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1.
Nature ; 596(7871): 221-226, 2021 08.
Artículo en Inglés | MEDLINE | ID: mdl-34381232

RESUMEN

Research on magnetic confinement of high-temperature plasmas has the ultimate goal of harnessing nuclear fusion for the production of electricity. Although the tokamak1 is the leading toroidal magnetic-confinement concept, it is not without shortcomings and the fusion community has therefore also pursued alternative concepts such as the stellarator. Unlike axisymmetric tokamaks, stellarators possess a three-dimensional (3D) magnetic field geometry. The availability of this additional dimension opens up an extensive configuration space for computational optimization of both the field geometry itself and the current-carrying coils that produce it. Such an optimization was undertaken in designing Wendelstein 7-X (W7-X)2, a large helical-axis advanced stellarator (HELIAS), which began operation in 2015 at Greifswald, Germany. A major drawback of 3D magnetic field geometry, however, is that it introduces a strong temperature dependence into the stellarator's non-turbulent 'neoclassical' energy transport. Indeed, such energy losses will become prohibitive in high-temperature reactor plasmas unless a strong reduction of the geometrical factor associated with this transport can be achieved; such a reduction was therefore a principal goal of the design of W7-X. In spite of the modest heating power currently available, W7-X has already been able to achieve high-temperature plasma conditions during its 2017 and 2018 experimental campaigns, producing record values of the fusion triple product for such stellarator plasmas3,4. The triple product of plasma density, ion temperature and energy confinement time is used in fusion research as a figure of merit, as it must attain a certain threshold value before net-energy-producing operation of a reactor becomes possible1,5. Here we demonstrate that such record values provide evidence for reduced neoclassical energy transport in W7-X, as the plasma profiles that produced these results could not have been obtained in stellarators lacking a comparably high level of neoclassical optimization.

2.
Phys Rev Lett ; 130(23): 239901, 2023 Jun 09.
Artículo en Inglés | MEDLINE | ID: mdl-37354427

RESUMEN

This corrects the article DOI: 10.1103/PhysRevLett.128.175001.

3.
Phys Rev Lett ; 128(17): 175001, 2022 Apr 29.
Artículo en Inglés | MEDLINE | ID: mdl-35570436

RESUMEN

Any collisionless plasma possesses some "available energy" (AE), defined as that part of the thermal energy that can be converted into instabilities and turbulence. Here, we present a calculation of the AE carried by magnetically trapped electrons in a flux tube of collisionless plasma. The AE is compared with nonlinear simulations of the energy flux resulting from collisionless turbulence driven by trapped-electron modes in various magnetic geometries. The numerical calculation of AE is rapid and shows a strong correlation with the simulated energy fluxes, which can be expressed as a power law and understood in terms of a simple model.

5.
Phys Rev Lett ; 127(15): 155001, 2021 Oct 08.
Artículo en Inglés | MEDLINE | ID: mdl-34678019

RESUMEN

A family of rigorous upper bounds on the growth rate of local gyrokinetic instabilities in magnetized plasmas is derived from the evolution equation for the Helmholtz free energy. These bounds hold for both electrostatic and electromagnetic instabilities, regardless of the number of particle species, their collision frequency, and the geometry of the magnetic field. A large number of results that have earlier been derived in special cases and observed in numerical simulations are thus brought into a unifying framework. These bounds apply not only to linear instabilities but also imply an upper limit to the nonlinear growth of the free energy.

6.
Phys Rev Lett ; 124(9): 095001, 2020 Mar 06.
Artículo en Inglés | MEDLINE | ID: mdl-32202856

RESUMEN

It is shown that the magnetic-field coils of a stellarator can, at least in principle, be substantially simplified by the use of permanent magnets. Such magnets cannot create toroidal magnetic flux, but they can be used to shape the plasma and thus to create poloidal flux and rotational transform, thereby easing the requirements on the magnetic-field coils. As an example, a quasiaxisymmetric stellarator configuration is constructed with only 8 circular coils (all identical) and permanent magnets.

7.
Phys Rev Lett ; 125(7): 075001, 2020 Aug 14.
Artículo en Inglés | MEDLINE | ID: mdl-32857529

RESUMEN

We theoretically assess two mechanisms thought to be responsible for the enhanced performance observed in plasma discharges of the Wendelstein 7-X stellarator experiment fueled by pellet injection. The effects of the ambipolar radial electric field and the electron density peaking on the turbulent ion heat transport are separately evaluated using large-scale gyrokinetic simulations. The essential role of the stellarator magnetic geometry is demonstrated, by comparison with a tokamak.

8.
Phys Rev Lett ; 119(13): 139901, 2017 09 29.
Artículo en Inglés | MEDLINE | ID: mdl-29341678

RESUMEN

This corrects the article DOI: 10.1103/PhysRevLett.118.105002.

