,Physics::Space Physics ,Mode coupling ,Wavenumber ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,Longitudinal wave - Abstract
The magnetohydrodynamic (MHD) normal modes of oscillation of sheared coronal arcades including longitudinal wave propagation are studied. Solutions have been computed to ascertain the effects of the longitudinal magnetic field component, By, and of the longitudinal wavenumber, ky, in these structures. Our results show that whenever By ≠ 0 and/or ky ≠ 0, fast modes, characterized by a global velocity structure and a discrete spectrum of frequencies, and Alfven continuum modes, characterized by a velocity perturbation confined to given magnetic surfaces, get coupled and no pure fast modes or pure Alfven modes exist, but modes with mixed properties arise. These oscillatory modes display a global spatial distribution, together with a nonsquare integrable singular behavior on certain magnetic surfaces. Moreover, this mode coupling is such that under some circumstances the Alfvenic contribution is also in the form of a smooth velocity profile covering a range of magnetic surfaces instead of a singularity on a fixed magnetic surface. The coupling between fast and Alfven modes is governed by the parity of their eigenfunctions in the direction along the equilibrium magnetic field. The parity rules determining the features of coupled modes in terms of their spatial structure, ky, and By are presented. We have found that the frequency of coupled modes is real when either By ≠ 0 or ky ≠ 0 but is complex when both By ≠ 0 and ky ≠ 0. Also, an important result is that coupled modes may not be observable since many of them leak energy away from the solar corona.
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- 2004
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17. Coupling of fast and Alfvén waves in a straight bounded magnetic field with density stratification
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I. Arregui, Jose Luis Ballester, and Ramon Oliver
- Subjects
Physics ,Wave propagation ,Field line ,Astronomy and Astrophysics ,Astrophysics ,Classification of discontinuities ,Computational physics ,Magnetic field ,Alfvén wave ,Classical mechanics ,Space and Planetary Science ,Physics::Space Physics ,Mode coupling ,Magnetohydrodynamic drive ,Magnetohydrodynamics - Abstract
The theoretical understanding of the linear standing or propagating magnetohydrodynamic waves in a variety of solar coronal structures is far from complete since analytical solutions to the linearised MHD equations can only be found for very simple magnetic configurations. In this paper, we use a numerical code to solve the linear fast and Alfven wave equations in a very simple, bounded magnetic configuration that incorporates two features that are not usually considered in similar works, namely the longitudinal magnetic field component and wave propagation in the longitudinal direction ($k_y\neq 0$). We use a numerical code (Arregui et al. 2001) that has been modified by including a staggered mesh that allows us to properly capture the spatial behaviour of solutions to the wave equations. Coupling between fast and Alfven modes has been studied in detail and it has been found that it does not take place when the longitudinal field component is zero and the frequency of the fast mode is outside the Alfven continuum with the same spatial structure along field lines. Under these circumstances, fast modes retain their global spatial behaviour and are also characterised by $\omega^2$ varying linearly with $k_y^2$, such as in a uniform medium (although here the Alfven speed changes exponentially in the direction normal to field lines). Regarding mode coupling, its main feature is the blend of fast and Alfven solutions with close frequencies in some modes with a mixture of their properties, namely discontinuities or jumps around certain magnetic surfaces (such as in pure Alfven waves), global spatial distribution of the normal velocity component and non-zero density perturbations (such as in fast waves).
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- 2003
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18. Numerical simulations of linear magnetohydrodynamic waves in two-dimensional force-free magnetic fields
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I. Arregui, Jose Luis Ballester, and Ramon Oliver
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Physics ,Trace (linear algebra) ,Spacecraft ,business.industry ,Oscillation ,Astronomy and Astrophysics ,Astrophysics ,Wave equation ,Magnetic field ,Space and Planetary Science ,Simple (abstract algebra) ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,business - Abstract
High resolution observations of the solar corona made with instruments onboard the SOHO and TRACE spacecrafts have provided new evidence for the presence of oscillations in a variety of coronal magnetic structures. Most of these observations have been interpreted in terms of linear standing or propagating magnetohydrodynamic (MHD) waves, but the theoretical understanding is far from complete since analytical solutions to the linearised MHD wave equations can only be found for very simple magnetic congurations. Taking into account that the solar corona is basically structured by force-free magnetic elds, our purpose in this paper is to present the derivation of the linear MHD wave equations for a two-dimensional force-free magnetic eld conguration having longitudinal invariance, as well as to introduce a numerical code to solve the resulting system of coupled partial dierential equations. The accuracy of the code has been checked by numerically solving two cases for which analytical or simple numerical solutions exist. To our knowledge, this is the only two-dimensional code developed to study the normal MHD modes of oscillation of a general force-free eld with longitudinal invariance.
- Published
- 2001
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19. The Sun and the Solar System
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Ramon Oliver, I. Arregui, Jose Luis Ballester, and Jaume Terradas
- Subjects
Protein filament ,Physics ,Transverse plane ,Flux tube ,Physics::Space Physics ,Coronal mass ejection ,Plasma ,Magnetohydrodynamic drive ,Astrophysics ,Magnetohydrodynamics ,Solar prominence ,Computational physics - Abstract
High-resolution observations provide evidence of the existence of small-amplitude transverse oscillations in solar filament fine structures. These oscillations are believed to represent fast magnetohydrodynamic (MHD) waves and the disturbances are seen to be damped in short timescales of the order of 1–4 periods. We propose that, due to the highly inhomogeneous nature of the filament plasma at the fine-structure spatial scale, the phenomenon of resonant absorption is likely to operate in the temporal attenuation of fast MHD oscillations. By considering transverse inhomogeneity in a straight flux tube model we find that, for density inhomogeneities typical of filament threads, the decay times are of a few oscillatory periods only.
