971 resultados para Rocky Mountain locust.
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Background Chronic mountain sickness (CMS) is often associated with vascular dysfunction, but the underlying mechanism is unknown. Sleep disordered breathing (SDB) frequently occurs at high altitude. At low altitude SDB causes vascular dysfunction. Moreover, in SDB, transient elevations of right-sided cardiac pressure may cause right-to-left shunting in the presence of a patent foramen ovale (PFO) and, in turn, further aggravate hypoxemia and pulmonary hypertension. We speculated that compared to healthy high-altitude dwellers, in patients with CMS, SDB and nocturnal hypoxemia are more pronounced and related to vascular dysfunction. Methods We performed overnight sleep recordings, and measured systemic and pulmonary-artery pressure in 23 patients with CMS (mean±SD age 52.8±9.8 y) and 12 healthy controls (47.8±7.8 y) at 3600 m. In a subgroup of 15 subjects with SDB, we searched for PFO with transesophagal echocardiography. Results The major new findings were that in CMS patients, a) SDB and nocturnal hypoxemia was more severe (P<0.01) than in controls (apnea/hypopnea index, AHI, 38.9±25.5 vs. 14.3±7.8[nb/h]; SaO2, 80.2±3.6 vs. 86.8±1.7[%], CMS vs. controls), and b) AHI was directly correlated with systemic blood pressure (r=0.5216, P=0.001) and pulmonary-artery pressure (r=0.4497, P=0.024). PFO was associated with more severe SDB (AHI 48.8±24.7 vs. 14.8±7.3[nb/h], P=0.013, PFO vs. no PFO) and hypoxemia. Conclusion SDB and nocturnal hypoxemia are more severe in CMS patients than in controls and are associated with systemic and pulmonary vascular dysfunction. The presence of a PFO appeared to further aggravate SDB. Closure of PFO may improve SDB, hypoxemia and vascular dysfunction in CMS patients. Clinical Trials Gov Registration NCT01182792.
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A deeper understanding of past vegetation dynamics is required to better assess future vegetation responses to global warming in the Alps. Lake sediments from Lac de Bretaye, a small subalpine lake in the Northern Swiss Alps (1780 m a.s.l.), were analysed to reconstruct past vegetation dynamics for the entire Holocene, using pollen, macrofossil and charcoal analyses as main proxies. The results show that timberline reached the lake’s catchment area at around 10,300 cal. BP, supporting the hypothesis of a delayed postglacial afforestation in the Northern Alps. At the same time, thermophilous trees such as Ulmus, Tilia and Acer established in the lowlands and expanded to the altitude of the lake, forming distinctive boreo-nemoral forests with Betula, Pinus cembra and Larix decidua. From about 5000 to 3500 cal. BP, thermophilous trees declined because of increasing human land use, mainly driven by the mass expansion of Picea abies and severe anthropogenic fire activity. From the Bronze Age onwards (c. 4200–2800 cal. BP), grazing indicators and high values for charcoal concentration and influx attest an intensifying human impact, fostering the expansion of Alnus viridis and Picea abies. Hence, biodiversity in alpine meadows increased, whereas forest diversity declined, as can be seen in other regional records. We argue that the anticipated climate change and decreasing human impact in the Alps today will not only lead to an upward movement of timberline with consequent loss of area for grasslands, but also to a disruption of Picea abies forests, which may allow the re-expansion of thermophilous tree species.
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Aims. We present an inversion method based on Bayesian analysis to constrain the interior structure of terrestrial exoplanets, in the form of chemical composition of the mantle and core size. Specifically, we identify what parts of the interior structure of terrestrial exoplanets can be determined from observations of mass, radius, and stellar elemental abundances. Methods. We perform a full probabilistic inverse analysis to formally account for observational and model uncertainties and obtain confidence regions of interior structure models. This enables us to characterize how model variability depends on data and associated uncertainties. Results. We test our method on terrestrial solar system planets and find that our model predictions are consistent with independent estimates. Furthermore, we apply our method to synthetic exoplanets up to 10 Earth masses and up to 1.7 Earth radii, and to exoplanet Kepler-36b. Importantly, the inversion strategy proposed here provides a framework for understanding the level of precision required to characterize the interior of exoplanets. Conclusions. Our main conclusions are (1) observations of mass and radius are sufficient to constrain core size; (2) stellar elemental abundances (Fe, Si, Mg) are principal constraints to reduce degeneracy in interior structure models and to constrain mantle composition; (3) the inherent degeneracy in determining interior structure from mass and radius observations does not only depend on measurement accuracies, but also on the actual size and density of the exoplanet. We argue that precise observations of stellar elemental abundances are central in order to place constraints on planetary bulk composition and to reduce model degeneracy. We provide a general methodology of analyzing interior structures of exoplanets that may help to understand how interior models are distributed among star systems. The methodology we propose is sufficiently general to allow its future extension to more complex internal structures including hydrogen- and water-rich exoplanets.
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Louise von Panhuys
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by Charles New, of the late Livingstone search and relief expedition
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Signatur des Originals: S 36/G00107