Monitorización de la temperatura del pie como herramienta en la neuropatía diabética

Objteivo: Valorar si existe relación entre el aumento de temperatura en el pie y la neuropatía diabética periférica. Métodos: La muestra fueron 27 pacientes diabéticos a que se le realizó una exploración neurológica y vascular, además, haciendo uso de un termómetro infrarrojo medimos la temperatura en distintos puntos anatómicos de la planta del pie. Resultados: La temperatura es mayor los pacientes con neuropatía con una diferencia de 2,24ºC (p=0,454) en el pie derecho y 0,86ºC (p=0,589) en el pie izquierdo. Conclusión: Los resultados sugieren que la automonitorización de la temperatura del pie por parte del paciente diabético podría ayudar a reducir la alta incidencia de complicaciones en el pie diabético.

Plasma ion evolution in the wake of a high-intensity ultrashort laser pulse

Experimental investigations of the late-time ion structures formed in the wake of an ultrashort, intense laser pulse propagating in a tenuous plasma have been performed using the proton imaging technique. The pattern found in the wake of the laser pulse shows unexpectedly regular modulations inside a long, finite width channel. On the basis of extensive particle in cell simulations of the plasma evolution in the wake of the pulse, we interpret this pattern as due to ion modulations developed during a two-stream instability excited by the return electric current generated by the wakefield.

Abnormal Functional Connectivity of Hippocampus During Episodic Memory Retrieval Processing Network in Amnestic Mild Cognitive Impairment.

BACKGROUND: Functional connectivity magnetic resonance imaging technique has revealed the importance of distributed network structures in higher cognitive processes in the human brain. The hippocampus has a key role in a distributed network supporting memory encoding and retrieval. Hippocampal dysfunction is a recurrent finding in memory disorders of aging such as amnestic mild cognitive impairment (aMCI) in which learning- and memory-related cognitive abilities are the predominant impairment. The functional connectivity method provides a novel approach in our attempts to better understand the changes occurring in this structure in aMCI patients. METHODS: Functional connectivity analysis was used to examine episodic memory retrieval networks in vivo in twenty 28 aMCI patients and 23 well-matched control subjects, specifically between the hippocampal structures and other brain regions. RESULTS: Compared with control subjects, aMCI patients showed significantly lower hippocampus functional connectivity in a network involving prefrontal lobe, temporal lobe, parietal lobe, and cerebellum, and higher functional connectivity to more diffuse areas of the brain than normal aging control subjects. In addition, those regions associated with increased functional connectivity with the hippocampus demonstrated a significantly negative correlation to episodic memory performance. CONCLUSIONS: aMCI patients displayed altered patterns of functional connectivity during memory retrieval. The degree of this disturbance appears to be related to level of impairment of processes involved in memory function. Because aMCI is a putative prodromal syndrome to Alzheimer's disease (AD), these early changes in functional connectivity involving the hippocampus may yield important new data to predict whether a patient will eventually develop AD.

Roche tomography of the secondary stars in CVs

The secondary stars in cataclysmic variables (CVs) are key to our understanding of the origin, evolution and behaviour of this class of interacting binary. In seeking a fuller understanding of these objects, the challenge for observers is to obtain images of the secondary star. This goal can be achieved through Roche tomography, an indirect imaging technique that can be used to map the Roche-lobe-filling secondary. The review begins with a description of the basic principles that underpin Roche tomography, including methods for determining the system parameters. Finally, we conclude with a look at the main scientific highlights to date, including the first unambiguous detection of starspots on AE Aqr B, and consider the future prospects of this technique.

High power laser production of short-lived isotopes for positron emission tomography

Positron emission tomography (PET) is a powerful diagnostic/imaging technique requiring the production of the short-lived positron emitting isotopes C-11, N-13, O-15 and F-18 by proton irradiation of natural/enriched targets using cyclotrons. The development of PET has been hampered due to the size and shielding requirements of nuclear installations. Recent results show that when an intense laser beam interacts with solid targets, megaelectronvolt (MeV) protons capable of producing PET isotopes are generated. This report describes how to generate intense PET sources of C-11 and F-18 using a petawatt laser beam. The work describing the laser production of F-18 through a (p,n) O-18 reaction, and the subsequent synthesis of 2-[F-18] is reported for the first time. The potential for developing compact laser technology for this purpose is discussed.

