259 research outputs found
RĆ“le et variations de l'expression de la superfamille des proteĢines IGFBP par les cellules bĆŖta des Ć®lots pancreĢatiques, notamment en cas d'atteinte pancreĢatique comme celle induite par le diabeĢte
L'insuline est une hormone seĢcreĢteĢe par les cellules bĆŖta des Ć®lots pancreĢatiques, qui joue un rĆ“le majeur dans le meĢtabolisme du glucose, notamment en reĢgulant l'augmentation de la glyceĢmie suite aĢ la prise alimentaire. Sa seĢcreĢtion est principalement stimuleĢe par l'augmentation du glucose dans le sang, qui joue un roĢle direct sur les cellules bĆŖta du pancreĢas.
En paralleĢle, les gluco-increĢtines, GLP-1 et GIP, seĢcreĢteĢes par l'intestin en reĢponse aĢ la prise alimentaire, jouent eĢgalement un roĢle important dans la seĢcreĢtion de l'insuline. Elles agissent en potentialisant l'effet du glucose sur la seĢcreĢtion de l'insuline par les cellules beĢta pancreĢatiques, tout en favorisant leur prolifeĢration et leur protection contre l'apoptose. Il a d'ailleurs eĢteĢ estimeĢ qu'environ 50% de la seĢcreĢtion d'insuline en reĢponse aĢ un repas eĢtait lieĢ aĢ l'effet des increĢtines (M. Virally et al., 2008).
Il a alors eĢteĢ montreĢ que le roĢle de GLP-1 sur la prolifeĢration et la protection contre l'apoptose des cellules beĢta du pancreĢas eĢtait en grande partie assureĢ par une boucle autocrine meĢdieĢe par IGF2. En effet, GLP-1 stimule l'expression de reĢcepteurs aĢ IGF aĢ la surface des cellules bĆŖta et l'activation de ces reĢcepteurs est assureĢe par une seĢcreĢtion autocrine d'IGF-2, seĢcreĢteĢ en concomitance avec l'insuline dans les granules de seĢcreĢtion (M. Cornu et al., 2009).
Les IGF, plus preĢciseĢment IGF-1 et IGF-2, sont des hormones principalement seĢcreĢteĢes par le foie qui influencent le meĢtabolisme cellulaire via leur reĢcepteur speĢcifique IGF1-R. Elles sont connues pour agir comme stimulateur de la croissance, de la prolifeĢration et de la diffeĢrenciation des cellules normales ainsi que des cellules malignes. La majeure partie des IGF circulantes dans le plasma se trouve lieĢ aĢ des proteĢines de liaison, au
Ā 2
nombre de 6, IGFBP (Insulin-like Growth Factor Binding Protein) 1 aĢ 6, qui augmentent leur stabiliteĢ et ainsi leur demi-vie mais diminuent eĢgalement leur biodisponibiliteĢ. C'est ainsi que ces proteĢines IGFBP assurent une reĢgulation de l'activiteĢ des IGF en reĢgulant leur disponibiliteĢ pour leurs reĢcepteurs speĢcifiques.
Pour finir, il a eĢteĢ montreĢ que les proteĢines IGFBP pouvaient avoir une action intrinseĢque, indeĢpendante de l'IGF. MeĢme si leur roĢle est encore mal deĢfini, certaines donneĢes ont montreĢ l'existence d'une action intrinseĢque, en particulier pour IGFBP3 et IGFBP5 (Vivian HWA et al., 1999).
Le but de mon travail consiste alors aĢ eĢtudier si les cellules beĢta pancreĢatiques expriment elles-meĢmes des proteĢines IGFBP, et si c'est le cas, d'essayer d'identifier les meĢcanismes qui reĢgulent leur expression en imaginant que leur seĢcreĢtion pourrait soit jouer un roĢle sur la voie de signalisation des gluco-increĢtines et la boucle autocrine qu'elles induisent en agissant sur la biodisponibiliteĢ d'IGF-2, soit agir de manieĢre intrinseĢque indeĢpendamment de l'IGF-2.
