Summary: Summary of essay main findings and critical evaluation of the research process. Conclusions: Summary of main analytical points from the research and recommendations for future research. Recommendations: Appropriate costed recommendations for change to policy and practice in the topic area should be made. Personal reflection: 500 words of personal reflection. In addition to requiring a large commitment from the student, the dissertation also requires a critical input from staff in the form of individual consultation and supervision. . Most staff are themselves interested in and engaged in research and therefore supervising student dissertations can be rewarding for both staff and students. Staff and students should be guided by the postgraduate masters Dissertation Handbook: guidelines for students, supervisors and Markers - mahrm dissertations, a guide to successful Completion. It is vital that appropriate supervisors are allocated to each dissertation topic. .
The main body of needed the dissertation. Depending on the project topic the main body of the dissertation may be structured in slightly different ways. . The following presents a guideline which students should discuss with their supervisor. Introduction: Rationale to the research, background to the research, and aims and objectives of the research. Literature review: Outline of previous research and critical evaluation of existing literature and research. Methodology: Outline of research philosophy and research methods and analysis used encompassing critical evaluation of the methods used. Findings: Outline of findings of research. Analysis: Analysis of findings.
List of tables : Individual listing of titles and pages of any tables, graphs and statistics. List of figures : Individual listing of titles and pages of photographs, illustrations and diagrams. List of Appendices : Individual listing by title of each appendix. Main Body of the text : see below. Bibliography : Listing, using the harvard method, of all sources used in the course of the dissertation. Presentation : The dissertation must be typed using double spacing and ten or twelve point printing. . Pages should be numbered at the bottom and margins.5 cm should be left at the top, bottom and both sides of the page. Binding : The dissertation may be soft bound but if hard bound (should be with navy blue cover and gold lettering). . It is the student's responsibility to organise binding and to ensure that binding takes place in advance of the submission date.
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The research project is intended to build on the taught modules of the student's ma award and matlab is underpinned by the research Methods in hrm module. . The dissertation is designed to demonstrate the synthesis of knowledge and skills developed throughout the award. . It is the largest piece of assessed work undertaken on the award, and is seen as the clearest expression of the student's ability to demonstrate what they have studied at Masters level. Successful completion of HR7155 Research Methods in hrm. The dissertation topic should be sufficiently well-focused to facilitate an in-depth study but broad enough to develop an informed overview of the topic area. . The required length of the dissertation is 12,000 (min) - 15,000 (max) words exclusive of title and contents page, figures, tables,"tions, appendices and bibliography. . The dissertation will be developed from the 3,000 word proposal submitted as part of the assessment in the research Methods in hrm module. .
Once the topic has been approved, the student will be allocated a supervisor with whom the student will work during the research and writing up stages prior to submission. Dissertation structur, e the structure of the dissertation may depend upon the nature of the research and there is no one correct structure. . However, the following must be included: cover Page : Institution's name; Award name; year of dissertation submission; Student's name; Dissertation title. Title page : Title of dissertation and author's name. Acknowledgements : Acknowledgements should be given to individuals who have provided substantive help with the research. Contents Page : Chapter headings and subheadings.
2-6, 1995 Haber,., toomre,., hill,., gough. Local Area analysis of High-Degree solar Oscillations: New Ring Fitting Procedures 4th soho workshop on Helioseismology, pacific Grove, california, apr. 2-6, 1995 Hill,. Tridimensional Distribution of Horizontal Velocity Flows Under the solar Surface doctoral dissertation, Instituto de Astrofísica de canarias. Tables Table 1: averages of velocities inferred by the fourier method and the ring method for the same sample power spectrum.
The velocities are given in m/s, the angle is in degrees measured westward from north. Method v_x v_y v angle fourier Ring Table 2: averages of velocities inferred by the fourier method for different regions on successive days. Heliocentric Date lon lat v angle 6/ / / /. Evolution of Complexity in real-World Domains. Next: Dissertation Committee, a dissertation presented to the faculty of the Graduate School of Arts and Sciences. Pablo funes, brandeis University, department of Computer Science, advisor: Jordan. Pollack (c) Copyright by pablo funes, 2001. The ma dissertation is a triple-weighted module and is designed to provide an opportunity for students to undertake a substantial piece of research in their subject field. .