- Published
- 2010
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20. The Temporal Evolution of Linear Fast and Alfvén MHD Waves in Solar Coronal Arcades
- Author
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I. Arregui, Jose Luis Ballester, Jaume Terradas, S. Rial, and Ramon Oliver
- Subjects
Physics ,Perturbation (astronomy) ,Plasma ,Wave equation ,Computational physics ,law.invention ,Protein filament ,Classical mechanics ,Physics::Plasma Physics ,law ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,Excitation ,Flare - Abstract
The excitation and temporal evolution of fast and Alfven magnetohydrodynamic oscillations in a two-dimensional coronal arcade are investigated. The approach is to consider an equilibrium magnetic and plasma structure and then to introduce a perturbation trying to mimic a nearby disturbance, such as a flare or filament eruption. By numerically solving the time-dependent linearized MHD wave equations, the properties of the solutions have been studied. First, the properties of uncoupled fast and Alfven waves are described. Then, longitudinal propagation of perturbations is included, and the properties of coupled waves are determined.
- Published
- 2010
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21. Analytical solution for the design of planar EBG structures with spurious-free frequency response
- Author
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I. Arnedo, J. D. Schwartz, I. Arregui, M. A. G. Laso, D. V. Plant, J. Azana, and T. Lopetegi
- Published
- 2009
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22. Multipactor prediction in novel high-power low-pass filters with wide rejection band
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I. Arregui, S. Anza, I. Arnedo, C. Vicente, A. Lujambio, J. Gil, M. Chudzik, B. Gimeno, T. Lopetegi, M. A. G. Laso, and V. E. Boria
- Published
- 2009
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23. Transverse Oscillations in Coronal Loops
- Author
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I. Arregui, M. Luna, R. Oliver, J. Terradas, J. L. Ballester, Cristiana Dumitrache, Vasile Mioc, and Nedelia A. Popescu
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Physics ,Transverse plane ,Physics::Space Physics ,Astrophysics::Solar and Stellar Astrophysics ,Coronal hole ,Coronal loop ,Magnetohydrodynamic drive ,Astrophysics ,Magnetohydrodynamics ,Corona ,Solar prominence ,Nanoflares - Abstract
During last years, direct evidence about oscillations in different coronal structures has been obtained thanks to the detailed observations made by SoHO and TRACE. With the help of magnetohydrodynamic (MHD) wave theory, we can explain these observations as due to the excitation and propagation of MHD waves in the solar corona. In spite that there are many solar coronal structures in which oscillations have been detected (prominences, loops, plumes, coronal holes, etc.), in the following we will concentrate on transverse oscillations of coronal loops, reviewing some theoretical models developed to understand these oscillations in terms of MHD waves.
- Published
- 2007
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24. Solar coronal loop oscillations: theory of resonantly damped oscillations and comparison with observations
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J. Andries, Stefaan Poedts, I. Arregui, M. Goossens, and Tom Van Doorsselaere
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Physics ,Loop (topology) ,Transverse plane ,Classical mechanics ,Mode (statistics) ,Boundary (topology) ,Coronal loop ,Mechanics ,Radial direction ,Damped oscillations ,Magnetic field - Abstract
One of the proposed damping mechanisms of coronal transverse loop oscillations in the kink mode is resonant absorption as a result of the spatial variation of the Alfven velocity in the equilibrium configuration. Analytical expressions for the period and the damping time exist for 1‐D cylindrical equilibrium models with thin non‐uniform transitional layers. Comparison with observations indicates that the assumption of thin non‐uniform transitional layers is not a very accurate approximation of reality. This contributions starts with a short review of observations on transverse oscillations in solar coronal loops. Then it presents results on periods and damping times of resonantly damped kink mode oscillations for (i) fully non‐uniform 1‐D cylindrical equilibrium models in which the equilibrium quantities vary in the radial direction across the magnetic field from the centre of the loop up to its boundary and (ii) non‐uniform 2‐D cylindrical equilibrium models in which the equilibrium quantities vary both ...
- Published
- 2005
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25. A systematic review of powered vs manual toothbrushes in periodontal cause-related therapy
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A, Sicilia, I, Arregui, M, Gallego, B, Cabezas, and S, Cuesta
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Adult ,Toothbrushing ,Sonication ,Tooth Abrasion ,Electricity ,Dental Plaque ,Health Education, Dental ,Humans ,Gingival Recession ,Equipment Design ,Periodontal Index ,Periodontal Diseases ,Randomized Controlled Trials as Topic - Abstract
Power-driven toothbrushes (PDT) have been designed to improve the efficacy of oral hygiene. It is not clear how they compare in efficacy with manual toothbrushes in cause-related periodontal therapy.To evaluate the effectiveness of the use of a PDT as compared with a manual toothbrush (MT), in terms of gingival bleeding or inflammation resolution, in cause-related periodontal therapy.An electronic (MEDLINE and Cochrane Oral Health Group Specialised Trials Register) and a manual search were made to detect studies which permitted the evaluation of the efficacy of PDT in the reduction of gingival bleeding or inflammation, and their effect on other secondary variables. Only randomized studies in adults, published in English up to June 2001, which compared a PDT with an MT, and evaluated the evolution of gingival bleeding or inflammation were included. The selection of articles, extraction of data and assessment of validity were made independently by several reviewers.Twenty-one studies were finally selected. The heterogeneity of the data prevented a quantitative analysis. A higher efficacy in the reduction of gingival bleeding or inflammation in the PDT patients was detected in 10 studies. This effect appears to be related to the capacity to reduce plaque, and is more evident in counter-rotational and oscillating-rotating brushes. No solid evidence was found for a higher efficacy of sonic brushes. In short-term studies with prophylaxis after initial examination, independently of the type of PDT tested, no significant differences were found.The use of PDT, especially counter-rotational and oscillating-rotating brushes, can be beneficial in reducing the levels of gingival bleeding or inflammation. There is a need for methodological homogeneity in future studies in this field to enable quantitative analysis of their results.
