The contribution of starspots to coronal structure

Significant progress has been made recently in our understanding of the structure of stellar magnetic fields, thanks to advances in detection methods such as Zeeman-Doppler Imaging. The extrapolation of this surface magnetic field into the corona has provided 3D models of the coronal magnetic field and plasma. This method is sensitive mainly to the magnetic field in the bright regions of the stellar surface. The dark (spotted) regions are censored because the Zeeman signature there is suppressed. By modelling the magnetic field that might have been contained in these spots, we have studied the effect that this loss of information might have on our understanding of the coronal structure. As examples, we have chosen two stars (V374 peg and AB Dor) that have very different magnetograms and patterns of spot coverage. We find that the effect of the spot field depends not only on the relative amount of flux in the spots, but also its distribution across the stellar surface. For a star such as AB Dor with a high spot coverage and a large polar spot, at its greatest effect the spot field may almost double the fraction of the flux that is open (hence decreasing the spindown time) while at the same time increasing the X-ray emission measure by two orders of magnitude and significantly affecting the X-ray rotational modulation.Comment: 10 pages, 10 figure

Witnessing single-photon entanglement with local homodyne measurements: analytical bounds and robustness to losses

Single-photon entanglement is one of the primary resources for quantum networks, including quantum repeater architectures. Such entanglement can be revealed with only local homodyne measurements through the entanglement witness presented in [Morin et al. Phys. Rev. Lett. 110, 130401 (2013)]. Here, we provide an extended analysis of this witness by introducing analytical bounds and by reporting measurements confirming its great robustness with regard to losses. This study highlights the potential of optical hybrid methods, where discrete entanglement is characterized through continuous-variable measurements

Etude de fils semi-conducteurs dopés individuels par techniques locales d'analyse de surface

This thesis addresses the characterization of individual doped semiconductors microand nanowires by photoemission electron microscopy (XPEEM) and near field techniques : Kelvin probe force microscopy (KFM) and scanning capacitance microscopy. The aim of this study is to evaluate the benefits of contactless surface methods, thanks to local work function and core level binding energy measurements, for the study of phenomena linked to doping in such objects, like for example axial uniformity. First, we highlight the importance of sample preparation required for these techniques: wires transfer methods, substrate/wire match, and preanalysis characterization influence. Then we present two case studies addressing technological issues: Si doped gallium nitride microwires (2μm diameter) for solid state lighting, and p-n junction nanowires (100 nm diameter) for low power microelectronics. In the first case, we have performed SCM for quick identification of n doping axial heterogeneity, then performed spectroscopic XPEEM using synchrotron radiation to, first, estimate local work function and surface band bending, then clarify surface silicon incorporation highlighting growth process influence over intentional (si on Ga sites) and unintentional doping (si on nitrogen vacancy). Complementary measurements on both axial and radial section of wires have been led by Auger microscopy and ToF-SIMS, highlighting silicon incorporation preferentially at the surface of the microwires. Regarding p-n junctions, after partial removal of surface oxide, we have linked results obtained independently by KFM and XPEEM. Both methods highlighted a weak local work function difference between n-doped and p-doped part, partly explained by Fermi level pinning induced by surface states.Ce mémoire de thèse traite de la caractérisation de microfils et nanofils semi conducteurs dopés individuels par microscopie à émission de photoélectrons X (XPEEM) complétée par des techniques de champ proche électrique: Kelvin force microscopy (KFM) et scanning capacitance microscopy (SCM). L'objectif est d'évaluer l'apport des méthodes locales de surface « sans contact », grâce à la mesure du travail de sortie local et de l'énergie de liaison des niveaux de cœur, pour l'étude des phénomènes liés au dopage dans ces objets, comme par exemple l'uniformité longitudinale. Nous mettons d'abord en évidence l'importance de la préparation des échantillons pour la mise en œuvre des techniques citées: méthodes de transfert des fils, adéquation du substrat, influence des caractérisations pré-analyse. Nous présentons ensuite deux principales études de cas en lien avec une problématique technologique : les microfils de nitrure de gallium dopés Si (diamètre 2 µm) pour applications dans l'éclairage à l'état solide, et les jonctions pn à nanofils de Si (diamètre 100 nm) pour la nanoélectronique basse puissance. Dans le premier cas, nous avons mis en œuvre la SCM pour l'identification rapide de l'hétérogénéité axiale du dopage n, puis avons utilisé l'imagerie XPEEM spectroscopique avec excitation synchrotron pour, d'abord, estimer le travail de sortie local et la courbure de bande en surface; ensuite, élucider les modes d'incorporation du silicium en surface, qui pointent notamment sur la sensibilité des conditions d'élaboration dans la part du dopage intentionnel (Si en sites Ga) et non intentionnel (Si sur sites lacunaires en azote). (Des mesures complémentaires sur sections radiales et longitudinales de fils, par microscopie Auger et spectrométrie ToF-SIMS montrent une incorporation du Si limitée à la surface des microfils). Concernant les jonctions pn à nanofils de silicium étudiées après retrait partiel de l'oxyde de surface, nous avons mis en relation des résultats obtenus indépendamment par KFM et par XPEEM. Ils mettent conjointement en lumière une très faible différence de travail de sortie local entre partie n et partie p, et qui semble en partie expliquée par un ancrage du niveau de Fermi en surface

