The role of space related non-governmental organizations (NGOs) in capacity building

Non-governmental organizations (NGOs) play a unique role in international affairs, providing access to resources, expertise, and assistance to supplement State resources. Sometimes the diplomatic skills and unofficial access of NGOs to policymakers through Track Two diplomacy can move a previously stalled critical issue forward and assist policymakers from different countries to find common ground outside official channels. Because they work outside of official channels, they are not bound by State policy that may inhibit negotiations between States. Some also have a convening power that sometimes makes it possible for State representatives to meet discipline experts and each other for informal discussions on issues of mutual interest. Finally, NGOs can draw attention to issues that may be overlooked or avoided by State organizations.     

Interdisciplinary Odysseys: The ESF/ESA/ESPI Vienna Conference on Humans in Outer Space

An interdisciplinary approach to discussing the human presence in outer space was undertaken on 11–12 October 2007 by the European Science Foundation (ESF), ESA and the European Space Policy Institute (ESPI). At the ‘Humans in Outer Space—Interdisciplinary Odysseys’ conference space experts and scholars from the area of humanities as well as social sciences discussed the roles disciplines such as law, philosophy, ethics, culture, art and psychology will increasingly play in space exploration. Conference output took form in the ‘Vienna Vision’, which provides a unique European perspective on the various needs and interests of humanities and social sciences linked with space exploration. This report presents the goals and outcome of the conference, as well describing the analysis leading to the creation of the Vienna Vision.     

Time dependent accretion onto a black hole in a disk plus corona system

Hard X-ray lightcurves exhibit delays of 1 s with respect to the soft X-ray lightcurves when the microquasar GRS 1915+105 is in the state of frequent, regular outbursts. Such outbursts are supposed to be driven by the radiation pressure instability of the inner disk parts. The hard X-ray delays are then caused by the time needed for the adjustment of the corona to changing conditions in the underlying disk. We support this claim by the computation of the time evolution of the disk, including a non-stationary evaporation of the disk and mass exchange with the corona.