- Published
- 2003
26. ANALYTIC APPROXIMATE SEISMOLOGY OF PROPAGATING MAGNETOHYDRODYNAMIC WAVES IN THE SOLAR CORONA
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M. Goossens, I. Arregui, J. Terradas, and Roberto Soler
- Subjects
Physics ,010504 meteorology & atmospheric sciences ,Phase (waves) ,Astronomy and Astrophysics ,Atmospheric-pressure plasma ,Inversion (meteorology) ,Solar atmosphere ,01 natural sciences ,Magnetic field ,Wavelength ,Physics::Plasma Physics ,Space and Planetary Science ,Physics::Space Physics ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Magnetohydrodynamic drive ,Magnetohydrodynamics ,010303 astronomy & astrophysics ,Seismology ,0105 earth and related environmental sciences - Abstract
Observations show that propagating magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere. The technique of MHD seismology uses the wave observations combined with MHD wave theory to indirectly infer physical parameters of the solar atmospheric plasma and magnetic field. Here we present an analytical seismological inversion scheme for propagating MHD waves. This scheme uses in a consistent manner the observational information on wavelengths and damping lengths, along with observed values of periods or phase velocities, and is based on approximate asymptotic expressions for the theoretical values of wavelengths and damping lengths. The applicability of the inversion scheme is discussed and an example is given.
- Published
- 2012
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27. Erratum: 'Magnetohydrodynamic Waves in Sheared Coronal Arcades' (ApJ, 602, 1006 [2004])
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Ramon Oliver, I. Arregui, and Jose Luis Ballester
- Subjects
Physics ,Space and Planetary Science ,Coronal plane ,Astronomy and Astrophysics ,Magnetohydrodynamic drive ,Astrophysics - Published
- 2004
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28. Damping of magnetohydrodynamic waves by resonant absorption in the solar atmosphere.
- Author
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M. Goossens, J. Andries, and I. Arregui
- Published
- 2006
29. Quasi-mode damping in two-dimensional fully non-uniform coronal loops.
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I. Arregui, T. Van Doorsselaere, J. Andries, M. Goossens, and D. Kimpe
- Published
- 2006
30. Normal Modes of Transverse Coronal Loop Oscillations from Numerical Simulations. I. Method and Test Case.
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S. Rial, I. Arregui, R. Oliver, and J. Terradas
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- *
COMPUTER simulation , *TEST methods , *OSCILLATIONS , *ORTHOGONAL functions , *EIGENFUNCTIONS - Abstract
The purpose of this work is to develop a procedure to obtain the normal modes of a coronal loop from time-dependent numerical simulations with the aim of better understanding observed transverse loop oscillations. To achieve this goal, in this paper we present a new method and test its performance with a problem for which the normal modes can be computed analytically. In a follow-up paper, the application to the simulations of Rial et al. is tackled. The method proceeds iteratively and at each step consists of (i) a time-dependent numerical simulation followed by (ii) the Complex Empirical Orthogonal Function (CEOF) analysis of the simulation results. The CEOF analysis provides an approximation to the normal mode eigenfunctions that can be used to set up the initial conditions for the numerical simulation of the following iteration, in which an improved normal mode approximation is obtained. The iterative process is stopped once the global difference between successive approximate eigenfunctions is below a prescribed threshold. The equilibrium used in this paper contains material discontinuities that result in one eigenfunction with a jump across these discontinuities and two eigenfunctions whose normal derivatives are discontinuous there. After six iterations, the approximations to the frequency and eigenfunctions are accurate to ≲0.7% except for the eigenfunction with discontinuities, which displays a much larger error at these positions. [ABSTRACT FROM AUTHOR]
- Published
- 2019
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31. ON THE MAGNETISM AND DYNAMICS OF PROMINENCE LEGS HOSTING TORNADOES.
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M. J. Martínez González, A. Asensio Ramos, I. Arregui, M. Collados, C. Beck, and J. de la Cruz Rodríguez
- Subjects
SOLAR prominences ,SOLAR magnetism ,ASTRONOMICAL polarimetry ,HELICAL structure ,SOLAR corona - Abstract
Solar tornadoes are dark vertical filamentary structures observed in the extreme ultraviolet associated with prominence legs and filament barbs. Their true nature and relationship to prominences requires an understanding of their magnetic structure and dynamic properties. Recently, a controversy has arisen: is the magnetic field organized forming vertical, helical structures or is it dominantly horizontal? And concerning their dynamics, are tornadoes really rotating or is it just a visual illusion? Here we analyze four consecutive spectro-polarimetric scans of a prominence hosting tornadoes on its legs, which helps us shed some light on their magnetic and dynamical properties. We show that the magnetic field is very smooth in all the prominence, which is probably an intrinsic property of the coronal field. The prominence legs have vertical helical fields that show slow temporal variation that is probably related to the motion of the fibrils. Concerning the dynamics, we argue that (1) if rotation exists, it is intermittent, lasting no more than one hour, and (2) the observed velocity pattern is also consistent with an oscillatory velocity pattern (waves). [ABSTRACT FROM AUTHOR]
- Published
- 2016
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32. MODEL COMPARISON FOR THE DENSITY STRUCTURE ACROSS SOLAR CORONAL WAVEGUIDES.
