Towards an agri-environment index for biodiversity conservation payment schemes

The aim of the paper is to give suggestions about how an agri-environment index can be designed by taking into account specific ecological and economical factors that reflect benefits and costs of biodiversity conservation. Main findings are that the general structure of an agri-environment index is recommended to be a benefits-to-cost ratio, whereby the conservation benefits are accounted for by the following factors which evaluate i) certain criteria that value the ecological quality of a site and point out its significance for biodiversity conservation (Conservation Significance Factor), ii) a criterion that reflects the connectivity of the site which is an important factor for species migration (Connectivity Factor) and iii) criteria that estimate the potential biodiversity outcomes induced by specific management actions (Conservation Management Factor). The Cost Factor reflects the amount of money that the landholder demands as compensation payment for his conservation services. The paper points out that an agri-environment index is a promising approach to encourage and compensate farmers for biodiversity-friendly management actions. Thereby, an improvement of the effectiveness and efficiency of European conservation payment schemes is a decisive contribution to biodiversity conservation in agricultural landscapes.agri-environmental policy, biodiversity benefits index, biodiversity conservation, ecosystem services, environmental benefits index, rural development

Towards an agri-environment index for biodiversity conservation payment schemes

The aim of the paper is to give suggestions about how an agri-environment index can be designed by taking into account specific ecological and economical factors that reflect benefits and costs of biodiversity conservation. Main findings are that the general structure of an agri- environment index is recommended to be a benefits-to-cost ratio, whereby the conservation benefits are accounted for by the following factors which evaluate i) certain criteria that value the ecological quality of a site and point out its significance for biodiversity conservation (Conservation Significance Factor), ii) a criterion that reflects the connectivity of the site which is an important factor for species migration (Connectivity Factor) and iii) criteria that estimate the potential biodiversity outcomes induced by specific management actions (Conservation Management Factor). The Cost Factor reflects the amount of money that the landholder demands as compensation payment for his conservation services. The paper points out that an agri- environment index is a promising approach to encourage and compensate farmers for biodiversity-friendly management actions. Thereby, an improvement of the effectiveness and efficiency of European conservation payment schemes is a decisive contribution to biodiversity conservation in agricultural landscapes

Privates Engagement für erneuerbare Energien in Unternehmen

Das private Engagement für die Energiewende auch am Arbeitsplatz einzubringen, bleibt vielen engagierten Bürgern verwehrt. Barrieren in Unternehmen stehen dem oftmals entgegen. Freiräume zur Gestaltung können ein Weg sein, um grüne Ideen am Arbeitsplatz umzusetzen

Non-standard neutrino interactions in IceCube

Non-standard neutrino interactions (NSI) may arise in various types of new physics. Their existence would change the potential that atmospheric neutrinos encounter when traversing Earth matter and hence alter their oscillation behavior. This imprint on coherent neutrino forward scattering can be probed using high-statistics neutrino experiments such as IceCube and its low-energy extension, DeepCore. Both provide extensive data samples that include all neutrino flavors, with oscillation baselines between tens of kilometers and the diameter of the Earth. DeepCore event energies reach from a few GeV up to the order of 100 GeV - which marks the lower threshold for higher energy IceCube atmospheric samples, ranging up to 10 TeV. In DeepCore data, the large sample size and energy range allow us to consider not only flavor-violating and flavor-nonuniversal NSI in the μ−τ sector, but also those involving electron flavor. The effective parameterization used in our analyses is independent of the underlying model and the new physics mass scale. In this way, competitive limits on several NSI parameters have been set in the past. The 8 years of data available now result in significantly improved sensitivities. This improvement stems not only from the increase in statistics but also from substantial improvement in the treatment of systematic uncertainties, background rejection and event reconstruction

IceCube Search for Earth-traversing ultra-high energy Neutrinos

The search for ultra-high energy neutrinos is more than half a century old. While the hunt for these neutrinos has led to major leaps in neutrino physics, including the detection of astrophysical neutrinos, neutrinos at the EeV energy scale remain undetected. Proposed strategies for the future have mostly been focused on direct detection of the first neutrino interaction, or the decay shower of the resulting charged particle. Here we present an analysis that uses, for the first time, an indirect detection strategy for EeV neutrinos. We focus on tau neutrinos that have traversed Earth, and show that they reach the IceCube detector, unabsorbed, at energies greater than 100 TeV for most trajectories. This opens up the search for ultra-high energy neutrinos to the entire sky. We use ten years of IceCube data to perform an analysis that looks for secondary neutrinos in the northern sky, and highlight the promise such a strategy can have in the next generation of experiments when combined with direct detection techniques

Posteriori analysis on IceCube double pulse tau neutrino candidates

The IceCube Neutrino Observatory at the South Pole detects Cherenkov light emitted by charged secondary particles created by primary neutrino interactions. Double pulse waveforms can arise from charged current interactions of astrophysical tau neutrinos with nucleons in the ice and the subsequent decay of tau leptons. The previous 8-year tau double pulse analysis found three tau neutrino candidate events. Among them, the most promising one observed in 2014 is located very near the dust layer in the middle of the detector. A posterior analysis on this event will be presented in this paper, using a new ice model treatment with continuously varying nuisance parameters to do the targeted Monte Carlo re-simulation for tau and other background neutrino ensembles. The impact of different ice models on the expected signal and background statistics will also be discussed