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It should be remembered that these results are preliminary. More careful calibration is required, we need to investigate sources of systematic errors, and we also need to verify the appropriate tracking rates to use in mapping. The most glaring deficiency in the present estimates, however, and one that commands urgent attention, is the lack of any inversion. The results presented are merely based on averages of frequency shifts over a fairly large set of modes. There are cases where there is quite large uncertainty in the velocity direction (based on the standard deviation of the contributing modes) even though the average velocities are quite high. These cases in particular are suggestive of the possibility of shear flows with depth. S., sá,., duvall,., essays haber,., toomre,., hill,. Plane-wave analysis of Solar Acoustic-Gravity waves: a (Slightly) New Approach 4th soho workshop on Helioseismology, pacific Grove, california, apr.
It can be seen that there is often good agreement between the velocities of adjacent regions and between the velocities of the same region on successive days, but that there are sometimes significant discontinuities in these patterns. Also, large uncertainies in direction are often, but not always, correlated with small absolute velocities. The comparatively large absolute value of the velocities we infer is a matter of some concern, as it is unusual to have consistent surface flows of this magnitude. However, it should be remembered that the flows are averaged in depth, with significant weighting from regions well below the photosphere. Furthermore, the values we find are similar in amplitude to those that have been found independently with Ring-diagram analysis of comparable data ( Hill, 1988 ; Patrón, 1994 ). The consistency of the velocities in both time and space with occasional discontinuities is what would be expected if we are detecting large-scale organized, slowly-evolving flow fields, such as giant cells. It is important to extend these measurements to observations covering a large fraction of a solar rotation in order to determine that they are not related to systematic errors having to do with either disc location or contamination of the signal by active regions. It would also be useful to compare estimates for overlapping regions of different sizes.
at the end of the day, and at latitude -25. The region has an extent of about 30 degrees (256*256 pixels with a scale at the map center.12 heliographic degree/pixel). In Paper 1 we used the differences between this and other deliberately mistracked fields to demonstrate the linearity of both methods and establish the agreement of the constant of proportionality relating the determined frequency variations to velocities. The present result seems to establish that whatever constant offset may exist between the real and the inferred velocity at least does not differ in the two techniques. This is important to demonstrate, since the typical average velocities inferred are several hundred meters per second relative to the supposedly stationary photosphere. Using the fourier technique we have explored multiple regions on the solar disc concurrently and extended the analysis over the full 4 days' of data. These data are presented in Table. Typically the averaged velocities are in the 50-200 m/s range, with statistical uncertainties of 30-60 m/s, so the results are statistically significant.
Some very preliminary estimates of velocities in the region sampled are presented here, and compared with other results obtained with similar data. The ca-k filtergrams are taken at a cadence of one per minute, with a spatial sampling of 2 arcsec per pixel, so that the entire solar disc is contained within a pixel frame. We have analyzed data from the four days Jun 22-25, 1993. On each of these days there were approximately eleven hours of data, with very few gaps. For each day we have analyzed 512 minutes of data centered on local noon. Data for the first day were available with corrections for scattered light, but our results do not seem to be particularly sensitive to this correction. The data were mapped and power spectra determined using the techniques described in Paper 1, and the acoustic-mode frequency shifts corresponding to the field motions estimated using both the techniques described in that paper and in, haber. The average velocities were estimated by averaging together, in the case of the fourier technique, values from 28 cylindrical cuts along a single surface ( n 2) at values of k separated by the spatial Nyquist frequency. With the ring diagram technique, rings corresponding to the same surface from 28 frequency-plane cuts were used, at values of w separated by the temporal Nyquist frequency.
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Preliminary Plane wave results, richard. Sá, center for Space Science astrophysics, Stanford Univerity, deborah Haber. Joint Institute for Laboratory Astrophysics, University of Colorado, frank hill, national Solar Observatory, national Optical Astronomy Observatories, table of contents. Abstract, using the techniques described in, bogart., 1995 (Paper i we have analyzed the p-mode spectra in four consecutive days of ca-k filtergram data from the high-l Helioseismometer at Kitt peak. Although the mode frequencies have not been inverted, the amplitude and phase of the frequency shifts analyzed this way demonstrate consistent behaviour that appears to be tied to solar features. These results are compared with results from a separate plane-wave (ring-diagram) analysis of the same data. In the process of developing plane-wave mode analysis techniques for application to data from the solar Oscillations Investigation (SOI). Soho, we have begun mba to analyze data from a four-day series of ca-k filtergrams made with the high-l Helioseismometer at the national.