Dynamics of charge-displacement channeling in intense laser-plasma interactions

The dynamics of transient electric fields generated by the interaction of high intensity laser pulses with underdense plasmas has been studied experimentally with the proton projection imaging technique. The formation of a charged channel, the propagation of its front edge and the late electric field evolution have been characterized with high temporal and spatial resolution. Particle-in-cell simulations and an electrostatic, ponderomotive model reproduce the experimental features and trace them back to the ponderomotive expulsion of electrons and the subsequent ion acceleration.

Dynamics of Self-Generated, Large Amplitude Magnetic Fields Following High-Intensity Laser Matter Interaction

The dynamics of magnetic fields with an amplitude of several tens of megagauss, generated at both sides of a solid target irradiated with a high-intensity (~1019W/cm2) picosecond laser pulse, has been spatially and temporally resolved using a proton imaging technique. The amplitude of the magnetic fields is sufficiently large to have a constraining effect on the radial expansion of the plasma sheath at the target surfaces. These results, supported by numerical simulations and simple analytical modeling, may have implications for ion acceleration driven by the plasma sheath at the rear side of the target as well as for the laboratory study of self-collimated high-energy plasma jets. © 2012 American Physical Society.

Fundus autofluorescence in the diagnosis of cystoid macular oedema

Aim: To determine the sensitivity and specificity of the non-invasive imaging technique, fundus autofluorescence (AF), in the diagnosis of cystoid macular oedema (CMO), using fluorescein angiography as the reference standard. Design: Retrospective, consecutive, observational case series. Methods: Ninety-six consecutive patients with CMO suspected clinically were selected from the AF database of the Retina Unit, Ophthalmology Department, Grampian University Hospitals-NHS Trust, between August 2004 and June 2006. Only patients in whom CMO was secondary to (1) cataract extraction, (2) inherited retinopathies, (3) inflammatory eye disease or (4) idiopathic cases were included in this study. Only patients in whom AF images had been performed within 2 weeks of FFA and, when obtained following FFA, there was a minimum gap of 4 days ("washing out" period), were considered eligible for this study. A total of 34 eyes from 34 patients were eligible and were included in this study. FFA was used as the reference test to confirm the presence of CMO, and, based on fluorescein angiography (FFA), CMO was graded as either mild or florid. AF images were examined in a masked fashion for the presence or absence of CMO. The sensitivity and specificity of AF in detecting CMO were then calculated. Results: CMO was seen on AF imaging as round or oval areas at the fovea with an AF signal similar to that of background levels. At this site (fovea), the AF signal is usually reduced compared with background, due to the blockage caused by luteal pigment. The diagnosis of CMO based on AF imaging had 81% sensitivity and 69% specificity when compared with the reference standard FFA. Based on the FFA, there were 12 cases of florid CMO and eight of mild CMO. Of the former, CMO was detected with AF imaging in 100% (12/12 eyes), and of the latter, in 50% (4/8 eyes). Conclusions: AF imaging can be used as a rapid, non-invasive technique in the diagnosis of CMO.

The AstraLux large M-dwarf multiplicity survey

We present the results of an extensive high-resolution imaging survey of M-dwarf multiplicity using the Lucky Imaging technique. The survey made use of the AstraLux Norte camera at the Calar Alto 2.2m telescope and the AstraLux Sur camera at the ESO New Technology Telescope in order to cover nearly the full sky. In total, 761 stars were observed (701M-type and 60 late K-type), among which 182 new and 37 previously known companions were detected in 205 systems. Most of the targets have been observed during two or more epochs, and could be confirmed as physical companions through common proper motion, often with orbital motion being confirmed in addition. After accounting for various bias effects, we find a total M-dwarf multiplicity fraction of 27% ± 3% within the AstraLux detection range of 008-6? (semimajor axes of ~3-227 AU at a median distance of 30pc). We examine various statistical multiplicity properties within the sample, such as the trend of multiplicity fraction with stellar mass and the semimajor axis distribution. The results indicate that M-dwarfs are largely consistent with constituting an intermediate step in a continuous distribution from higher-mass stars down to brown dwarfs. Along with other observational results in the literature, this provides further indications that stars and brown dwarfs may share a common formation mechanism, rather than being distinct populations. © 2012. The American Astronomical Society. All rights reserved.

