‘Discourses of climate delay’ pervade current debates on climate action. These discourses accept the existence of climate change, but justify inaction or inadequate efforts. In contemporary discussions on what actions should be taken, by whom and how fast, proponents of climate delay would argue for minimal action or action taken by others. They focus attention on the negative social effects of climate policies and raise doubt that mitigation is possible. Here, we outline the common features of climate delay discourses and provide a guide to identifying them.

We construct a renewal structure for random walks on surface groups. The renewal times are defined as times when the random walks enter a particular type of cone and never leave it again. As a consequence, the trajectory of the random walk can be expressed as an aligned union of independent and identically distributed trajectories between the renewal times. Once having established this renewal structure, we prove a central limit theorem for the distance to the origin under exponential moment conditions. Analyticity of the speed and of the asymptotic variance are natural consequences of our approach. Furthermore, our method applies to groups with infinitely many ends and therefore generalizes classic results on central limit theorems on free groups.

To understand the dynamics of ice shelves, a knowledge of their internal and basal structure is very important. As the capacity to perform local surveys is limited, remote sensing provides an opportunity to obtain the relevant information. We must prove, however, that the relevant information can be obtained from remote sensing of the surface. That is the aim of this study. The Jelbart Ice Shelf, Antarctica, exhibits a variety of surface structures appearing as stripe-like features in radar imagery. We performed an airborne geophysical survey across these features and compared the results to TerraSAR-X imagery. We find that the stripe-like structures indicate surface troughs coinciding with the location of basal channels and crevasse-like features, revealed by radio-echo sounding. HH and VV polarizations do not show different magnitude. In surface troughs, the local accumulation rate is larger than at the flat surface. Viscoelastic modelling is used to gain an understanding of the surface undulations and their origin. The surface displacement, computed with a Maxwell model, matches the observed surface reasonably well. Our simulations show that the surface troughs develop over decadal to centennial timescales.

Indium has attracted much attention as a beneficial addition to cobalt–antimony-based skutterudites as a result of good thermoelectric performance. In this study, as-cast InxCo4Sb12 with x = 0.05, 0.2 were examined using x-ray diffraction analysis and scanning electron microscopy. For x = 0.2 we found, besides the skutterudite main phase, nanometer-sized regions of secondary phases distributed along the grain boundaries, which exhibit substructures. As-cast material with x = 0.05 does not show visible precipitates. We further observed that changing one of the heat treatment parameters of In0.2Co4Sb12 has a major effect on the microstructure and shape of the precipitates, but minor influence on the skutterudite matrix composition. Energy dispersive x-ray spectroscopy analysis by transmission electron microscopy) reveals that indium is to a large extent distributed into the skutterudite structure. Measurements of short-term sintered material confirm that the addition of indium and particularly the modification of the synthesis parameter entails to an enhanced ZT.

Spider walks are systems of interacting particles. The particles move independently as long as their movements do not violate some given rules describing the relative position of the particles; moves that violate the rules are not realized. The goal of this paper is to study qualitative properties, as recurrence, transience, ergodicity, and positive rate of escape of these Markov processes.

ϵ Eridani hosts one known inner planet and an outer Kuiper belt analog. Further, Spitzer/IRS measurements indicate that warm dust is present at distances as close as a few AU from the star. Its origin is puzzling, since an “asteroid belt” that could produce this dust would be unstable because of the inner planet. We tested a hypothesis that the observed warm dust is generated by collisions in the outer belt and is transported inward by P-R drag and strong stellar winds. With numerical simulation we investigated how the dust streams from the outer ring into the inner system, and calculated the thermal emission of the dust. We show that the observed warm dust can indeed stem from the outer belt. Our models reproduce the shape and magnitude of the observed SED from mid-IR to sub-mm wavelengths, as well as the Spitzer/MIPS radial brightness profiles.

In the mammalian retina, neuronal nitric oxide synthase (NOS) is mainly localized in subpopulations of amacrine cells. One function of nitric oxide (NO) is to stimulate soluble guanylate cyclases which in turn synthesize cGMP. We used an antibody specific for cGMP to demonstrate cGMP-like immunoreactivity (cG-IR) in bovine, rat, and rabbit retinae and investigated the effects on cGMP levels of both exogenously applied NO and of endogenously released NO. We found that cGMP levels in inner and outer retina were controlled in opposite ways. In the presence of the NO-donors SNP, SIN-1 or SNAP, cG-IR was prominent in neurons of the inner retina, mainly in cone bipolar cells, some amacrine and ganglion cells. Retinae incubated in IBMX showed weak cG-IR in bipolar cells. Glutamate increased cG-IR in the inner retina, presumably by stimulating endogenous NO release, whereas NOS inhibitors or GABA and glycine decreased cG-IR in bipolar cells by reducing NO release. In somata, inner segments and spherules of rod photoreceptors the situation was reversed. cG-IR was undetectable in the presence of NO-donors or glutamate, was moderate in IBMX-treated retinae, but increased strongly in the presence of NOS inhibitors or GABA/glycine. We conclude that NO is released endogenously in the retina. In the presence of NO, cGMP levels are increased in neurons of the inner retina, but are decreased in rods.