Empathetic Practice: Reflective Reading Journals in the CEGEP Classroom

Abstract: In order to observe whether or not students appreciate the opportunity to learn affectively, this research was designed as an exploratory project aimed at identifying the ways in which reflective reading journals enabled students to respond empathetically to works of literary fiction. To understand the relationship between the act of reading and the experience of empathy, several questions were asked. The main question was: In what ways do reflective reading journals encourage students to read and understand works of fiction empathetically? Related concerns were taken into consideration: How do students describe their experience of empathy in response to the literary techniques such as plot and characterization? Students were also expected to consider the ways in which their thoughts on writing reflective reading journals underscored the need to forge empathetic awareness of the variety of opinions, experiences, and perspectives expressed in the works of fiction.||Résumé: Dans le but d'observer si les étudiants apprécient ou non la possibilité d'apprendre affectivement, cette recherche a été conçue comme un projet exploratoire visant à identifier les moyens que les journaux de lecture de réflexion ont permis aux étudiants de répondre avec empathie aux oeuvres de fiction littéraire. Pour comprendre la relation entre l'acte de lecture et l'expérience de l'empathie, plusieurs questions ont été posées. La question principale était la suivante: de quelles façons les journaux de lecture de réflexion encouragent les étudiants à lire et comprendre des oeuvres de fiction avec empathie? Des préoccupations du même ordre ont été prises en considération: Comment les étudiants décrivent-ils leur expérience de l'empathie en réponse aux techniques littéraires telles que l'intrigue et la caractérisation? Les étudiants doivent aussi examiner les façons dont leurs idées sur la rédaction de journaux de lecture de réflexion ont mis en évidence la nécessité de forger la prise de conscience empathique de la diversité d'opinions, d'expériences et de perspectives exprimée dans les oeuvres de fiction.

Solar magnetic carpet I: simulation of synthetic magnetograms

This paper describes a new 2D model for the photospheric evolution of the magnetic carpet. It is the first in a series of papers working towards constructing a realistic 3D non-potential model for the interaction of small-scale solar magnetic fields. In the model, the basic evolution of the magnetic elements is governed by a supergranular flow profile. In addition, magnetic elements may evolve through the processes of emergence, cancellation, coalescence and fragmentation. Model parameters for the emergence of bipoles are based upon the results of observational studies. Using this model, several simulations are considered, where the range of flux with which bipoles may emerge is varied. In all cases the model quickly reaches a steady state where the rates of emergence and cancellation balance. Analysis of the resulting magnetic field shows that we reproduce observed quantities such as the flux distribution, mean field, cancellation rates, photospheric recycle time and a magnetic network. As expected, the simulation matches observations more closely when a larger, and consequently more realistic, range of emerging flux values is allowed (4×1016 - 1019 Mx). The model best reproduces the current observed properties of the magnetic carpet when we take the minimum absolute flux for emerging bipoles to be 4×1016 Mx. In future, this 2D model will be used as an evolving photospheric boundary condition for 3D non-potential modeling.

Solar magnetic carpet II: coronal interactions of small-scale magnetic fields

This paper is the second in a series of studies working towards constructing a realistic, evolving, non-potential coronal model for the solar magnetic carpet. In the present study, the interaction of two magnetic elements is considered. Our objectives are to study magnetic energy build-up, storage and dissipation as a result of emergence, cancellation, and flyby of these magnetic elements. In the future these interactions will be the basic building blocks of more complicated simulations involving hundreds of elements. Each interaction is simulated in the presence of an overlying uniform magnetic field, which lies at various orientations with respect to the evolving magnetic elements. For these three small-scale interactions, the free energy stored in the field at the end of the simulation ranges from 0.2 – 2.1×1026 ergs, whilst the total energy dissipated ranges from 1.3 – 6.3×1026 ergs. For all cases, a stronger overlying field results in higher energy storage and dissipation. For the cancellation and emergence simulations, motion perpendicular to the overlying field results in the highest values. For the flyby simulations, motion parallel to the overlying field gives the highest values. In all cases, the free energy built up is sufficient to explain small-scale phenomena such as X-ray bright points or nanoflares. In addition, if scaled for the correct number of magnetic elements for the volume considered, the energy continually dissipated provides a significant fraction of the quiet Sun coronal heating budget.

