Modernising Planning: Public Participation in the UK Planning System

In the UK the formal land-use planning system is once more at a crossroads with the unprecedented levels of public comment on the recent Governmental Green Paper on Planning. A recent international report on the planning process in Westernised countries highlighted a dearth of public participation in the UK planning system this is despite an obvious undercurrent of concern on environmental issues and the like. The paper sets out to gauge the extent of public interest in the Planning system, in the light of current proposals to revise it. The paper concentrates on the nature of public participation in Planning and to consider whether the public are more satisfied with process, seeing it as fair and robust, if they are more actively involved in the process of consultation. Other aspects to consider are the need to seek consultation from the wider public, not just individuals and special interest groups. There are several forgotten frontiers of the past effort to promote public participation. Theory dating from the 1970s exposed differences between sociological approaches in Planning and solutions tended to be lost in complexity of Local Development Plans. Subsequent theory (Healey 1997) has argued for the need to reconcile plural interests across localities. What is neglected in the research is the fuller appreciation of the actual public interest by those in the Planning system. A recent international report by Heriott-Watt University, Edinburgh and DePaul University, Chicago called for the notion of ‘public participation’ to be turned on its head and instead encourage the practice of ‘participatory planning’- the use of third parties to pre-mediate conflicts between stakeholders before and during the process of an open consultation as opposed to seeking public opinions after the plans have been drawn. This paper aims to review the modernising agenda and set out the case for shifting public participation to participatory planning within the context of the UK. Particularly pertinent due to recent recommendations to increase sustainability communities. It uses several qualitative case studies drawn from urban planning authorities and rural districts from the UK, which reveal Local Planning Authorities may be as yet unprepared to fully grasp the concepts underpinning the notion of participatory planning.

Forming American Politics

Originally published in 1994. In this pathbreaking book Alan Tully offers an unprecedented comparative study of colonial political life and a rethinking of the foundations of American political culture. Tully chooses for his comparison the two colonies that arguably had the most profound impact on American political history—New York and Pennsylvania, the rich and varied colonies at the geographical and ideological center of British colonial America.Fundamental to the book is Tully's argument that out of Anglo-American influences and the cumulative character of each colonial experience, New York and Pennsylvania developed their own distinctive but complementary characteristics. In making this case Tully enters—from a new perspective—the prominent argument between the "classical republican" and "liberal" views of early American public thought. He contends that the radical Whig element of classical republicanism was far less influential than historians have believed and that the political experience of New York and Pennsylvania led to their role as innovators of liberal political concepts and discourse. In a conclusion that pursues his insights into the revolutionary and early republican years, Tully underlines a paradox in American political development: not only were the pathbreaking liberal politicians of New York and Pennsylvania the least inclined towards revolutionary fervor, but their political language and concepts—integral to an emerging liberal democratic order—were rooted in oligarchical political practice."A momentous contribution to the burgeoning literature on the middle Atlantic region, and to the vexed question of whether it constitutes a coherent cultural configuration. Tully argues persuasively that it does, and his arguments will have to be reckoned with like few that have gone before, even as he develops an array of differences between the two colonies more subtle and penetrating than any of his predecessors has ever put forth."—Michael Zuckerman, University of Pennsylvania

Our Peculiar Motion Away from the Local Void

The peculiar velocity of the Local Group of galaxies manifested in the Cosmic Microwave Background dipole is found to decompose into three dominant components. The three components are clearly separated because they arise on distinct spatial scales and are fortuitously almost orthogonal in their influences. The nearest, which is distinguished by a velocity discontinuity at ~7 Mpc, arises from the evacuation of the Local Void. We lie in the Local Sheet that bounds the void. Random motions within the Local Sheet are small. Our Galaxy participates in the bulk motion of the Local Sheet away from the Local Void. The component of our motion on an intermediate scale is attributed to the Virgo Cluster and its surroundings, 17 Mpc away. The third and largest component is an attraction on scales larger than 3000 km/s and centered near the direction of the Centaurus Cluster. The amplitudes of the three components are 259, 185, and 455 km/s, respectively, adding collectively to 631 km/s in the reference frame of the Local Sheet. Taking the nearby influences into account causes the residual attributed to large scales to align with observed concentrations of distant galaxies and reduces somewhat the amplitude of motion attributed to their pull. On small scales, in addition to the motion of our Local Sheet away from the Local Void, the nearest adjacent filament, the Leo Spur, is seen to be moving in a direction that will lead to convergence with our filament. Finally, a good distance to an isolated galaxy within the Local Void reveals that this dwarf system has a motion of at least 230 km/s away from the void center. Given the velocities expected from gravitational instability theory in the standard cosmological paradigm, the distance to the center of the Local Void must be at least 23 Mpc from our position. The Local Void is large!Comment: Tentatively scheduled for Astrophysical Journal, 676 (March 20), 2008. 18 figures, 3 tables including web link for 2 tables, web links to 2 video

Deploying Wireless Sensor Devices in Intelligent Transportation System Applications