Pour cela, apreĢs avoir montreĢ que les cellules beĢta pancreĢatiques expriment des proteĢines IGFBP, nous eĢtudierons l'effet des gluco-increĢtines sur leur expression, puis les variations susceptibles d'eĢtre induites par les meĢcanismes responsables de la diminution de la masse cellulaire beĢta observeĢe dans les iĢlots pancreĢatiques des patients diabeĢtiques
Methanol exchange between grassland and the atmosphere
International audienceConcentrations and fluxes of methanol were measured above two differently managed grassland fields (intensive and extensive) in central Switzerland during summer 2004. The measurements were performed with a proton-transfer-reaction mass-spectrometer and fluxes were determined by the eddy covariance method. The observed methanol emission showed a distinct diurnal cycle and was strongly correlated with global radiation and water vapour flux. Mean and maximum daily emissions were found to depend on grassland species composition and, for the intensive field, also on the growing state. The extensive field with a more complex species composition had higher emissions than the graminoid-dominated intensive field, both on an area and on a biomass basis. A simple parameterisation depending on the water vapour flux and the leaf area index allowed a satisfying simulation of the temporal variation of methanol emissions over the growing phase. Accumulated carbon losses due to methanol emissions accounted for 0.024 and 0.048% of net primary productivity for the intensive and extensive field, respectively. The integral methanol emissions over the growing periods were more than one order of magnitude higher than the emissions related to cut and drying events
The annual ammonia budget of fertilised cut grassland ā Part 1: Micrometeorological flux measurements and emissions after slurry application
Two commercial ammonia (NH<sub>3</sub>) analysers were customised to allow continuous measurements of vertical concentration gradients. The gradients were used to derive ammonia exchange fluxes above a managed grassland site at Oensingen (Switzerland) by application of the aerodynamic gradient method. The measurements from July 2006 to October 2007 covered five complete growth-cut cycles and included six applications of liquid cattle slurry. The average accuracy of the flux measurements during unstable and near-neutral conditions was 20% and the detection limit was 10 ng NH<sub>3</sub> m<sup>&minus;2</sup> s<sup>&minus;1</sup>. Hence the flux measurements are considered sufficiently accurate for studying typical NH<sub>3</sub> deposition rates over growing vegetation. Quantifying the overall emissions after slurry applications required the application of elaborate interpolations because of difficulties capturing the initial emissions during broadspreading of liquid manure. The emissions were also calculated with a mass balance method yielding similar fluxes. NH<sub>3</sub> losses after slurry application expressed as percentage of emitted nitrogen versus applied total ammoniacal nitrogen (TAN) varied between 4 and 19%, which is roughly a factor of three lower than the values for broadspreading of liquid manure in emission inventories. The comparatively low emission factors appear to be a consequence of the low dry matter content of the applied slurry and soil properties favouring ammonium adsorption
The annual ammonia budget of fertilised cut grassland ā Part 2: Seasonal variations and compensation point modeling
The net annual NH<sub>3</sub> exchange budget of a fertilised, cut grassland in Central Switzerland is presented. The observation-based budget was computed from semi-continuous micrometeorological fluxes over a time period of 16 months and using a process-based gap-filling procedure. The data for emission peak events following the application of cattle slurry and for background exchange were analysed separately to distinguish short-term perturbations from longer-term ecosystem functioning. A canopy compensation point model of background exchange is parameterised on the basis of measured data and applied for the purposes of gap-filling. The data show that, outside fertilisation events, grassland behaves as a net sink for atmospheric NH<sub>3</sub> with an annual dry deposition flux of &minus;3.0 kg N ha<sup>&minus;1</sup> yr<sup>&minus;1</sup>, although small NH<sub>3</sub> emissions by the canopy were measured in dry daytime conditions. The median &Gamma;<sub><i>s</i></sub> ratio in the apoplast (=[NH<sub>4</sub><sup>+</sup>]/[H<sup>+</sup>]) estimated from micrometeorological measurements