Solar magnetic carpet III: coronal modelling of synthetic magnetograms

This article is the third in a series working towards the construction of a realistic, evolving, non-linear force-free coronal-field model for the solar magnetic carpet. Here, we present preliminary results of 3D time-dependent simulations of the small-scale coronal field of the magnetic carpet. Four simulations are considered, each with the same evolving photospheric boundary condition: a 48-hour time series of synthetic magnetograms produced from the model of Meyer et al. ( Solar Phys. 272, 29, 2011). Three simulations include a uniform, overlying coronal magnetic field of differing strength, the fourth simulation includes no overlying field. The build-up, storage, and dissipation of magnetic energy within the simulations is studied. In particular, we study their dependence upon the evolution of the photospheric magnetic field and the strength of the overlying coronal field. We also consider where energy is stored and dissipated within the coronal field. The free magnetic energy built up is found to be more than sufficient to power small-scale, transient phenomena such as nanoflares and X-ray bright points, with the bulk of the free energy found to be stored low down, between 0.5 - 0.8 Mm. The energy dissipated is currently found to be too small to account for the heating of the entire quiet-Sun corona. However, the form and location of energy-dissipation regions qualitatively agree with what is observed on small scales on the Sun. Future MHD modelling using the same synthetic magnetograms may lead to a higher energy release.

The storage and dissipation of magnetic energy in the quiet sun corona determined from SDO/HMI magnetograms

In recent years, higher cadence, higher resolution observations have revealed the quiet-Sun photosphere to be complex and rapidly evolving. Since magnetic fields anchored in the photosphere extend up into the solar corona, it is expected that the small-scale coronal magnetic field exhibits similar complexity. For the first time, the quiet-Sun coronal magnetic field is continuously evolved through a series of non-potential, quasi-static equilibria, deduced from magnetograms observed by the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory, where the photospheric boundary condition which drives the coronal evolution exactly reproduces the observed magnetograms. The build-up, storage, and dissipation of magnetic energy within the simulations is studied. We find that the free magnetic energy built up and stored within the field is sufficient to explain small-scale, impulsive events such as nanoflares. On comparing with coronal images of the same region, the energy storage and dissipation visually reproduces many of the observed features. The results indicate that the complex small-scale magnetic evolution of a large number of magnetic features is a key element in explaining the nature of the solar corona.

Simulating the formation of a sigmoidal flux rope in AR10977 from SOHO/MDI magnetograms

The modeling technique of Mackay et al. is applied to simulate the coronal magnetic field of NOAA active region AR10977 over a seven day period (2007 December 2-10). The simulation is driven with a sequence of line-of-sight component magnetograms from SOHO/MDI and evolves the coronal magnetic field though a continuous series of non-linear force-free states. Upon comparison with Hinode/XRT observations, results show that the simulation reproduces many features of the active region's evolution. In particular, it describes the formation of a flux rope across the polarity inversion line during flux cancellation. The flux rope forms at the same location as an observed X-ray sigmoid. After five days of evolution, the free magnetic energy contained within the flux rope was found to be 3.9 × 1030 erg. This value is more than sufficient to account for the B1.4 GOES flare observed from the active region on 2007 December 7. At the time of the observed eruption, the flux rope was found to contain 20% of the active region flux. We conclude that the modeling technique proposed in Mackay et al.—which directly uses observed magnetograms to energize the coronal field—is a viable method to simulate the evolution of the coronal magnetic field.

Modelling the Sun's small scale global photospheric magnetic field

We present a new model for the Sun's global photospheric magnetic field during a deep minimum of activity, in which no active regions emerge. The emergence and subsequent evolution of small- scale magnetic features across the full solar surface is simulated, subject to the influence of a global supergranular flow pattern. Visually, the resulting simulated magnetograms reproduce the typical structure and scale observed in quiet Sun magnetograms. Quantitatively, the simulation quickly reaches a steady state, resulting in a mean field and flux distribution that are in good agreement with those determined from observations. A potential coronal magnetic field is extrapolated from the simulated full Sun magnetograms, to consider the implications of such a quiet photospheric magnetic field on the corona and inner heliosphere. The bulk of the coronal magnetic field closes very low down, in short connections between small-scale features in the simulated magnetic network. Just 0.1% of the photospheric magnetic flux is found to be open at 2:5 Rʘ, around 10 - 100 times less than that determined for typical HMI synoptic map observations. If such conditions were to exist on the Sun, this would lead to a significantly weaker interplanetary magnetic field than is presently observed, and hence a much higher cosmic ray flux at Earth.