- Author
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I. Arregui, R. Soler, and A. Asensio Ramos
- Subjects
- *
SOLAR corona , *WAVEGUIDES , *SOLAR atmosphere , *MAGNETOHYDRODYNAMICS , *OSCILLATIONS , *SPATIAL variation - Abstract
The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave damping and energy dissipation. The direct measurement of the spatial distribution of density, however, is difficult, and indirect seismology inversion methods have been suggested as an alternative. We applied Bayesian inference, model comparison, and model-averaging techniques to the inference of the cross-field density structuring in solar magnetic waveguides using information on periods and damping times for resonantly damped magnetohydrodynamic transverse kink oscillations. Three commonly employed alternative profiles were used to model the variation of the mass density across the waveguide boundary. Parameter inference enabled us to obtain information on physical quantities such as the Alfvén travel time, the density contrast, and the transverse inhomogeneity length scale. The inference results from alternative density models were compared and their differences quantified. Then, the relative plausibility of the considered models was assessed by performing model comparison. Our results indicate that the evidence in favor of any of the three models is minimal, unless the oscillations are strongly damped. In such a circumstance, the application of model-averaging techniques enables the computation of an evidence-weighted inference that takes into account the plausibility of each model in the calculation of a combined inversion for the unknown physical parameters. [ABSTRACT FROM AUTHOR]
- Published
- 2015
- Full Text
- View/download PDF
33. Methicillin-resistant Staphylococcus aureus bacteremia carrying the mecC gene.
- Author
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Arregui Garcia I, Portillo ME, Torroba Álvarez L, and Ezpeleta Baquedano C
- Subjects
- Humans, Anti-Bacterial Agents, Bacterial Proteins genetics, Methicillin-Resistant Staphylococcus aureus genetics, Bacteremia drug therapy
- Published
- 2023
- Full Text
- View/download PDF
34. Emergence of multidrug-resistant Haemophilus parainfluenzae in genital specimens: Importance of culture and antimicrobial susceptibility surveillance.
- Author
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Arregui Garcia I, Portillo Bordonabe ME, Gil Setas A, and Ezpeleta Baquedano C
- Subjects
- Humans, Anti-Bacterial Agents therapeutic use, Genitalia, Haemophilus parainfluenzae, Haemophilus Infections epidemiology
- Published
- 2023
- Full Text
- View/download PDF
35. The impact of plasma 25-hydroxyvitamin D on pulmonary function and exercise physiology in cystic fibrosis: A multicentre retrospective study.
- Author
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Revuelta Iniesta R, Causer AJ, Arregui-Fresneda I, Connett G, Allenby MI, Daniels T, Carroll MP, Urquhart DS, and Saynor ZL
- Subjects
- Adolescent, Adult, Child, Female, Humans, Lung, Male, Prospective Studies, Retrospective Studies, Vitamin D analogs & derivatives, Young Adult, Cystic Fibrosis complications, Exocrine Pancreatic Insufficiency
- Abstract
Background: A 25-hydroxyvitamin D (25OHD) may exert immunomodulatory effects on respiratory health, which may translate to improvements in exercise physiology. Thus, we aimed to investigate whether plasma 25OHD is associated with lung function and aerobic fitness in people with cystic fibrosis (pwCF)., Methods: A multicentre retrospective review of pwCF (> 9 years old) attending the Royal Hospital for Sick Children (Edinburgh) or Wessex CF-Unit (Southampton) was performed between July 2017 and October 2019. Demographic and clinical data were collected. Plasma 25OHD measured closest in time to clinical cardiopulmonary exercise testing and/or spirometry [forced expiratory volume (FEV
1 )% predicted] was recorded. Pancreatic insufficiency was diagnosed based on faecal elastase of < 100 µg g-1 . We performed multiple-regression analysis with aerobic fitness outcomes [peak oxygen uptake (VO2 peak )] and FEV1 % predicted as primary outcomes., Results: Ninety pwCF [mean ± SD age: 19.1 ± 8.6 years, 54 (60%) children, 48 (53%) males and 88 (98%) Caucasian] were included. 25OHD deficiency and insufficiency was 15 (17%) and 44 (49%), respectively. 25OHD deficiency and insufficiency was significantly associated with pancreatic insufficiency (χ2 = 4.8, p = 0.02). Plasma 25OHD was not significantly associated with FEV1 % predicted (r2 = 0.06, p = 0.42, 95% CI = -0.09 to 0.19) or VO2 peak (r2 = 0.04, p = 0.07, 95% CI = -011 to 0.005) in all pwCF. However, 25OHD was significantly associated with both FEV1 % (r2 = 0.15, p = 0.02, 95% CI = 1.99-2.64) and VO2 peak (r2 = 0.13, p = 0.05, 95% CI = -0.26 to -0.005) in the paediatric cohort., Conclusions: We showed that 25OHD is associated with improved lung function and aerobic fitness in children and adolescents with CF. Mechanistic and high-quality prospective studies including both lung function and aerobic fitness as primary outcomes are now warranted., (© 2021 The British Dietetic Association Ltd.)- Published
- 2022
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36. [Cryptosporidiosis in immunosuppressed renal transplant patient].