Roche Tomography of the Secondary Stars in CVS

The secondary stars in cataclysmic variables (CVs) are key to our understanding of the origin evolution and behaviour of this class of interacting binary. In seeking a fuller understanding of these objects the challenge for observers is to obtain images of the secondary star. This goal can be achieved through Roche tomography an indirect imaging technique that can be used to map the Roche-lobe-filling secondary star. The review begins with a description of the basic principles that underpin Roche tomography including methods for determining the binary system parameters. Noise propagation onto Roche tomograms is also covered. Finally the review concludes with a look at the main scientific highlights to date and the future prospects for Roche tomography

Fragmentation of CD+ induced by intense ultrashort laser pulses

The fragmentation of CD+ in intense ultrashort laser pulses was investigated using a coincidence three-dimensional momentum imaging technique improved by employing both transverse and longitudinal electric fields. This allowed clear separation of all fragmentation channels and the determination of the kinetic energy release down to nearly zero, for a molecule with significant mass asymmetry. The most probable dissociation pathways for the two lowest dissociation limits, C+ + D and C+ D+, were identified for both 22-fs, 798-nm and 50-fs, 392-nm pulses. Curiously, the charge asymmetric dissociation of CD2+ was not observed for 392-nm photons, even though it was clearly visible for the fundamental 798 nm at the same peak intensity.

Explaining the Coexistence of Large-scale and Small-scale Magnetic Fields in Fully Convective Stars

Despite the lack of a shear-rich tachocline region, low-mass fully convective (FC) stars are capable of generating strong magnetic fields, indicating that a dynamo mechanism fundamentally different from the solar dynamo is at work in these objects. We present a self-consistent three-dimensional model of magnetic field generation in low-mass FC stars. The model utilizes the anelastic magnetohydrodynamic equations to simulate compressible convection in a rotating sphere. A distributed dynamo working in the model spontaneously produces a dipole-dominated surface magnetic field of the observed strength. The interaction of this field with the turbulent convection in outer layers shreds it, producing small-scale fields that carry most of the magnetic flux. The Zeeman–Doppler-Imaging technique applied to synthetic spectropolarimetric data based on our model recovers most of the large-scale field. Our model simultaneously reproduces the morphology and magnitude of the large-scale field as well as the magnitude of the small-scale field observed on low-mass FC stars.

Infrared thermography: A non-invasive window into thermal physiology

Infrared thermography is a non-invasive technique that measures mid to long-wave infrared radiation emanating from all objects and converts this to temperature. As an imaging technique, the value of modern infrared thermography is its ability to produce a digitized image or high speed video rendering a thermal map of the scene in false colour. Since temperature is an important environmental parameter influencing animal physiology and metabolic heat production an energetically expensive process, measuring temperature and energy exchange in animals is critical to understanding physiology, especially under field conditions. As a non-contact approach, infrared thermography provides a non-invasive complement to physiological data gathering. One caveat, however, is that only surface temperatures are measured, which guides much research to those thermal events occurring at the skin and insulating regions of the body. As an imaging technique, infrared thermal imaging is also subject to certain uncertainties that require physical modeling, which is typically done via built-in software approaches. Infrared thermal imaging has enabled different insights into the comparative physiology of phenomena ranging from thermogenesis, peripheral blood flow adjustments, evaporative cooling, and to respiratory physiology. In this review, I provide background and guidelines for the use of thermal imaging, primarily aimed at field physiologists and biologists interested in thermal biology. I also discuss some of the better known approaches and discoveries revealed from using thermal imaging with the objective of encouraging more quantitative assessment.

Modulation du cytochrome P450 dans un modèle murin d'insuffisance rénale chronique