Annual Report of the Game Department for the year ended 31st December 1938

The annual report presents information on the following under fisheries section Breaches of Game Laws (Fish Sections) Development and Control of the Lake Victoria Fishing Industry. Collection of Statistics Statistical Tables.- (A) Number of half-yearly licences issued (B) Quantities and value of nets imported (C) Dried fish handled by Railways and Steamers (D) Smoked and salted fish exported to the Belgian Congo Mpondwe Customs Post Lake Bunyonyi Lake Mugisha (or Kaiyumbu) Lake Chahafi Lake Mulehe Lake Mutanda Lake Saka Lake Nabugabo Lake Kachira and Lake Kijanebalola Lake Kyoga Commercial Development:- Lake Edward and associated fisheries Uganda Fisheries Limited Nsonzi Fishery, Kigezi Experimental Nets in Lake Victoria Legislation (B) angling a) Trout (b) Nile pereh or mpufa

Annual Report of the Game Department for the year ended 31st December, 1947

) General (2) Legislation (3) Nets (4) Imports and Exports of Dried Fish (B) Economic:- (I) Lake Victoria (2) Lake Albert (including the Albert Nile (3) Lake Edward and Associated Fisheries (4) Lake Kyoga (5) Minor Lakes, Dams and the Victoria Nile (6) Introductions (7) Fish Transfers (8) Crocodiles:- (C) Angling Trout Nile Perch Barbel Tilapia Variabilis

Annual Report of the Game Department for the year ended 31st December, 1948

Fisheries section of the annual report covers the following A. ADMINISTRATION (1) General, (2) Legislation, (3) Nets (4) Imports and Exports of Dried Fish, (B) ECONOMIC :( 1) Lake Victoria, (2) Lake Albert (including the Albert Nile), (3) Lake Edward and Associated Fisheries, (4) Report by Fish Culturist, (5) Lake Kyoga, (6) Minor Lakes and the Victoria Nile, (7) Dams,(8) Introductions,(9) Fish Transfers (10) Crocodiles:(i) Control,(ii) Industry, (iii) General (ll) General Notes, (C) ANGLING:Trout, Nile Perch Barbei, Tilapia variabilis.

Annual Report of the Game Department for the year ended 31st December, 1935

The fisheries section of the Annual report provides information on the following: Development and Control of the Victoria Nyanza Fishing Industry, Preparation of Statistics Statistical Tables: (A) Number of half yearly licences issued; (B) Quantities of nets imported; (0) Dried fish landed from Sese and Kome; (D) Dried fish imported from Mwanza ; (E) Dried fish exported to Belgian Congo; Lake Bunyonyi Lake Mutanda Lake Mureyhe Lake Mugisha (or Raiyumbu) I,ake Saka Lake Wamala Commercial Development: (i) Lake Albert: (ii) Lake Edward (iii) Other Waters (iv) Nsonzi Fishery, Kigezi (v) Introductions Experimental Nets and fisheries legislation

Annual Report of the Game Department for the year ended 31st December 1949

The fisheries section of the Annual report provides information on the following: (1) General information (2) Legislation (3) Nets (4) Imports and Exports of Dried Fish B) Economic:- (1) Lake Victoria (2) Lake Albert (including the Albert Nile) (3) Report by Lake Albert Fisheries Officer (4) Lake Edward and Associated Fisheries (5) Lake Kyoga (6) Minor Lakes and the Victoria Nile (7) Dams and (8)Fish Transfers

Annual Report of the Game and Fisheries Department for the period 1st January, 1954, to 30th June, 1955