- Author
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Arregui Garcia I, Elía Lòpez M, Aguinaga Pérez A, Manrique Escola J, and Ezpeleta Baquedano C
- Subjects
- Feces, Humans, Immunocompromised Host, Cryptosporidiosis drug therapy, Kidney Transplantation
- Published
- 2021
- Full Text
- View/download PDF
37. Influenza Vaccination and Risk of SARS-CoV-2 Infection in a Cohort of Health Workers.
- Author
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Martínez-Baz I, Trobajo-Sanmartín C, Arregui I, Navascués A, Adelantado M, Indurain J, Fresán U, Ezpeleta C, and Castilla J
- Abstract
Vaccines may induce positive non-specific immune responses to other pathogens. This study aims to evaluate if influenza vaccination in the 2019-2020 season had any effect on the risk of SARS-CoV-2 confirmed infection in a cohort of health workers. During the first SARS-CoV-2 epidemic wave in Spain, between March and May 2020, a cohort of 11,201 health workers was highly tested by RT-qPCR and/or rapid antibody test when the infection was suspected. Later in June, 8665 of them were tested for total antibodies in serum. A total of 890 (7.9%) health workers were laboratory-confirmed for SARS-CoV-2 infection by any type of test, while no case of influenza was detected. The adjusted odds ratio between 2019-2020 influenza vaccination and SARS-CoV-2 confirmed infection was the same (1.07; 95% CI, 0.92-1.24) in both comparisons of positive testers with all others (cohort design) and with negative testers (test-negative design). Among symptomatic patients tested by RT-qPCR, the comparison of positive cases and negative controls showed an adjusted odds ratio of 0.86 (95% CI, 0.68-1.08). These results suggest that influenza vaccination does not significantly modify the risk of SARS-CoV-2 infection. The development of specific vaccines against SARS-CoV-2 is urgent.
- Published
- 2020
- Full Text
- View/download PDF
38. The implications of dysglycaemia on aerobic exercise and ventilatory function in cystic fibrosis.
- Author
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Causer AJ, Shute JK, Cummings MH, Shepherd AI, Wallbanks SR, Allenby MI, Arregui-Fresneda I, Bright V, Carroll MP, Connett G, Daniels T, Meredith T, and Saynor ZL
- Subjects
- Adult, Cardiorespiratory Fitness physiology, Correlation of Data, Female, Forced Expiratory Volume, Glucose Intolerance diagnosis, Glucose Intolerance etiology, Humans, Male, Oxygen Consumption, Respiratory Function Tests methods, Respiratory Function Tests statistics & numerical data, Retrospective Studies, Severity of Illness Index, United Kingdom epidemiology, Cystic Fibrosis diagnosis, Cystic Fibrosis epidemiology, Cystic Fibrosis metabolism, Cystic Fibrosis physiopathology, Diabetes Mellitus blood, Diabetes Mellitus diagnosis, Diabetes Mellitus etiology, Exercise physiology, Exercise Test methods, Exercise Test statistics & numerical data, Glucose Tolerance Test methods, Glucose Tolerance Test statistics & numerical data
- Abstract
Background: The development of cystic fibrosis (CF)-related diabetes (CFRD) in paediatric groups is associated with a reduced aerobic fitness. However, this has yet to be investigated in adults with more severe lung disease., Methods: Cardiopulmonary exercise and glycaemic control tests were retrospectively analysed in 46 adults with CF (age: 26.9 y [range: 16.3-66.5 y]; forced expiratory volume in 1s: 65.3% [range: 26.8-105.7%]; 26 males), diagnosed with CFRD (n = 19), impaired glucose tolerance (IGT; n = 8) or normal glucose tolerance (NGT; n = 19)., Results: Maximal oxygen uptake (V˙O
2max ) was reduced in adults with IGT and CFRD compared to their age- and gender-matched counterparts with NGT (p < 0.05); however, there was no difference when lung function was included as a covariate (all p > 0.05). V˙O2max was greater in adults who experienced post-reactive hypoglycaemia vs. NGT without hypoglycaemia (p < 0.05). The frequency of ventilatory limitation (84%, 63% and 37%, respectively; p < 0.05) but not ventilation-perfusion mismatch (42%, 38% and 16%, respectively; p > 0.05), was greater with CFRD and IGT vs. NGT. There was also no difference in arterial oxygen saturation changes between groups (p > 0.05). Gender and body mass index were significant predictors of V˙O2max (adjusted R2 = 0.37, p < 0.01), but glycaemic control did not explain additional variance (p > 0.05)., Conclusions: Adults with CF-related dysglycaemia had a reduced V˙O2max compared to age- and gender-matched counterparts, due to a greater degree of CF lung disease in these populations., Competing Interests: Declaration of Competing Interest None., (Crown Copyright © 2019. Published by Elsevier B.V. All rights reserved.)- Published
- 2020
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- View/download PDF
39. Large-scale distribution of tuna species in a warming ocean.
- Author
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Erauskin-Extramiana M, Arrizabalaga H, Hobday AJ, Cabré A, Ibaibarriaga L, Arregui I, Murua H, and Chust G
- Subjects
- Animals, Atlantic Ocean, Ecosystem, Population Dynamics, Climate Change, Tuna
- Abstract
Tuna are globally distributed species of major commercial importance and some tuna species are a major source of protein in many countries. Tuna are characterized by dynamic distribution patterns that respond to climate variability and long-term change. Here, we investigated the effect of environmental conditions on the worldwide distribution and relative abundance of six tuna species between 1958 and 2004 and estimated the expected end-of-the-century changes based on a high-greenhouse gas concentration scenario (RCP8.5). We created species distribution models using a long-term Japanese longline fishery dataset and two-step generalized additive models. Over the historical period, suitable habitats shifted poleward for 20 out of 22 tuna stocks, based on their gravity centre (GC) and/or one of their distribution limits. On average, tuna habitat distribution limits have shifted poleward 6.5 km per decade in the northern hemisphere and 5.5 km per decade in the southern hemisphere. Larger tuna distribution shifts and changes in abundance are expected in the future, especially by the end-of-the-century (2080-2099). Temperate tunas (albacore, Atlantic bluefin, and southern bluefin) and the tropical bigeye tuna are expected to decline in the tropics and shift poleward. In contrast, skipjack and yellowfin tunas are projected to become more abundant in tropical areas as well as in most coastal countries' exclusive economic zones (EEZ). These results provide global information on the potential effects of climate change in tuna populations and can assist countries seeking to minimize these effects via adaptive management., (© 2019 John Wiley & Sons Ltd.)
