Regional Seas integrative studies,as a basis for an ecosystem-based approach to management: The case of the Bay of Biscay

Marine legislation world-wide has, as a recent final objective, the maintenance of a good environmental or ecological status for marine waters, habitats and resources. The concept of environmental status takes into account the structure, function and processes of marine ecosystems, bringing together physical, chemical, physiographic, geographic and climatic factors: subsequently, integrating such conditions, with anthropogenic impacts and activities undertaken in the area concerned. Such an approach is intended to permit an assessment of the environmental status at the ecosystem level, i.e. ‘ecosystem-based approach’, or ‘ecosystem-based management’.Such legislation emphasises the need for the development of methodologies, to assess environmental status. As such the knowledge acquired within Regional Seas, discussed at International Symposia and, finally, published as Special Issues, can serve as the basis for a regional ecosystem-based approach to management and the integrative assessment of marine systems. Hence, the Bay of Biscay is used in this contribution, as an example, to show past and present research, together with perspectives for the future. It is concluded that collaboration between institutions (marine research institutes, universities) and countries (France, Spain, Portugal, the United Kingdom and Ireland) could result in an interesting ‘case-study’, for the further implementation of the European Marine Strategy Framework Directive, at the level of this particular Regional Sea. In this way, the experience gained in the implementation of the Water Framework Directive within the ecoregion, together with the information collated in the eleven International Symposia of Oceanography of the Bay of Biscay, celebrated until now, can be very useful, for an ecosystem-based management approach for this Regional Sea.     

A Rising Tide in Bangladesh: livelihood adaptation to climate stress

ABSTRACT

Bangladesh is at the forefront of countries experiencing and debating climate change, despite having contributed little to global emissions, and has the greatest vulnerability to climate change due to inadequate institutional support for the dense population dispersed in low-lying terrain. A micro-level study of livelihoods in the Panpatti Union, a district of the coastal zone exposed to climate stress and an array of other social, economic and political stresses, demonstrated that adaptation strategies to a range of shocks were both reactive and proactive. The persistent nature of shocks, and the limited margins in which to respond, meant that achieving sustainable long-term livelihoods was unusually difficult. Despite cases of dynamism and flexibility, where livelihoods had been effectively diversified, rural people largely failed to reduce their exposure to vulnerability. That was especially true of extremely poor, landless and female-headed households. In such challenging circumstances external interventions were required to ensure sustainable development, but were unlikely because of the isolation of Panpatti and the number of villages and people in similar circumstances. This emphasised the need to develop a more robust livelihoods framework to support the most vulnerable communities in severe economic and environmental contexts where climate change is likely to exacerbate all existing problems.     

The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering

We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of magnitude larger than previous redshift surveys used to address this issue. We measure the projected two-point correlation function of galaxies in a series of volume-limited samples. The projected correlation function is free from any distortion of the clustering pattern induced by peculiar motions and is well described by a power law in pair separation over the range     . The clustering of     galaxies in real space is well-fitted by a correlation length     and power-law slope     . The clustering amplitude increases slowly with absolute magnitude for galaxies fainter than M *, but rises more strongly at higher luminosities. At low luminosities, our results agree with measurements from the Southern Sky Redshift Survey 2 by Benoist et al. However, we find a weaker dependence of clustering strength on luminosity at the highest luminosities. The correlation function amplitude increases by a factor of 4.0 between     and −22.5, and the most luminous galaxies are 3.0 times more strongly clustered than L * galaxies. The power-law slope of the correlation function shows remarkably little variation for samples spanning a factor of 20 in luminosity. Our measurements are in very good agreement with the predictions of the hierarchical galaxy formation models of Benson et al.