The Gleaner and Niagara Newspaper, December 18th, 1817

The Gleaner and Niagara Newspaper was a weekly paper in the town of Niagara-on-the-Lake that began publication December 4, 1817 and ceased in 1830. This bound volume has been divided by publication dates. Other dates included in the volume are: 25 December 1817 1818 January 1 1818 January 8 1818 January 15 1818 January 22 There is also a letter that was found inside the bound volume written by Andrew Heron on October 1 1817.

Some aspects of history of Indian mathematics in 18th and early 19th century

This thesis is an attempt to throw light on the works of some Indian Mathematicians who wrote in Arabic or persian In the Introductory Chapter on outline of general history of Mathematics during the eighteenth Bnd nineteenth century has been sketched. During that period there were two streams of Mathematical activity. On one side many eminent scholers, who wrote in Sanskrit, .he l d the field as before without being much influenced by other sources. On the other side there were scholars whose writings were based on Arabic and Persian text but who occasionally drew upon other sources also.

Adaptaci??n de la Sydney Attribution Scale en poblaci??n universitaria espa??ola

Resumen tomado de la publicaci??n

Curriculum Innovation Network Conference - 18th & 19th January 2011

Presentations from the Curriculum Innovation Network Conference that took place on 18th & 19th January 2011 at the University of Southampton. The ambition was to bring together a global network of universities who are engaged in institution-wide curriculum innovation. The focus of the network is to share learning and practice in a collaborative way, to identify best practice and to explore practical solutions to the challenges we face. Keynote speakers from across the world and colleagues from leading universities came together to share their experience on approaches to transforming their curricula and the overall learning experience of their students. The challenges of doing this are significant, and there is much that we can learn from each other as we seek to transform the learning environment of our institutions. We hope that all who attend found these two days of great value in starting and enhancing a global dialogue about education transformation. Additional presentations will be uploaded in due course. Please note the copy right of these presentations remains with the author.

De Sydney 2000 a Alicante 2001 : un proyecto de trabajo para el ámbito científico de diversificación curricular.

Contiene resumen y memoria. Premios Nacionales 2001 a la Innovación Educativa

The Economic anI Racial Implications of the Globalization of Knowledge by Catholic Missionaries in Portuguese India, 16th-18th Centuries

The European Missionaries benefitted from the native Asian sources and knowledge providers much more than it is honestly acknowledged.

The heliospheric Hale cycle over the last 300 years and its implications for a “lost” late 18th century solar cycle

A Hale cycle, one complete magnetic cycle of the Sun, spans two complete Schwabe cycles (also referred to as sunspot and, more generally, solar cycles). The approximately 22-year Hale cycle is seen in magnetic polarities of both sunspots and polar fields, as well as in the intensity of galactic cosmic rays reaching Earth, with odd- and even-numbered solar cycles displaying qualitatively different waveforms. Correct numbering of solar cycles also underpins empirical cycle-to-cycle relations which are used as first-order tests of stellar dynamo models. There has been much debate about whether the unusually long solar cycle 4 (SC4), spanning- 1784–1799, was actually two shorter solar cycles combined as a result of poor data coverage in the original Wolf sunspot number record. Indeed, the group sunspot number does show a small increase around 1794–1799 and there is evidence of an increase in the mean latitude of sunspots at this time, suggesting the existence of a cycle ‘‘4b’’. In this study, we use cosmogenic radionuclide data and associated reconstructions of the heliospheric magnetic field (HMF) to show that the Hale cycle has persisted over the last 300 years and that data prior to 1800 are more consistent with cycle 4 being a single long cycle (the ‘‘no SC4b’’ scenario). We also investigate the effect of cycle 4b on the HMF using an open solar flux (OSF) continuity model, in which the OSF source term is related to sunspot number and the OSF loss term is determined by the heliospheric current sheet tilt, assumed to be a simple function of solar cycle phase. The results are surprising; Without SC4b, the HMF shows two distinct peaks in the 1784–1799 interval, while the addition of SC4b removes the secondary peak, as the OSF loss term acts in opposition to the later rise in sunspot number. The timing and magnitude of the main SC4 HMF peak is also significantly changed by the addition of SC4b. These results are compared with the cosmogenic isotope reconstructions of HMF and historical aurora records. These data marginally favour the existence of SC4b (the ‘‘SC4b’’ scenario), though the result is less certain than that based on the persistence of the Hale cycle. Thus while the current uncertainties in the observations preclude any definitive conclusions, the data favour the ‘‘no SC4b’’ scenario. Future improvements to cosmogenic isotope reconstructions of the HMF, through either improved modelling or additional ice cores from well-separated geographic locations, may enable questions of the existence of SC4b and the phase of Hale cycle prior to the Maunder minimum to be settled conclusively.