As future intelligent infrastructure will bring together and connect individuals, vehicles and infrastructure through wireless communications, it is critical that robust communication technologies are developed. Mobile wireless sensor networks are self-organising mobile networks where nodes exchange data without the need for an underlying infrastructure. In the road transport domain, schemes which are fully infrastructure-less and those which use a combination of fixed (infrastructure) devices and mobile devices fitted to vehicles and other moving objects are of significant interest to the ITS community as they have the potential to deliver a ‘connected environment’ where individuals, vehicles and infrastructure can co-exist and cooperate, thus delivering more knowledge about the transport environment, the state of the network and who indeed is travelling or wishes to travel. This may offer benefits in terms of real-time management, optimisation of transportation systems, intelligent design and the use of such systems for innovative road charging and possibly carbon trading schemes as well as through the CVHS (Cooperative Vehicle and Highway Systems) for safety and control applications. As the wireless sensor networks technology is still relatively new and very little is known about its real application in the transport domain. Our involvement in the transport-related projects provides us with an opportunity to carry out research and development of wireless sensor network applications in transport systems. This chapter outlines our experience in the ASTRA (ASTRA, 2005), TRACKSS (TRACKSS, 2007) and EMMA (EMMA, 2007) projects and provides an illustration of the important role that the wireless sensor technology can play in future ITS. This chapter also presents encouraging results obtained from the experiments in investigating the feasibility of utilising wireless sensor networks in vehicle and vehicle to infrastructure communication in real ITS applications

Integrating Smartdust into Intelligent Transportation System

The last few years have seen the emergence of many new technologies that can potentially have major impacts on Intelligent Transportation Systems (ITS). One of these technologies is a micro-electromechanical device called smartdust. A smartdust device (or a mote) is typically composed of a processing unit, some memory, and a radio chip, which allows it to communicate wirelessly with other motes within range. These motes can also be augmented with additional sensors – such as those for detecting light, temperature and acceleration – hence enhancing their features and making their application areas virtually limitless. As the smartdust concept is still relatively new, and very little is known about its application in transport domain, conducting research in this area may prove to be very valuable. It is generally perceived that smartdust will become the low-cost, ubiquitous sensor of the future, especially once its size shrinks dramatically to merit its name. Our involvement in several transport-related EU and UK funded projects (ASTRA, 2005; ASK-IT, 2007; EMMA, 2007; Foot-LITE, 2007; MESSAGE, 2007; TRACKSS, 2007) provides us with an opportunity to carry out experiments and to develop demonstrations of smartdust applications in transport systems. We also have a chance to investigate how smartdust can be used in collaboration with other (more traditional) transport sensors for developing better Co-operative Transport Systems (CTS). This paper outlines our experience in these projects and provides an illustration on the important role that the smartdust technology can play in future ITS. We also present encouraging results obtained from our experiments in investigating the feasibility of utilising smartdust in real ITS applications

Interictal Dysfunction of a Brainstem Descending Modulatory Center in Migraine Patients

Background: The brainstem contains descending circuitry that can modulate nociceptive processing (neural signals associated with pain) in the dorsal horn of the spinal cord and the medullary dorsal horn. In migraineurs, abnormal brainstem function during attacks suggest that dysfunction of descending modulation may facilitate migraine attacks, either by reducing descending inhibition or increasing facilitation. To determine whether a brainstem dysfunction could play a role in facilitating migraine attacks, we measured brainstem function in migraineurs when they were not having an attack (i.e. the interictal phase). Methods and Findings: Using fMRI (functional magnetic resonance imaging), we mapped brainstem activity to heat stimuli in 12 episodic migraine patients during the interictal phase. Separate scans were collected to measure responses to 41°C and noxious heat (pain threshold+1°C). Stimuli were either applied to the forehead on the affected side (as reported during an attack) or the dorsum of the hand. This was repeated in 12 age-gender-matched control subjects, and the side tested corresponded to that in the matched migraine patients. Nucleus cuneiformis (NCF), a component of brainstem pain modulatory circuits, appears to be hypofunctional in migraineurs. 3 out of the 4 thermal stimulus conditions showed significantly greater NCF activation in control subjects than the migraine patients. Conclusions: Altered descending modulation has been postulated to contribute to migraine, leading to loss of inhibition or enhanced facilitation resulting in hyperexcitability of trigeminovascular neurons. NCF function could potentially serve as a diagnostic measure in migraine patients, even when not experiencing an attack. This has important implications for the evaluation of therapies for migraine

Galaxy redshift surveys selected by neutral hydrogen using FAST

We discuss the possibility of performing a substantial spectroscopic galaxy redshift survey selected via the 21cm emission from neutral hydrogen using the Five-hundred metre Aperture Spherical Telescope (FAST) to be built in China. We consider issues related to the estimation of the source counts and optimizations of the survey, and discuss the constraints on cosmological models that such a survey could provide. We find that a survey taking around two years could detect ~10^7 galaxies with an average redshift of ~0.15 making the survey complementary to those already carried out at optical wavelengths. These conservative estimates have used the z=0 HI mass function and have ignored the possibility of evolution. The results could be used to constrain Gamma = (Omega_m h) to 5 per cent and the spectral index, n_s, to 7 per cent independent of cosmic microwave background data. If we also use simulated power spectra from the Planck satellite, we can constrain w to be within 5 per cent of -1.Comment: 13 pages, 15 figures, Accepted by MNRAS, minor correction