Exhibitions & Performances DRHA2014

Communication Futures: Connecting interdisciplinary design practices in arts/culture, academia and the creative industries. Site-Specific projections, Exhibitions, Installations in and around the Old Royal Naval College, Greenwich Maritime campus. This catalogue includes exhibits related to practice-based research in performance and arts. Delegates presenting theatrical performances or an installations. For over 13 years DRHA: Digital Research in the Humanities and Arts (Previously named: Digital Resources in Humanities and the Arts) continues to be a key gathering for all those are influenced by the digitization of cultural activity, recourses and heritage in the UK

An international campaign of the 19th century to determine the solar parallax - The US Naval expedition to the southern hemisphere 1849 - 1852

In 1847 Christian Ludwig Gerling, Marburg (Germany), suggested the solar parallax to be determined by measuring the position of Venus close to its inferior conjunction, especially at the stationary points, from observatories on nearly the same meridian but widely differing in latitude. James M. Gilliss,astronomer at the newly founded U.S. Naval Observatory, enthusiastically adopted this idea and procured a grant for the young astronomical community of the United States for an expedition to Chile. There they were to observe several conjunctions of Venus and oppositions of Mars, while the accompanying measurements were to be taken at the US Naval Observatory in Washington D.C. and the Harvard College Observatory at Cambridge, USA. This expedition was supported by A. v. Humboldt, C.F. Gau{\ss}, J.F. Encke, S.C. Walker, A.D. Bache, B. Peirce and others. From 1849 to 1852 not only were astronomical, but also meteorological and magnetic observations and measurements recorded, mainly in Santa Lucia close to Santiago, Chile. By comparing these measurements with those taken simultaneously at other observatories around the world the solar parallax could be calculated, although incomplete data from the corresponding northern observatories threatened the project's success. In retrospect this expedition can be recognized as the foundation of the Chilean astronomy. The first director of the new National Astronomical Observatory of Chile was Dr. C.W. Moesta, a Hessian student of Christian Ludwig Gerling's. The exchange of data between German, American and other astronomers during this expedition was well mediated by J.G. Fl\"ugel, consul of the United States of America and representative of the Smithsonian Institution in Europe, who altogether played a major role in nurturing the relationship between the growing scientific community in the U.S. and the well established one in Europe at that time.Comment: 20 pages, 7 figure

Glasgow time signals

From 1859 to 1864, both visual and audio one o’clock time signals operated in Glasgow. Although the University carried a remit to provide the city’s time, following convoluted processes of establishment, a local chronometer-maker operated a time ball for 4 years. Towards the end of the period, time guns were triggered by telegraph from the Royal Observatory Edinburgh. Both exercises caused aggravation for the University. For the ball, the Professor of Astronomy, John Pringle Nichol, failed to convince the City Council that the “drop” control should originate from the University’s Observatory. For the guns, Robert Grant, the newly appointed Astronomy Chair holder, was aggrieved by the Astronomer Royal for Scotland, Piazzi Smyth, appearing to operate above his station. Rather than having only a once per day reference, both projects were abandoned as the University laid a dedicated telegraph cable from its observatory to control many public clocks and additional clocks with large sweep fingers indicating exact time to the second

Stargazing: Observatories at Gettysburg College, 1874-Present

Astronomy has long been a subject which has attracted the interest of man. Examples of early astronomers can be found in many ancient civilizations, including but not limited to, the Egyptians, the Chinese and the Greeks. As time passed the methods for interpreting the stars and theories that surrounded them changed concordant with the technology available. One of the largest breakthroughs in the world of astronomy was the invention of the telescope in the early seventeenth century. Often mis-attributed to Galileo (who was responsible for building the first reflecting telescope in 1688), the telescope was actually first designed by a Dutch spectacle-maker by the name of Johann Lippershey. Improvements were eventually made upon these designs leading to the creation of government funded observatories, such as the Royal Greenwich Observatory in England, and later private and collegiate research observatories. By the early to mid-nineteenth century, the astronomical craze had begun to develop in America, resulting in the creation of many new observatories in the North and West (now the Mid-West). [excerpt] Course Information: Course Title: HIST 300: Historical Method Academic Term: Spring 2006 Course Instructor: Dr. Michael J. Birkner \u2772 Hidden in Plain Sight is a collection of student papers on objects that are hidden in plain sight around the Gettysburg College campus. Topics range from the Glatfelter Hall gargoyles to the statue of Eisenhower and from historical markers to athletic accomplishments. You can download the paper in pdf format and click View Photo to see the image in greater detail.https://cupola.gettysburg.edu/hiddenpapers/1007/thumbnail.jp