Processus dynamos dans les étoiles entièrement convectives

Dans les étoiles de type solaire la génération de champ magnétique par effet dynamo se concentre dans la tachocline, une fine zone de fort cisaillement à l'interface entre le cœur radiatif et l'enveloppe convective. En dessous de 0.35 masse solaire, les étoiles de la séquence principale sont entièrement convectives et ne possèdent donc pas de tachocline. Or certaines de ces étoiles sont très actives, et des champs magnétiques très intenses ont été mesurés. La dynamo de ces objets doit donc reposer sur des processus physiques différents de ceux à l'œuvre dans le Soleil. En dépit des avancées théoriques récentes, la dynamo des étoiles entièrement convective reste mal comprise. La partie observationnelle de ce travail a consisté en l'étude d'un échantillon d'étoiles situées de part et d'autre de la limite entièrement convective à partir d'observations spectropolarimétriques et de la technique d'imagerie Zeeman-Doppler. Cela a permis d'analyser comment les paramètres stellaires, période de rotation et masse, influent sur le champ magnétique à grande échelle. Un changement brutal de topologie magnétique des naines M est mis en évidence à proximité de la limite entièrement convective. Un comportement inattendu est également détecté en dessous de 0.2 masse solaire : des étoiles de paramètres stellaires quasi-identiques présentent des topologies magnétiques radicalement différentes. Ce travail observationnel est doublé d'une approche numérique : des simulations MHD 3D "star-in-a-box" visent à mieux comprendre les divergences qui existent entre les premières simulations et les observations.In solar-type stars, the generation of magnetic field through dynamo effect concentrates in the tachocline, a thin layer of strong shear located at the interface between the radiative core and the convective envelope. Below 0.35 solar mass, main sequence stars are fully convective and thus do not possess a tachocline. And yet, some fully-convective dwarfs are very active, and strong photospheric magnetic fields have been detected. The generation of magnetic field in these objects therefore relies on non-solar dynamo processes.In spite of recent theoretical advances, dynamo processes in fully convective dwarfs remain poorly understood. The observational part of this work has consisted in a spectropolarimetric survey of a small sample of M dwarfs located on both sides of the fully-convective divide. Large-scale magnetic topologies and their dependency on main stellar parameters - mass and rotation period - have been investigated with Zeeman-Doppler Imaging techniques. This study reveals a sharp transition in magnetic topologies of M dwarfs close to the fully convective boundary. The presence of an unexpected behaviour below 0.2 solar mass is also evidenced : stars with similar parameters host radically different large-scale magnetic fields

Effect of the heralding detector properties on the conditional generation of single-photon states

Single-photons play an important role in emerging quantum technologies and information processing. An efficient generation technique consists in preparing such states via a conditional measurement on photon-number correlated beams: the detection of a single-photon on one of the beam can herald the generation of a single-photon state on the other one. Such scheme strongly depends on the heralding detector properties, such as its quantum efficiency, noise or photon-number resolution ability. These parameters affect the preparation rate and the fidelity of the generated state. After reviewing the theoretical description of optical detectors and conditional measurements, and how both are here connected, we evaluate the effects of these properties and compare two kind of devices, a conventional on/off detector and a two-channel detector with photon-number resolution ability

Witnessing trustworthy single-photon entanglement with local homodyne measurements

Single-photon entangled states, i.e. states describing two optical paths sharing a single photon, constitute the simplest form of entanglement. Yet they provide a valuable resource in quantum information science. Specifically, they lie at the heart of quantum networks, as they can be used for quantum teleportation, swapped and purified with linear optics. The main drawback of such entanglement is the difficulty in measuring it. Here, we present and experimentally test an entanglement witness allowing one not only to say whether a given state is path-entangled but also that entanglement lies in the subspace where the optical paths are each filled with one photon at most, i.e. refers to single-photon entanglement. It uses local homodyning only and relies on no assumption about the Hilbert space dimension of the measured system. Our work provides a simple and trustful method for verifying the proper functioning of future quantum networks.Comment: published versio

Rainfall modeling for integrating radar information into hydrological model

A spatial rainfall model was applied to radar data of air mass thunderstorms to yield a rainstorm representation as a set of convective rain cells. The modeled rainfall was used as input into hydrological model, instead of the standard radar-grid data. This approach allows a comprehensive linkage between runoff responses and rainfall structures. Copyright © 2005 Royal Meteorological Society

A novel p21-activated kinase binds the actin and microtubule networks and induces microtubule stabilization

Coordination of the different cytoskeleton networks in the cell is of central importance for morphogenesis, organelle transport, and motility. The Rho family proteins are well characterized for their effects on the actin cytoskeleton, but increasing evidence indicates that they may also control microtubule (MT) dynamics. Here, we demonstrate that a novel Cdc42/Rac effector, X-p21-activated kinase (PAK)5, colocalizes and binds to both the actin and MT networks and that its subcellular localization is regulated during cell cycle progression. In transfected cells, X-PAK5 promotes the formation of stabilized MTs that are associated in bundles and interferes with MTs dynamics, slowing both the elongation and shrinkage rates and inducing long paused periods. X-PAK5 subcellular localization is regulated tightly, since coexpression with active Rac or Cdc42 induces its shuttling to actin-rich structures. Thus, X-PAK5 is a novel MT-associated protein that may communicate between the actin and MT networks during cellular responses to environmental conditions