PLANNED INCAPACITY TO SUCCEED? POLICY-MAKING STRUCTURE AND POLICY FAILURE

Policies may fail in two analytically distinct ways: they may fail to achieve their goals, or they may fail to retain political support and be terminated. By failing to distinguish between ineffectiveness and political failure, the three most common interpretations of the War on Poverty and the Comprehensive Employment and Training Act (failure owing to central government incompetence, failure owing to pluralism, and "hidden" success) cannot adequately account for the gap between their ambiguous performance and their clear political failure. To understand these differences, one must understand the effect of America's fragmented political structure on the design and implementation of poverty and unemployment remedies. Under resource constraints and given a large degree of policy discretion, American states in the aggregate have retained their historic resistance to social policies that would increase short-term expenditures and reduce the attractiveness of their business climate. These jurisdictions and their Congressional representatives opposed new fully nationalized initiatives, insisting on policy designs that promised fiscal relief while protecting state and local policy control. National policymakers found that grant-in-aid programs offered the path of least resistance in these circumstances. Although social policy grant programs could win initial approval in Congress, these designs proved to be increasingly unwieldy, expensive, and difficult to control in practice. The programs yielded ambiguous overall results but provided unambiguous examples of waste, fraud and abuse, fueling the perception of failure and contributing to the backlash against these programs and their political failure. Copyright 1988 by The Policy Studies Organization.

Atmospheric Escape and Evolution of Terrestrial Planets and Satellites

International audienceThe origin and evolution of Venus', Earth's, Mars' and Titan's atmospheres are discussed from the time when the active young Sun arrived at the Zero-Age-Main-Sequence. We show that the high EUV flux of the young Sun, depending on the thermospheric composition, the amount of IR-coolers and the mass and size of the planet, could have been responsible that hydrostatic equilibrium was not always maintained and hydrodynamic flow and expansion of the upper atmosphere resulting in adiabatic cooling of the exobase temperature could develop. Furthermore, thermal and various nonthermal atmospheric escape processes influenced the evolution and isotope fractionation of the atmospheres and water inventories of the terrestrial planets and Saturn's large satellite Titan efficiently