The fisheries section of the annual report covers information from the following regions: Lake Albert Region: Introduction Staff Launch Licensing Production Export to the Belgian Congo Marketing Departmental Activities Sporting Fishing Statistics Rainfall and Fish Landing Acholi region Lakes George/Edward Region: Introduction General Lake George The Kazinga Channel-Katunguru Lake Edward Minor Lakes Ruwenzori Trout Fisheries Launch Records of Catches Lake Kyoga Region: Introduction General Lake, Kyoga and Minor Lakes Production and fish farming

Reading Pitscottie's Cronicles: a case study on the history of literacy in Scotland, 1575-1814

This thesis addresses a range of research questions regarding literacy in early modern Scotland. Using the early modern manuscripts and printed editions of Robert Lindsay of Pitscottie’s late sixteenth-century 'Cronicles of Scotland' as a case study on literacy history, this thesis poses the complementary questions of how and why early modern Scottish reading communities were encountering Pitscottie’s 'Cronicles', and how features of the material page can be interpreted as indicators of contemporary literacy practices. The answers to these questions then provide the basis for the thesis to ask broader socio-cultural and theoretical questions regarding the overall literacy environment in Scotland between 1575 and 1814, and how theorists conceptualise the history of literacy. Positioned within the theoretical groundings of historical pragmatics and ‘new philology’ – and the related approach of pragmaphilology – this thesis returns to the earlier philological practice of close textual analysis, and engages with the theoretical concept of mouvance, in order to analyse how the changing ‘form’ of Pitscottie’s 'Cronicles', as it was reproduced in manuscript and print throughout the early modern period, indicates its changing ‘function’. More specifically, it suggests that the punctuation practices and paratextual features of individual witnesses of the text function to aid the highly-nuanced reading practices and purposes of the discrete reading communities for which they were produced. This thesis includes extensive descriptive material which presents previously unrecorded data regarding twenty manuscripts and printed witnesses of Pitscottie’s 'Cronicles', contributing to a gap in Scotland’s literary/historiographical canon. It then analyses this material using a transferable methodological framework which combines the quantitative analysis of micro-data with qualitative analysis of this data within its socio-cultural context, in order to conduct diachronic comparative analysis of copy-specific information. The principal findings of this thesis suggest that Pitscottie’s 'Cronicles' were being read for a combination of devotional and didactic purposes, and that multiple reading communities, employing highly nuanced reading practices, were encountering the text near-contemporaneously. This thesis further suggests that early modern literacy practices, and the specific reading communities which employ them, should be described as existing within a spectrum of available practices (i.e. more or less oral/aural or silent, and intensive or extensive in practice) rather than as dichotomous entities. As such, this thesis argues for the rejection of evolutionary theories of the history of literacy, suggesting that rather than being described antithetically, historical reading practices and purposes must be recognised as complex, coexisting socio-cultural practices, and the multiplicity of reading communities within a single society must be acknowledged and analysed as such, as opposed to being interpreted as universal entities.

Objectives for management of socio-ecological systems in the Great Barrier Reef region, Australia

A wide range of goals and objectives have to be taken into account in natural resources management. Defining these objectives in operational terms, including dimensions such as sustainability, productivity, and equity, is by no means easy, especially if they must capture the diversity of community and stakeholder values. This is especially true in the coastal zone where land activities affect regional marine ecosystems. In this study, the aim was firstly to identify and hierarchically organise the goals and objectives for coastal systems, as defined by local stakeholders. Two case study areas are used within the Great Barrier Reef region being Mackay and Bowen–Burdekin. Secondly, the aim was to identify similarities between the case study results and thus develop a generic set of goals to be used as a starting point in other coastal communities. Results show that overarching high-level goals have nested sub-goals that contain a set of more detailed regional objectives. The similarities in high-level environmental, governance, and socio-economic goals suggest that regionally specific objectives can be developed based on a generic set of goals. The prominence of governance objectives reflects local stakeholder perceptions that current coastal zone management is not achieving the outcomes they feel important and that there is a need for increased community engagement and co-management. More importantly, it raises the question of how to make issues relevant for the local community and entice participation in the local management of public resources to achieve sustainable environmental, social, and economic management outcomes. © 2015 Springer-Verlag Berlin Heidelberg