Participatory Integrated Climate Services for Agriculture (PICSA) Intermediary Training in Muhanga, Rwanda

The Rwanda Climate Services for Agriculture project is a four-year initiative (2016-2019) that seeks to transform Rwanda’s rural farming communities and national economy through improved climate risk management. This report presents the outputs of a five-day training workshop in Muhanga, Rwanda on the use of the Participatory Integrated Climate Services for Agriculture (PICSA) approach to help farmers make climate informed decisions. This training brought together farmer promoters, Social Economic Development Officers (SEDOs), as well as Sector Agronomists from the four pilot districts in Rwanda. The training workshop aimed to initiate the process of PICSA implementation starting by training lead farmers who will train farmers in the use of the PICSA approach. The report includes the process of the training workshop, presentations, and the evaluation by participants

Participatory Integrated Climate Services for Agriculture (PICSA) Specialist Intermediary Training in Nyamata, Rwanda

The Rwanda Climate Services for Agriculture project is a four-year initiative (2016-2019) that seeks to transform Rwanda’s rural farming communities and national economy through improved climate risk management. This report presents the outputs of a five-day training on the use of a Participatory Integrated Climate Services for Agriculture (PICSA) approach to help farmers make climate informed decisions. This training brought together key government agencies in Rwanda, research organizations, farmers’ representatives, development partners, non-governmental organizations, and media. The one week training workshop aimed to initiate the process to develop skills of staff to become a group of expert trainers in the PICSA approach. The report includes the proceeding of the training workshop as well as reflections on workshop outcomes and feedback by participants

966-45 QT Dispersion in Essential Hypertension

Increased QT dispersion (QTd) reflects regional variation in ventricular repolarisation, and has been shown in heart failure and hypertrophic cardiomyopathy to relate to an increased incidence of sudden death. As essential hypertensives (EH) are also at increased risk of sudden death we aimed to determine whether increased QTd is found in those EH who are known to be at the highest risk of sudden death. In 50 EH we measured QTd (maximum corrected QT interval minus minimum corrected QT interval), echocardiographic left ventricular mass index (LVMI) (n=46 as 4 patients non-echogenic), office systolic and diastolic blood pressure (SSP, DSP), and 24 hour ambulatory systolic and diastolic blood pressure (24 SSP, 24 DSP) (n=40). Univariate analysis demonstrated no relationship between QTd and age, sex, height, weight, 24 SSP or 24 DBP. Significant relationships existed between QTd and LVMI (R2=0.25, P<0.001), SSP (R2=0.16, P<0.01), DSP (R2=0.08, P<0.05). Multiple linear regression analysis revealed the only relationships to QTd were LVMI (p<0.01) and SSP (p<0.05). Excluding 4 patients with electro-cardiographic left ventricular hypertrophy (ECG-LVH) from the analysis a significant relationship between QTd and LVMI (R2=0.13, P<0.05) and SSP (R2=0.10, P<0.05) persists. These demonstrate that increased QTd is found in EH with the highest risk of sudden death (greatest SSP and LVMI). This relationship persists in the absence of ECG-LVH. Further study of QTd, as a predictor of sudden death in EH is warranted

Cone-Beam Computed Tomography as an Adjunct to Performance of Percutaneous Cementoplasty of the Acetabulum

AbstractAcetabuloplasty is a valuable palliative adjunct for the treatment of patients with painful metastatic disease to the pelvis in selected cases. We report the case of a 45-year-old woman with morbid obesity and with breast carcinoma who was technically difficult to treat under fluoroscopic guidance due to very poor visualization secondary to her body habitus. It was possible to perform radiofrequency ablation and acetabuloplasty with the use of cone-beam computed tomography for guidance

How close can an Inhomogeneous Universe mimic the Concordance Model?

Recently, spatially inhomogeneous cosmological models have been proposed as an alternative to the LCDM model, with the aim of reproducing the late time dynamics of the Universe without introducing a cosmological constant or dark energy. This paper investigates the possibility of distinguishing such models from the standard LCDM using background or large scale structure data. It also illustrates and emphasizes the necessity of testing the Copernican principle in order to confront the tests of general relativity with the large scale structure.Comment: 15 pages, 7 figure