- Published
- 2019
- Full Text
- View/download PDF
40. Detecting the presence-absence of bluefin tuna by automated analysis of medium-range sonars on fishing vessels.
- Author
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Uranga J, Arrizabalaga H, Boyra G, Hernandez MC, Goñi N, Arregui I, Fernandes JA, Yurramendi Y, and Santiago J
- Subjects
- Animals, Atlantic Ocean, Population Surveillance methods, Sound, Fisheries, Tuna
- Abstract
This study presents a methodology for the automated analysis of commercial medium-range sonar signals for detecting presence/absence of bluefin tuna (Tunnus thynnus) in the Bay of Biscay. The approach uses image processing techniques to analyze sonar screenshots. For each sonar image we extracted measurable regions and analyzed their characteristics. Scientific data was used to classify each region into a class ("tuna" or "no-tuna") and build a dataset to train and evaluate classification models by using supervised learning. The methodology performed well when validated with commercial sonar screenshots, and has the potential to automatically analyze high volumes of data at a low cost. This represents a first milestone towards the development of acoustic, fishery-independent indices of abundance for bluefin tuna in the Bay of Biscay. Future research lines and additional alternatives to inform stock assessments are also discussed., Competing Interests: The authors have declared that no competing interests exist.
- Published
- 2017
- Full Text
- View/download PDF
41. Correction: New Archaeological Evidence for an Early Human Presence at Monte Verde, Chile.
- Author
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Dillehay TD, Ocampo C, Saavedra J, Sawakuchi AO, Vega RM, Pino M, Collins MB, Cummings LS, Arregui I, Villagran XS, Hartmann GA, Mella M, González A, and Dix G
- Published
- 2015
- Full Text
- View/download PDF
42. New Archaeological Evidence for an Early Human Presence at Monte Verde, Chile.
- Author
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Dillehay TD, Ocampo C, Saavedra J, Sawakuchi AO, Vega RM, Pino M, Collins MB, Scott Cummings L, Arregui I, Villagran XS, Hartmann GA, Mella M, González A, and Dix G
- Subjects
- Carbon, Chile, Culture, Humans, Radioisotopes, Archaeology, Human Migration, Paleontology
- Abstract
Questions surrounding the chronology, place, and character of the initial human colonization of the Americas are a long-standing focus of debate. Interdisciplinary debate continues over the timing of entry, the rapidity and direction of dispersion, the variety of human responses to diverse habitats, the criteria for evaluating the validity of early sites, and the differences and similarities between colonization in North and South America. Despite recent advances in our understanding of these issues, archaeology still faces challenges in defining interdisciplinary research problems, assessing the reliability of the data, and applying new interpretative models. As the debates and challenges continue, new studies take place and previous research reexamined. Here we discuss recent exploratory excavation at and interdisciplinary data from the Monte Verde area in Chile to further our understanding of the first peopling of the Americas. New evidence of stone artifacts, faunal remains, and burned areas suggests discrete horizons of ephemeral human activity in a sandur plain setting radiocarbon and luminescence dated between at least ~18,500 and 14,500 cal BP. Based on multiple lines of evidence, including sedimentary proxies and artifact analysis, we present the probable anthropogenic origins and wider implications of this evidence. In a non-glacial cold climate environment of the south-central Andes, which is challenging for human occupation and for the preservation of hunter-gatherer sites, these horizons provide insight into an earlier context of late Pleistocene human behavior in northern Patagonia.
- Published
- 2015
- Full Text
- View/download PDF
43. Wave heating of the solar atmosphere.
- Author
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Arregui I
- Abstract
Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their significance has increased because of their potential as a remote diagnostic tool and their presumed contribution to plasma heating processes. We discuss our current understanding of coronal heating by magnetic waves, based on recent observational evidence and theoretical advances. The discussion starts with a selection of observational discoveries that have brought magnetic waves to the forefront of the coronal heating discussion. Then, our theoretical understanding of the nature and properties of the observed waves and the physical processes that have been proposed to explain observations are described. Particular attention is given to the sequence of processes that link observed wave characteristics with concealed energy transport, dissipation and heat conversion. We conclude with a commentary on how the combination of theory and observations should help us to understand and quantify magnetic wave heating of the solar atmosphere., (© 2015 The Author(s) Published by the Royal Society. All rights reserved.)
- Published
- 2015
- Full Text
- View/download PDF
44. Postoperative chyle leak after major pancreatic resections in patients who receive enteral feed: risk factors and management options.