was 620, equivalent to a stomatal compensation point of 1.3 &mu;g NH<sub>3</sub> m<sup>&minus;3</sup> at 15 &deg;C. Non-stomatal resistance to deposition <i>R<sub>w</sub></i> was shown to increase with temperature and decrease with surface relative humidity, and <i>R<sub>w</sub></i> values were among the highest published for European grasslands, consistent with a relatively high ratio of NH<sub>3</sub> to acid gases in the boundary layer at this site. Since the gross annual NH<sub>3</sub> emission by slurry spreading was of the order of +20 kg N ha<sup>&minus;1</sup> yr<sup>&minus;1</sup>, the fertilised grassland was a net NH<sub>3</sub> source of +17 kg N ha<sup>&minus;1</sup> yr<sup>&minus;1</sup>. A comparison with the few other measurement-based budget values from the literature reveals considerable variability, demonstrating both the influence of soil, climate, management and grassland type on the NH<sub>3</sub> budget and the difficulty of scaling up to the national level
Technical note: Water vapour concentration and flux measurements with PTR-MS
International audienceThe most direct approach for measuring the exchange of biogenic volatile organic compounds between terrestrial ecosystems and the atmosphere is the eddy covariance technique. It has been applied several times in the last few years using fast response proton-transfer-reaction mass spectrometry (PTR-MS). We present an independent validation of this technique by applying it to measure the water vapour flux in comparison to a common reference system comprising an infra-red gas analyser (IRGA). Water vapour was detected in the PTR-MS at mass 37 (atomic mass units) corresponding to the cluster ion H3O+Ā·H2O. During a five-week field campaign at a grassland site, we obtained a non-linear but stable calibration function between the mass 37 signal and the reference water vapour concentration. With a correction of the high-frequency damping loss based on empirical ogive analysis, the eddy covariance water vapour flux obtained with the PTR-MS showed a very good agreement with the flux of the reference system. The application of the empirical ogive method for high-frequency correction led to significantly better results than using a correction based on theoretical spectral transfer functions. This finding is attributed to adsorption effects on the tube walls that are presently not included in the theoretical correction approach. The proposed high-frequency correction method can also be used for other trace gases with different adsorption characteristics
Atmosphere-snow transfer function for H2O2: microphysical considerations
H2O2 analyses of polar ice cores show an increase in concentration from 200 years to the present. In order to quantitatively relate the observed trend in the ice to atmospheric levels, the atmosphere-snow transfer behavior and postdepositional changes must be known. Atmosphere-snow transfer was studied by investigating uptake and release of H2O2 in a series of laboratory column experiments in the temperature range ā3Ā°C to ā45Ā°C. Experiments consisted of passing H2O2-containing air through a column packed with 200-Ī¼m diameter ice spheres and measuring the change in gas phase H2O2 concentration with time. The uptake of H2O2 was a slow process requiring several hours to reach equilibrium. Uptake involved incorporation of H2O2 into the bulk ice as well as surface accumulation. The amount of H2O2 taken up by the ice was greater at the lower temperatures. The sticking coefficient for H2O2 on ice in the same experiments was estimated to be of the order of 0.02 to 0.5. Release of H2O2 from the ice occurred upon passing H2O2-free air through the packed columns, with the time scale for degassing similar to that for uptake. These results suggest that systematic losses of H2O2 from polar snow could occur under similar conditions, when atmospheric concentrations of H2O2 are low, that is, in the winter
Flux measurements of biogenic VOCs during ECHO 2003