Using the Rural Economic and Enterprise Development (REED) framework for analysis and joint action: outline and workplan for action research

The framework for fostering Rural Economic and Enterprise Development (REED) which is based on the analysis of successes and experiences of programmes and projects by an international group of practitioners from different professional backgrounds and countries is an example of a more holistic and spatial approach to local, rural and urban development. The framework, which tries to address the shortcomings of the traditional rural-urban dichotomy, is comprised of ten cornerstones for successful intervention, covering the policy and institutional dimension, access to infrastructure, services and markets, entrepreneurial competence and stakeholder links (see Figure 1). The REED framework can be applied at different levels, i.e., national and regional, because it is areabased. For example, many decisions concerning the political, economic and institutional environment for Rural Economic and Enterprise Development are made at national level. Decision-makers on public policies for rural areas are charged with designing strategies for rural development. Increasingly, this is done in a programmatic way, such as in inter-ministerial committees for designing PRSPs, sector investment programmes (SIPs) and sector-wide approaches (SWAPs). The REED framework adds value to the planning process because it feeds the perceptions, needs and experiences of relevant stakeholders in a systematic way. Where the focus is on developing a certain region (at sub-national level), regional development authorities can use the REED framework to create a dynamic environment for economic activity and to stimulate innovation. In this way, the specific characteristics of the region and the relevant framework conditions can be taken into consideration when elaborating and formulating key strategies, processes and possible ways to implement them, related to the individual cornerstones (see Figure 1). Within the cycle of typical government and donor-supported public investment, policies/ interventions, there are several options for applying the REED framework

On Stability of the Demand for Money in a Developing OECD

This paper empirically analyses the stability of the narrow money demand function (M1) in Turkey for the period 1950-2002. As part of the IMF-sponsored stabilisation programme, Turkey has been pursuing base money targets. To ascertain whether this policy framework satisfies the necessary condition for effectiveness, we estimate and test for the stability of Turkish M1 by employing a recent single cointegration procedure proposed by Pesaran et al. (2001) along with the CUSUM and CUSUMSQ stability tests. We demonstrate that there is a stable money demand function and it could be used as an intermediate target of monetary policy in Turkey.co-integration, money demand, stability, Turkey

Sunspot observations on 10 and 11 February 1917: a case study in collating known and previously undocumented records

An extensive investigation of ships’ logs, as part of the ‘Old Weather’ citizen-science project, identified a sunspot observation made from HMS Hilary on 10 February 1917. This sunspot record was accompanied by detailed meteorological records that have enabled a reconstruction of the conditions under which the observation was made (overcast with detached clouds). Although there is no incontrovertible evidence that this was an unaided-eye observation, comparison with an unaided-eye observation recorded on the 11 February 1917 in a local treatise from Hénán province in China confirms that this sunspot group was visible to the unaided eye. White-light photographs from the Dehra Dun Observatory confirm the detailed description of the sunspot group provided by the naval observer. Moreover, comparisons with tabular data published by the Royal Observatory, Greenwich, confirm the statement that this was an unusually large sunspot group. Indeed, on 11 February 1917 the area of the sunspot group was greater than the area of any sunspot group recorded previously at the Royal Observatory, Greenwich. A comparison with a modern unaided-eye observation confirms that it is possible to observe sunspots under meteorological conditions similar to those experienced on-board HMS Hilary