Reminiscences of East Greenwich

Address delivered before the East Greenwich Business Men’s Association by Henry E. Turner, April 11, 1892. Henry E. Turner, a member of the East Greenwich Business Men’s Association, recounts the early history of notable events and people of the town of East Greenwich, Rhode Island, during the first half of the 19thcentury.https://digitalcommons.providence.edu/ri_history/1005/thumbnail.jp

Decomposing the Growth in Residential Land in the United States

This paper decomposes the growth in land occupied by residences in the United States to give the relative contributions of changing demographics versus increases in the land area used by individual households. Between 1976 and 1992 the amount of residential land in the United States grew 47.5% while population only grew 17.8%. At first glance, this suggests an important role for per-household increases. However, the calculations in this paper show that only 24.3% of the growth in residential land area can be attributed to State level changes in land per household. 37.5% is due to overall population growth, 5.9% to the shift of population towards States with larger houses, 22.7% to an increase in the number of households over this period, and the remaining 9.5% to interactions between these changes. There are large differences across states and metropolitan areas in the relative importance of these components.land use, population growth

Dear old southland

https://digitalcommons.ithaca.edu/sheetmusic/1128/thumbnail.jp

After You\u27ve Gone

https://digitalcommons.library.umaine.edu/mmb-vp/1155/thumbnail.jp

Astronomy with integral field spectroscopy:: observation, data analysis and results

With a new generation of facility instruments being commissioned for 8 metre telescopes, integral field spectroscopy will soon be a standard tool in astronomy, opening a range of exciting new research opportunities. It is clear, however, that reducing and analyzing integral field data is a complex problem, which will need considerable attention before the full potential of the hardware can be realized. The purpose of this thesis is therefore to explore some of the scientific capabilities of integral field spectroscopy, developing the techniques needed to produce astrophysical results from the data. Two chapters are dedicated to the problem of analyzing observations from the densely-packed optical fibre instruments pioneered at Durham. It is shown that, in the limit where each spectrum is sampled by only one detector row, data maybe treated in a similar way to those from an image slicer. The properties of raw fibre data are considered in the context of the Sampling Theorem and methods for three dimensional image reconstruction are discussed. These ideas are implemented in an IRAF data reduction package for the Thousand Element Integral Field Unit (TEIFU), with source code provided on the accompanying compact disc. Two observational studies are also presented. In the first case, the 3D infrared image slicer has been used to test for the presence of a super-massive black hole in the giant early-type galaxy NGC 1316. Measurements of the stellar kinematics do not reveal a black hole of mass 5 x l0(^9)M©, as predicted from bulge luminosity using the relationship of Kormendy & Richstone (1995). The second study is an investigation into the origin of [Fell] line emission in the Seyfert galaxy NGC4151, using Durham University's SMIRFS-IFU. By mapping [Fell] line strength and velocity at the galaxy centre, it is shown that the emission is associated with the optical narrow line region, rather than the radio jet, indicating that the excitation is primarily due to photoionizing X-rays.Finally, a report is given on the performance of TEIFU, which was commissioned at the William Herschel Telescope in 1999. Measurements of throughput and fibre response variation are given and a reconstructed test observation of the radio galaxy 3C 327 is shown, demonstrating the functionality of the instrument and software

Causes of sprawl: A portrait from space

We study the extent to which US urban development is sprawling and consider what determines differences in sprawl across space. Using remote-sensing data to track the evolution of land use on a grid of 8.7 billion 30x30 metre cells, we measure sprawl as the amount of undeveloped land surrounding an average urban dwelling. On this measure, while the extent of sprawl remained roughly unchanged between 1976 and 1992, it varied dramatically across metropolitan areas. Ground water availability, temperate climate, rugged terrain, decentralized employment, early public transport infrastructure, uncertainty about metropolitan growth, and unincorporated land in the urban fringe all increase sprawl.urban sprawl; land development; remote sensing

Fat City: The Relationship Between Urban Sprawl and Obesity

We study the relationship between urban sprawl and obesity. Using data that tracks individuals over time, we find no evidence that urban sprawl causes obesity. We show that previous findings of a positive relationship most likely reflect a failure to properly control for the fact the individuals who are more likely to be obese choose to live in more sprawling neighborhoods. Our results indicate that current interest in changing the built environment to counter the rise in obesity is misguided.urban sprawl; obesity; selection effects