International audienceWithin the framework of the AFO 2000 project ECHO, two PTR-MS instruments were operated in combination with sonic anemometers to determine biogenic VOC fluxes from a mixed deciduous forest site in North-Western Germany using the eddy covariance (EC) technique. The measurement site was characterised by a forest of inhomogeneous composition, complex canopy structure, limited extension in certain wind directions and frequent calm wind conditions during night time. As a consequence, a considerable fraction of the measurements did not qualify for flux calculations by EC and had to be discarded. The validated results show light and temperature dependent emissions of isoprene and monoterpenes from this forest, with average emissions (normalised to 30Ā°C and 1000 Āµmoles m?2 s?1 PAR) of 1.5 and 0.39 Āµg m?2 s?1, respectively. Emissions of methanol reached on average 0.087 Āµg m?2 s?1 during daytime, but fluxes were too small to be detected during night time. Upward fluxes of the isoprene oxidation products methyl vinyl ketone (MVK) and methacrolein (MACR) were also found, being two orders of magnitude lower than those of isoprene. The observed fluxes are consistent with upscalings from leaf-level emission measurements of representative tree species in this forest and, in the case of MVK and MACR, can plausibly be explained by chemical production through oxidation of isoprene within the canopy. Calculations with an analytical footprint model indicate that the observed isoprene fluxes correlate with the fraction of oaks within the footprints of the flux measurement
Diel variations of H2O2 in Greenland: A discussion of the cause and effect relationship
Atmospheric hydrogen peroxide (H2O2) measurements at Summit, Greenland, in MayāJune, 1993 exhibited a diel variation, with afternoon highs typically 1ā2 parts per billion by volume (ppbv) and nighttime lows about 0.5 ppbv lower. This variation closely followed that for temperature; specific humidity exhibited the same general trend. During a 17-day snowfall-free period, surface snow was accumulating H2O2, apparently from nighttime cocondensation of H2O and H2O2. Previous photochemical modeling (Neftel et al., 1995) suggests that daytime H2O2 should be about 1 ppbv, significantly lower than our measured values. Previous equilibrium partitioning measurements between ice and gas phase (Conklin et al., 1993) suggest that air in equilibrium with H2O2 concentrations measured in surface snow (15ā18 Ī¼M) should have an H2O2 concentration 2ā3 times what we measured 0.2ā3.5 m above the snow surface. A simple eddy diffusion model, with vertical eddy diffusion coefficients calculated from balloon soundings, suggested that atmospheric H2O2 concentrations should be affected by any H2O2 degassed from surface snow. However, field measurements showed the absence of either high concentrations of H2O2 or a measurable concentration gradient between inlets 0.2 and 3 m above the snow. A surface resistance to degassing, that is, slow release of H2O2 from the ice matrix, is a plausible explanation for the differences between observations and modeled atmospheric profiles. Degassing of H2O2 at a rate below our detection limit would still influence measured atmospheric concentrations and help explain the difference between measurements and photochemical modeling. The cumulative evidence suggests that surface snow adjusts slowly to drops in atmospheric H2O2 concentration, over timescales of at least weeks. The H2O2 losses previously observed in pits sampled over more than 1 year are thought to have occurred later in the summer or fall, after the MayāJuly field season
Abyssal Atlantic circulation during the Last Glacial Maximum: Constraining the ratio between transport and vertical mixing
The oceanās role in regulating atmospheric carbon dioxide on glacialāinterglacial timescales remains an
unresolved issue in paleoclimatology. Reduced mixing between deep water masses may have aided oceanic
storage of atmospheric CO_2 during the Last Glacial Maximum (LGM), but data supporting this idea have
remained elusive. The Ī“^(13)C of benthic foraminifera indicate the Atlantic Ocean was more chemically
stratified during the LGM, but the nonconservative nature of Ī“^(13)C complicates interpretation of the LGM
signal. Here we use benthic foraminiferal Ī“^(18)O as a conservative tracer to constrain the ratio of meridional
transport to vertical diffusivity in the deep Atlantic. Our calculations suggest that the ratio was at least twice
as large at the LGM. We speculate that the primary cause was reduced mixing between northern and
southern component waters, associated with movement of this water mass boundary away from the zone of
intense mixing near the seafloor. The shallower water mass boundary yields an order of magnitude increase
in the volume of southern component water, suggesting its residence time may have increased substantially.
Our analysis supports the idea that an expanded volume of Antarctic Bottom Water and limited vertical
mixing enhanced the abyssal oceanās ability to trap carbon during glacial times
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