- Author
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Abu Hilal M, Layfield DM, Di Fabio F, Arregui-Fresneda I, Panagiotopoulou IG, Armstrong TH, Pearce NW, and Johnson CD
- Subjects
- Adult, Aged, Aged, 80 and over, Drainage, Female, Follow-Up Studies, Humans, Logistic Models, Male, Middle Aged, Multivariate Analysis, Parenteral Nutrition, Total, Postoperative Care methods, Postoperative Complications diagnosis, Postoperative Complications prevention & control, Postoperative Complications therapy, Retrospective Studies, Risk Factors, Treatment Outcome, Chyle, Enteral Nutrition adverse effects, Pancreatectomy, Pancreaticoduodenectomy, Postoperative Care adverse effects, Postoperative Complications etiology
- Abstract
Background: Chyle leak complicates 1.3-10.8 % of pancreatic resections. Universal use of parenteral nutrition following pancreatic resection may reduce the incidence of chyle leak. However, this denies the majority of patients who do not develop chyle leak the benefits of enteral nutrition (EN). The present study aimed to identify risk factors for chyle leak following pancreatic resection within a single institution where EN was used universally., Methods: All patients who underwent pancreatic resection between January 2007 and December 2010 were identified retrospectively. The patients had been treated according to a common unit protocol of enteral feeding; those developing chyle leak were switched to a medium-chain triglyceride (MCT) regimen. Clinical progress and recovery after surgery was evaluated. Multivariate analysis was performed to identify factors associated with chyle leak., Results: A total of 245 patients underwent major pancreatic resection (231 pancreatoduodenectomy, 14 total pancreatectomy). Chyle leak complicated 40 cases (16.3 %). After multivariate analysis, both extensive lymphadenectomy (P = 0.002) and postoperative portal/mesenteric venous thrombosis (PVT) (P = 0.009) were independently linked with a higher incidence of chyle leak. The development of chyle leak was not associated with poorer survival or prolonged duration of hospital stay. It was associated with a significantly increased duration of abdominal drainage and reduced likelihood of early hospital discharge (P = 0.026)., Conclusions: Universal use of enteral feeding is associated with a high rate of chyle leak following pancreatic resection. Patients undergoing extensive lymphadenectomy or those who develop PVT postoperatively are at increased risk. Development of chyle leak was not associated with additional morbidity or mortality following implementation of an MCT regimen. The implication is that reactive management of chyle leak with conversion to a MCT predominant diet is safe.
- Published
- 2013
- Full Text
- View/download PDF
45. Titanium allergy in dental implant patients: a clinical study on 1500 consecutive patients.
- Author
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Sicilia A, Cuesta S, Coma G, Arregui I, Guisasola C, Ruiz E, and Maestro A
- Subjects
- Adult, Case-Control Studies, Dental Implantation, Endosseous adverse effects, Dental Restoration Failure, Female, Humans, Male, Middle Aged, Reference Values, Titanium adverse effects, Dental Alloys adverse effects, Dental Implants adverse effects, Hypersensitivity immunology, Titanium immunology
- Abstract
Background: In dentistry, allergic reactions to Ti implants have not been studied, nor considered by professionals. Placing permanent metal dental implants in allergic patients can provoke type IV or I reactions. Several symptoms have been described, from skin rashes and implant failure, to non-specific immune suppression., Objective: Our objective was to evaluate the presence of titanium allergy by the anamnesis and examination of patients, together with the selective use of cutaneous and epicutaneous testing, in patients treated with or intending to receive dental implants of such material., Material and Methods: Thirty-five subjects out of 1500 implant patients treated and/or examined (2002-2004) were selected for Ti allergy analysis. Sixteen presented allergic symptoms after implant placement or unexplained implant failures [allergy compatible response group (ACRG)], while 19 had a history of other allergies, or were heavily Ti exposed during implant surgeries or had explained implant failures [predisposing factors group (PFG)]. Thirty-five controls were randomly selected (CG) in the Allergy Centre. Cutaneous and epicutaneous tests were carried out., Results: Nine out of the 1500 patients displayed positive (+) reactions to Ti allergy tests (0.6%): eight in the ACRG (50%), one in the PFG (5.3%)(P=0.009) and zero in the control group. Five positives were unexplained implant failures (five out of eight)., Conclusions: Ti allergy can be detected in dental implant patients, even though its estimated prevalence is low (0.6%). A significantly higher risk of positive allergic reaction was found in patients showing post-op allergy compatible response (ACRG), in which cases allergy tests could be recommended.
- Published
- 2008
- Full Text
- View/download PDF
46. Damping of magnetohydrodynamic waves by resonant absorption in the solar atmosphere.
- Author
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Goossens M, Andries J, and Arregui I
- Abstract
In the last decade we have been overwhelmed by an avalanche of discoveries of magnetohydrodynamic (MHD) waves by the Solar and Heliospheric Observatory and Transition Region and Coronal Explorer observatories. Both standing and propagating versions of fast magnetoacoustic and slow magnetoacoustic MHD waves have been detected. Information on the damping times and damping distances of these waves is less detailed and less accurate than that on periods and amplitudes. Nevertheless, observations show the damping times and damping lengths are often short. Also, different types of MHD waves in different types of magnetic structures likely require different damping mechanisms. The phenomenon of fast damping is well documented for the standing fast magnetosonic kink waves in coronal loops. This paper concentrates on standing fast magnetosonic waves. It reports on results on periods and damping times due to resonant absorption in one-dimensional and two-dimensional models of coronal loops. Special attention is given to multiple modes.
- Published
- 2006
- Full Text
- View/download PDF
47. Quasi-mode damping in two-dimensional fully non-uniform coronal loops.
- Author
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Arregui I, Van Doorsselaere T, Andries J, Goossens M, and Kimpe D
- Abstract
Resonantly damped fast kink quasi-modes are computed in fully resistive magnetohydrodynamics for fully non-uniform two-dimensional equilibrium models. The equilibrium model is a straight cylindrically symmetric flux tube with a plasma density that is non-uniform both across and along the loop. The variation of density across the loop can cover the whole loop. Our results indicate that the period and damping of coronal loop oscillations mainly depend on the density contrast and the inhomogeneity length-scale and are independent of the details of longitudinal stratification. This study extends previous studies on coronal loop oscillations, and allows for a better comparison between observations and theory.
- Published
- 2006
- Full Text
- View/download PDF
48. Evaluation of the efficacy of two potassium nitrate bioadhesive gels (5% and 10%) in the treatment of dentine hypersensitivity. A randomised clinical trial.