Introduction : Les modèles murins sont grandement utilisés dans l’étude des maladies rénales et des pathologies associées. La concentration de la créatinine sérique est un bon indicateur de la filtration glomérulaire et en présence d’insuffisance rénale chronique (IRC), les concentrations de créatinine sérique (et la clairance) reflètent la sévérité de l’IRC. De plus, il a été démontré que l’IRC modifie le métabolisme des médicaments en diminuant l’activité et l’expression des enzymes hépatiques du cytochrome P450 (CYP450). Afin d’étudier la modulation du P450 par l’IRC avec un modèle murin et de confirmer nos résultats chez le rat, nous devons 1) développer un modèle d’IRC chez la souris, 2) mettre au point une technique de dosage des marqueurs de l’IRC et, 3) évaluer l’expression protéique du CYP450 en présence IRC. Matériel et Méthode : Trois modèles chirurgicaux d’IRC chez la souris ont été développés. Une méthode du dosage de la créatinine par chromatographie liquide à haute performance (CLHP) a été mise au point chez la souris et l’expression protéique du P450 a été mesurée par immunobuvardage de type Western. Résultats : Plusieurs paramètres de CLHP comme le pH, la concentration et le débit de la phase mobile modifient le pic d’élution et le temps de rétention de la créatinine. Concernant le modèle expérimental, on observe une perte de poids et une augmentation de la concentration plasmatique de la créatinine chez les souris avec une IRC. De plus, l’expression protéique de plusieurs isoformes du cytochrome P450 est modulée par l’IRC. Nous observons une diminution du CYP 2D de 42% (p < 0,01), du CYP 3A11 de 60% et du CYP 1A de 37% (p <0,01) par rapport aux souris témoins. On ne dénote aucun changement significatif au niveau de l’isoforme 2E1. Conclusion : Il est possible d’induire une insuffisance rénale chronique chez la souris suite à une néphrectomie. La technique de dosage de la créatinine par CLHP est précise et exacte et permet de caractériser la sévérité de l’IRC chez la souris. L’expression protéique du CYP450 est régulée à la baisse dans le foie des souris atteintes d’IRC.

Analyse fonctionnelle de deux nouvelles mutations récessives de l’AQP2 impliquées dans le diabète insipide néphrogénique par expression dans les ovocytes de Xenopus laevis

Le diabète insipide néphrogénique (DIN) autosomal peut être causé par les mutations du gène codant pour le canal à eau aquaporine-2 (AQP2). Un modèle couramment utilisé pour l’étude des protéines membranaires telle l’AQP2 est l’expression hétérologue dans les ovocytes de Xenopus laevis. Malheureusement, les techniques déjà existantes de purification de membranes plasmiques sont soit trop longues, trop difficiles ou demandent trop de matériel, ne permettent pas l’analyse adéquate du ciblage des formes sauvage comme mutantes, un élément crucial de ce type d’étude. Nous avons donc dans un premier temps mis au point une technique rapide et efficace de purification de membranes plasmiques qui combine la digestion partielle de la membrane vitelline, sa polymérisation à la membrane plasmique suivi de centrifugations à basse vitesse pour récolter les membranes purifiées. Nous avons utilisé cette technique dans l’étude de deux nouveaux cas familiaux de patients hétérozygotes possédant les mutations V24A et R187C dans un cas et K228E et R187C dans le second cas. Pour chaque mutation, nous avons analysé autant les éléments de fonctionnalité que les paramètres d’expression des protéines mutantes. Les expériences de perméabilité membranaire démontrent que les ovocytes exprimant AQP2-V24A (Pf = 16.3 ± 3.5 x 10-4 cm/s, 10 ng) et AQP2- K228E (Pf = 19.9 ± 7.0 x 10-4 cm/s, 10 ng) ont des activités similaires à celle exprimant la forme native (Pf = 14.4 ± 5.5 x 10-4 cm/s, 1 ng), tandis que AQP2- R187C (Pf = 2.6 ± 0.6 x 10-4 cm/s, 10 ng) ne semble avoir aucune activité comme ce qui est observé chez les ovocytes non-injectés (Pf = 2.8 ± 1.0 x 10-4 cm/s). Les études de co-expression ont démontré un effet d’additivité lorsque AQP2-V24A et -K228E sont injectées avec la forme native et un effet s’apparentant à la dominance négative lorsque AQP2-R187C est injecté avec la forme native, avec AQP2-V24A ou avec –K228E. Les résultats obtenus par immunobuvardage représente bien ce qui a été démontré précédemment, on remarque la présence des mutations K228E, V24A et la forme sauvage à la membrane plasmique, contrairement à la mutation R187C. Cependant, lorsque les mutations sont exprimées dans des cellules mIMCD-3, il n’y a qu’une faible expression à la membrane de la forme –K228E et une absence totale des formes –V24A et –R187C à la membrane plasmique, contrairement à la forme native. Les résultats de nos études démontrent que tout dépendant du système d’expression les formes –K228E et –V24A peuvent être utiles dans l’étude des problèmes d’adressage à la membrane à l’aide de chaperonne chimique. De plus, la forme –R187C démontre des difficultés d’adressage qui devront être étudiées afin de mieux comprendre la synthèse des formes natives.