Cosmic magnetic fields from velocity perturbations in the early Universe

We show, using a covariant and gauge-invariant charged multifluid perturbation scheme, that velocity perturbations of the matter-dominated dust Friedmann-Lemaitre-Robertson-Walker (FLRW) model can lead to the generation of cosmic magnetic fields. Moreover, using cosmic microwave background (CMB) constraints, it is argued that these fields can reach strengths of between 10^{-28} and 10^{-29} G at the time the dynamo mechanism sets in, making them plausible seed field candidates.Comment: 11 pages, 1 figure, IOP style, minor changes and typos correcte

B\"acklund transformations for the second Painlev\'e hierarchy: a modified truncation approach

The second Painlev\'e hierarchy is defined as the hierarchy of ordinary differential equations obtained by similarity reduction from the modified Korteweg-de Vries hierarchy. Its first member is the well-known second Painlev\'e equation, P2. In this paper we use this hierarchy in order to illustrate our application of the truncation procedure in Painlev\'e analysis to ordinary differential equations. We extend these techniques in order to derive auto-B\"acklund transformations for the second Painlev\'e hierarchy. We also derive a number of other B\"acklund transformations, including a B\"acklund transformation onto a hierarchy of P34 equations, and a little known B\"acklund transformation for P2 itself. We then use our results on B\"acklund transformations to obtain, for each member of the P2 hierarchy, a sequence of special integrals.Comment: 12 pages in LaTeX 2.09 (uses ioplppt.sty), to appear in Inverse Problem

The thermal emission of the exoplanets WASP-1b and WASP-2b

We present a comparative study of the thermal emission of the transiting exoplanets WASP-1b and WASP-2b using the Spitzer Space Telescope. The two planets have very similar masses but suffer different levels of irradiation and are predicted to fall either side of a sharp transition between planets with and without hot stratospheres. WASP-1b is one of the most highly irradiated planets studied to date. We measure planet/star contrast ratios in all four of the IRAC bands for both planets (3.6-8.0um), and our results indicate the presence of a strong temperature inversion in the atmosphere of WASP-1b, particularly apparent at 8um, and no inversion in WASP-2b. In both cases the measured eclipse depths favor models in which incident energy is not redistributed efficiently from the day side to the night side of the planet. We fit the Spitzer light curves simultaneously with the best available radial velocity curves and transit photometry in order to provide updated measurements of system parameters. We do not find significant eccentricity in the orbit of either planet, suggesting that the inflated radius of WASP-1b is unlikely to be the result of tidal heating. Finally, by plotting ratios of secondary eclipse depths at 8um and 4.5um against irradiation for all available planets, we find evidence for a sharp transition in the emission spectra of hot Jupiters at an irradiation level of 2 x 10^9 erg/s/cm^2. We suggest this transition may be due to the presence of TiO in the upper atmospheres of the most strongly irradiated hot Jupiters.Comment: 10 pages, submitted to Ap

Density growth in Kantowski-Sachs cosmologies with cosmological constant

In this work the growth of density perturbations in Kantowski-Sachs cosmologies with a positive cosmological constant is studied, using the 1+3 and 1+1+2 covariant formalisms. For each wave number we obtain a closed system for scalars formed from quantities that are zero on the background and hence are gauge-invariant. The solutions to this system are then analyzed both analytically and numerically. In particular the effects of anisotropy and the behaviour close to a bounce in the cosmic scale factor are considered. We find that typically the density gradient in the bouncing directions experiences a local maximum at or slightly after the bounce.Comment: 33 pages, 17 picture

Drivers of plant traits that allow survival in wetlands

Plants have developed a suite of traits to survive the anaerobic and anoxic soil conditions in wetlands. Previous studies on wetland plant adaptive traits have focused mainly on physiological aspects under experimental conditions, or compared the trait expression of the local species pool. Thus, a comprehensive analysis of potential factors driving wetland plant adaptive traits under natural environmental conditions is still missing.In this study, we analysed three important wetland adaptive traits, i.e. root porosity, root/shoot ratio and underwater photosynthetic rate, to explore driving factors using a newly compiled dataset of wetland plants. Based on 21 studies at 38 sites across different biomes, we found that root porosity was affected by an interaction of temperature and hydrological regime; root:shoot ratio was affected by temperature, precipitation and habitat type; and underwater photosynthetic rate was affected by precipitation and life form. This suggests that a variety of driving mechanisms affect the expression of different adaptive traits.The quantitative relationships we observed between the adaptive traits and their driving factors will be a useful reference for future global methane and denitrification modelling studies. Our results also stress that besides the traditionally emphasized hydrological driving factors, other factors at several spatial scales should also be taken into consideration in the context of future functional wetland ecology.Environmental Biolog