9.
Phys Rev Lett ; 118(10): 105002, 2017 Mar 10.
Artículo en Inglés | MEDLINE | ID: mdl-28339251

RESUMEN

In the complex 3D magnetic fields of stellarators, ion-temperature-gradient turbulence is shown to have two distinct saturation regimes, as revealed by petascale numerical simulations and explained by a simple turbulence theory. The first regime is marked by strong zonal flows and matches previous observations in tokamaks. The newly observed second regime, in contrast, exhibits small-scale quasi-two-dimensional turbulence, negligible zonal flows, and, surprisingly, a weaker heat flux scaling. Our findings suggest that key details of the magnetic geometry control turbulence in stellarators.

10.
Phys Rev Lett ; 118(15): 155002, 2017 Apr 14.
Artículo en Inglés | MEDLINE | ID: mdl-28452542

RESUMEN

A potential threat to the performance of magnetically confined fusion plasmas is the problem of impurity accumulation, which causes the concentration of highly charged impurity ions to rise uncontrollably in the center of the plasma and spoil the energy confinement by excessive radiation. It has long been thought that the collisional transport of impurities in stellarators always leads to such an accumulation (if the electric field points inwards, which is usually the case), whereas tokamaks, being axisymmetric, can benefit from "temperature screening," i.e., an outward flux of impurities driven by the temperature gradient. Here it is shown, using analytical techniques supported by results from a new numerical code, that such screening can arise in stellarator plasmas, too, and indeed does so in one of the most relevant operating regimes, where the impurities are highly collisional while the bulk plasma is at low collisionality.

11.
Phys Rev Lett ; 113(13): 135003, 2014 Sep 26.
Artículo en Inglés | MEDLINE | ID: mdl-25302897

RESUMEN

It is shown that magnetically confined electron-positron plasmas can enjoy remarkable stability properties. Many of the microinstabilities driving turbulence and transport in electron-ion plasmas are absent if the density is so low that the Debye length is significantly larger than the gyroradius. In some magnetic configurations, almost complete linear stability may be attainable in large parts of the parameter space.

12.
Phys Rev Lett ; 113(15): 155001, 2014 Oct 10.
Artículo en Inglés | MEDLINE | ID: mdl-25375712

RESUMEN

Turbulence is widely expected to limit the confinement and, thus, the overall performance of modern neoclassically optimized stellarators. We employ novel petaflop-scale gyrokinetic simulations to predict the distribution of turbulence fluctuations and the related transport scaling on entire stellarator magnetic surfaces and reveal striking differences to tokamaks. Using a stochastic global-search optimization method, we derive the first turbulence-optimized stellarator configuration stemming from an existing quasiomnigenous design.

13.
Phys Rev Lett ; 108(24): 245002, 2012 Jun 15.
Artículo en Inglés | MEDLINE | ID: mdl-23004281

RESUMEN

It is shown that in perfectly quasi-isodynamic stellarators, trapped particles with a bounce frequency much higher than the frequency of the instability are stabilizing in the electrostatic and collisionless limit. The collisionless trapped-particle instability is therefore stable as well as the ordinary electron-density-gradient-driven trapped-electron mode. This result follows from the energy balance of electrostatic instabilities and is thus independent of all other details of the magnetic geometry.

14.
Phys Rev Lett ; 107(24): 245002, 2011 Dec 09.
Artículo en Inglés | MEDLINE | ID: mdl-22243005

RESUMEN

The relation between magnetic geometry and the level of ion-temperature-gradient (ITG) driven turbulence in stellarators is explored through gyrokinetic theory and direct linear and nonlinear simulations. It is found that the ITG radial heat flux is sensitive to details of the magnetic configuration that can be understood in terms of the linear behavior of zonal flows. The results throw light on the question of how the optimization of neoclassical confinement is related to the reduction of turbulence.

15.
Int J Oral Maxillofac Surg ; 35(7): 631-5, 2006 Jul.
Artículo en Inglés | MEDLINE | ID: mdl-16540288

RESUMEN

In many cases only the temporary presence of a biomaterial is needed in tissue support, augmentation or replacement. In such cases biodegradable materials are better alternatives than biostable ones. At present, biodegradable polymers are widely used in the field of maxillofacial surgery as sutures, fracture fixation devices and as absorbable membranes. The most often used polymers are aliphatic polyesters, such as polyglycolic acid (PGA) and polylactic acid (PLA). Poly(ortho ester) is a surface eroding polymer, which has been under development since 1970, but is used mostly in drug delivery systems in semisolid form. The aim of this study was to evaluate the tissue reactions of solid poly(ortho ester) (POE), histologically and immunohistochemically. Resorption times and the effect of 2 different sterilization methods (gamma radiation and ethylene oxide) upon resorption were also evaluated. Material was implanted into the tibia and subcutaneously into the mandibular ramus area of 24 rabbits. Follow-up times were 1-10, 14 and 24 weeks. Histological studies showed that POE induces a moderate inflammation in soft tissue and in bone. At 24 week follow-up, inflammation was mild in soft tissue and moderate in bone. In immunohistochemical studies, no highly fluorescent layer of tenascin or fibronectin was found adjacent to the implant. Resorption of gamma-sterilized rods was faster than ethylene oxide-sterilized rods. The total resorption time was more than 24 weeks in both groups. Clinically the healing was uneventful and the implants the well tolerated by the living tissue. This encourages these authors to continue studies with this interesting new material to search for the ideal material for bone filling and fracture fixation.