- Author
-
Frechoso SC, Menéndez M, Guisasola C, Arregui I, Tejerina JM, and Sicilia A
- Subjects
- Adhesives administration & dosage, Adult, Aged, Analysis of Variance, Female, Follow-Up Studies, Gels, Humans, Male, Middle Aged, Nitrates administration & dosage, Patient Satisfaction, Placebos, Potassium Compounds administration & dosage, Single-Blind Method, Statistics, Nonparametric, Tooth Root drug effects, Treatment Outcome, Adhesives therapeutic use, Dentin Sensitivity drug therapy, Nitrates therapeutic use, Potassium Compounds therapeutic use
- Abstract
Aim: A randomised clinical trial was designed to compare the immediate efficacy (48-96 h) of two treatments with bioadhesive gels with different concentrations of potassium nitrate (NK 5% versus NK 10%) on dentine hypersensitivity (DH). We evaluated DH by means of the use of the evaporative stimulus (ES), as the main outcome, using a placebo control group as reference., Patients and Methods: Forty-five consecutive patients who, after stimulation with a blast of air, had at least one tooth with DH > or = 2 according to the verbal ratings scale (VRS) scale were selected. They were randomly treated with a bioadhesive gel with 5% NK, 10% NK or a placebo gel without NK. The DH was evaluated at baseline, days 2, 4, 7 and 14 by an examiner blind to the procedure. The response to the ES with a blast of air, to the tactile stimulation with a probe and the subjective evaluation of the patient measured on the VRS scale were recorded. Statistical analysis was made using the Kruskal-Wallis test., Results: A greater reduction of DH after ES was observed after 48 h of treatment in the NK10% group (35.8%) compared to the NK5% group and placebo group (11.8% and 13.4%, respectively). This difference increased significantly at 96 h (p=0.003). No significant differences were observed for the other variables. These preliminary results may support the usefulness of an NK 10% gel to reduce the DH after stimulation with a blast of air during the first 4 days of its appearance.
- Published
- 2003
- Full Text
- View/download PDF
49. Home oral hygiene revisited. Options and evidence.
- Author
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Sicilia A, Arregui I, Gallego M, Cabezas B, and Cuesta S
- Subjects
- Dental Devices, Home Care, Equipment Design, Gingival Hemorrhage prevention & control, Humans, Oral Hygiene instrumentation, Toothbrushing instrumentation, Dental Plaque prevention & control, Gingivitis prevention & control, Oral Hygiene methods, Self Care
- Abstract
In regard to the limited literature on the subject, and the contradictions observed, we can not conclude that the types of manual brushes produce clinically important effects on the patients' gingival health, or that these effects can be detected consistently. However, the best results have been obtained with new brush designs, and future studies are necessary to clarify the existing contradictions. There is a clear need of long-term studies which comparatively evaluate the ability to reduce gingivitis and plaque with the newly designed brushes. On the other hand, there is evidence that supports the use of powered toothbrushes in the general population, especially those of the oscillating-rotating and counter-rotational type, as they have shown their ability to reduce gingival bleeding or inflammation, and dental plaque with greater efficacy than manual brushes. There is a clear need of long-term trials on the efficacy of powered brushes in orthodontic patients. With the existing studies we can conclude that there is limited evidence that orthodontic patients using a powered toothbrush show a slight, but significant, reduction of bleeding, compared with users of manual brushes. No conclusion can be made concerning the type of brush to be used. The techniques of interproximal oral hygiene, fundamentally the use of dental floss and interproximal brushes, appear to add additional benefits, in terms of plaque reduction, when they are associated with conventional manual brushes. Further long-term studies are necessary to confirm their efficacy in the reduction of gingival bleeding or inflammation. The choice of the type of technique must be made in relation to the characteristics of the patient: dental floss could be indicated in individuals with closed interdental spaces, and inter-proximal brushes in periodontal patients, or in those with open embrasures.
- Published
- 2003
50. A systematic review of powered vs manual toothbrushes in periodontal cause-related therapy.
- Author
-
Sicilia A, Arregui I, Gallego M, Cabezas B, and Cuesta S
- Subjects
- Adult, Electricity, Equipment Design, Gingival Recession etiology, Health Education, Dental, Humans, Periodontal Index, Randomized Controlled Trials as Topic, Sonication, Tooth Abrasion etiology, Toothbrushing adverse effects, Dental Plaque therapy, Periodontal Diseases therapy, Toothbrushing instrumentation
- Abstract
Background: Power-driven toothbrushes (PDT) have been designed to improve the efficacy of oral hygiene. It is not clear how they compare in efficacy with manual toothbrushes in cause-related periodontal therapy., Objectives: To evaluate the effectiveness of the use of a PDT as compared with a manual toothbrush (MT), in terms of gingival bleeding or inflammation resolution, in cause-related periodontal therapy., Material and Methods: An electronic (MEDLINE and Cochrane Oral Health Group Specialised Trials Register) and a manual search were made to detect studies which permitted the evaluation of the efficacy of PDT in the reduction of gingival bleeding or inflammation, and their effect on other secondary variables. Only randomized studies in adults, published in English up to June 2001, which compared a PDT with an MT, and evaluated the evolution of gingival bleeding or inflammation were included. The selection of articles, extraction of data and assessment of validity were made independently by several reviewers., Results: Twenty-one studies were finally selected. The heterogeneity of the data prevented a quantitative analysis. A higher efficacy in the reduction of gingival bleeding or inflammation in the PDT patients was detected in 10 studies. This effect appears to be related to the capacity to reduce plaque, and is more evident in counter-rotational and oscillating-rotating brushes. No solid evidence was found for a higher efficacy of sonic brushes. In short-term studies with prophylaxis after initial examination, independently of the type of PDT tested, no significant differences were found., Conclusion: The use of PDT, especially counter-rotational and oscillating-rotating brushes, can be beneficial in reducing the levels of gingival bleeding or inflammation. There is a need for methodological homogeneity in future studies in this field to enable quantitative analysis of their results.
- Published
- 2002
- Full Text
- View/download PDF
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