Asunto(s)
Implantes Absorbibles/efectos adversos , Sustitutos de Huesos/toxicidad , Reacción a Cuerpo Extraño/etiología , Polímeros/toxicidad , Animales , Tejido Conectivo/efectos de los fármacos , Tejido Conectivo/cirugía , Óxido de Etileno/farmacología , Femenino , Fibronectinas/análisis , Rayos gamma , Inmunohistoquímica , Mandíbula/efectos de los fármacos , Mandíbula/cirugía , Conejos , Esterilización/métodos , Tenascina/análisis , Tibia/efectos de los fármacos , Tibia/cirugía
16.
Nat Commun ; 7: 13493, 2016 11 30.
Artículo en Inglés | MEDLINE | ID: mdl-27901043

RESUMEN

Fusion energy research has in the past 40 years focused primarily on the tokamak concept, but recent advances in plasma theory and computational power have led to renewed interest in stellarators. The largest and most sophisticated stellarator in the world, Wendelstein 7-X (W7-X), has just started operation, with the aim to show that the earlier weaknesses of this concept have been addressed successfully, and that the intrinsic advantages of the concept persist, also at plasma parameters approaching those of a future fusion power plant. Here we show the first physics results, obtained before plasma operation: that the carefully tailored topology of nested magnetic surfaces needed for good confinement is realized, and that the measured deviations are smaller than one part in 100,000. This is a significant step forward in stellarator research, since it shows that the complicated and delicate magnetic topology can be created and verified with the required accuracy.

17.
Phys Rev Lett ; 84(3): 495-8, 2000 Jan 17.
Artículo en Inglés | MEDLINE | ID: mdl-11015947

RESUMEN

H-mode operation has been achieved in high current (I(p)>200 kA) plasmas in the START spherical tokamak for both neutral-beam-injection-heated and Ohmic discharges. The transition to H mode features the development of well-defined edge pedestals in density and temperature, which signifies the formation of an edge-transport barrier, and associated edge-localized modes. Recent operation at plasma currents exceeding 250 kA shows that these features are accompanied by increases in energy confinement time. This is the first clear demonstration of the H-mode regime in a spherical tokamak.

18.
Anal Bioanal Chem ; 355(3-4): 357-8, 1996 Jun.
Artículo en Inglés | MEDLINE | ID: mdl-15045411

RESUMEN

The use of an optothermal window (OW) was proposed for the direct (no need for sample preparation) spectroscopic, non-destructive measurement of SO(4)(2-) in water at 1078 cm(-1). The presently determined limit of detection (LOD) of 1 mmol/L is comparable to that provided by CO(2) laser photoacoustic spectroscopy, but about one order of magnitude superior to that obtainable by the ATR method.

19.
J Biochem Biophys Methods ; 34(3): 205-11, 1997 Jun 09.
Artículo en Inglés | MEDLINE | ID: mdl-9314098

RESUMEN

During production of both normal and low-alcohol beers, sugar is fermented to ethanol, carbon dioxide and several flavour products. Tight control of fermentation is necessary in order to keep production costs low, and to prevent formation of excessive ethanol in low-alcohol beer. Several types of control devices based on, e.g., determination of carbon dioxide, ethanol, and extract have been developed so far; the main disadvantage of these devices is their unsuitability for on-line applications. Here, the optothermal window was used in a laboratory experiment as a new sensor for real time monitoring fermentation of glucose by Saccharomyces cerevisiae, and the results were compared to those obtained by conventional techniques.


Asunto(s)
Cerveza , Tecnología de Alimentos/métodos , Glucosa/análisis , Saccharomyces cerevisiae/metabolismo , Fermentación , Glucosa/metabolismo , Calefacción
20.
Carbohydr Res ; 88(1): 77-84, 1981 Jan 15.
Artículo en Inglés | MEDLINE | ID: mdl-6970617

RESUMEN

The structures of two capsular polysaccharides elaborated by Haemophilus influenzae type e, strains NCTC 8455 and 8472, respectively, have been investigated, methylation analysis and n.m.r. spectrometry being the principal methods used. It is concluded that the polysaccharides are composed of repeating-units having the following structure: Formula: [See Text]. In the polysaccharide from strain NCTC 8472, all of the repeating-units contain the beta-D-fructofuranosyl group. The polysaccharide from strain NCTC 8455, however, contains only traces of D-fructose, corresponding to approximately one group per 100 repeating-units.


Asunto(s)
Haemophilus influenzae/análisis , Polisacáridos Bacterianos , Conformación de Carbohidratos , Secuencia de Carbohidratos , Metilación , Especificidad de la Especie
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