Use of new generation geospatial data and technology for low cost drought monitoring and SDG reporting solution : a thesis presented in partial fulfillment of the requirement for the degree of Master of Science in Computer Science at Massey University, Manawatū, New Zealand

Food security is dependent on ecosystems including forests, lakes and wetlands, which in turn depend on water availability and quality. The importance of water availability and monitoring drought has been highlighted in the Sustainable Development Goals (SDGs) within the 2030 agenda under indicator 15.3. In this context the UN member countries, which agreed to the SDGs, have an obligation to report their information to the UN. The objective of this research is to develop a methodology to monitor drought and help countries to report their ndings to UN in a cost-e ective manner. The Standard Precipitation Index (SPI) is a drought indicator which requires longterm precipitation data collected from weather stations as per World Meteorological Organization recommendation. However, weather stations cannot monitor large areas and many developing countries currently struggling with drought do not have access to a large number of weather-stations due to lack of funds and expertise. Therefore, alternative methodologies should be adopted to monitor SPI. In this research SPI values were calculated from available weather stations in Iran and New Zealand. By using Google Earth Engine (GEE), Sentinel-1 and Sentinel- 2 imagery and other complementary data to estimate SPI values. Two genetic algorithms were created, one which constructed additional features using indices calculated from Sentinel-2 imagery and the other data which was used for feature selection of the Sentinel-2 indices including the constructed features. Followed by the feature selection process two datasets were created which contained the Sentinel- 1 and Sentinel-2 data and other complementary information such as seasonal data and Shuttle Radar Topography Mission (SRTM) derived information. The Automated Machine Learning tool known as TPOT was used to create optimized machine learning pipelines using genetic programming. The resulting models yielded an average of 90 percent accuracy in 10-fold cross validation for the Sentinel- 1 dataset and an average of approximately 70 percent for the Sentinel-2 dataset. The nal model achieved a test accuracy of 80 percent in classifying short-term SPI (SPI- 1 and SPI-3) and an accuracy of 65 percent of SPI-6 by using the Sentinel-1 test dataset. However, the results generated by using Sentinel-2 dataset was lower than Sentinel-1 (45 percent for SPI-1 and 65 percent for SPI-6) with the exception of SPI-3 which had an accuracy of 85 percent. The research shows that it is possible to monitor short-term SPI adequately using cost free satellite imagery in particular Sentinel-1 imagery and machine learning. In addition, this methodology reduces the workload on statistical o ces of countries in reporting information to the SDG framework for SDG indicator 15.3. It emerged that Sentinel-1 imagery alone cannot be used to monitor SPI and therefore complementary data are required for the monitoring process. In addition the use of Sentinel-2 imagery did not result in accurate results for SPI-1 and SPI-6 but adequate results for SPI-3. Further research is required to investigate how the use of Sentinel-2 imagery with Sentinel-1 imagery impact the accuracy of the models

Things Fall Apart and Chinua Achebe’s Postcolonial Discourse

Chinua Achebe, the contemporary Nigerian novelist, is considered as one of the prominent figures in African anti-colonial literature. What makes his works specific is the way he approaches the issues of colonization of Africa in an objective manner and through an innovative language which aims at providing a pathology; a pathological reading meant to draw on the pre-colonial and colonial history without any presumptions so as to present the readers with possible alternative African discourses in future. His first novel Things Fall Apart can be taken as the best representative of such a penchant in Achebe. The present study seeks to approach Things Fall apart by reflecting on those discursive features which have provided the ground for constructing such a pathological reading and an alternative to the colonial discourse. To this end, some key terms introduced by Homi Bhabha and Mikhail Bakhtin such as ‘hybridity’, ‘otherness’ and ‘polyphony’, constitute the cornerstone of this study. Presumably, such an innovative reading of Achebe’s Things Fall Apart is to lead to a better understanding of his discourse and the efforts made by him to help the African readers figure out how to piece together what once fell apart; what they can rely on for building an independent future in the so-called postcolonial era

Anti fungal activity of alcoholic extract of Peganum harmala seeds

In our study, it was aimed to determine antifungal activity of Peganum harmala on medically important yeasts and molds in vitro. Fungal suspensions of Candida spp and aspergillus spp isolated from the clinical specimens were treated with serial dilutions of P. harmala alcoholic extract in Sabouraud Broth. The titers included: 1/20, 1/40, 1/80, 1/160, 1/320, 1/640, and incubated for 24 h at 30°C. Anti fungal activity of the extract was determined as MIC and MFC. For the determination of MFC, a small volume of above serial dilutions was cultured on SGA 4% medium. After 24 to 72 h of incubation at 30°C, the cultures were looked for fungal growth. The highest and lowest inhibitory effects of P. harmala extract were determined on C. glabrata (MIC: 0.312 mg/ml) and C. albicans (MIC: 1.25 mg/ml), respectively. The MFC for Candida species was differed from 0.62 to 2.5 mg/ml. The highest fungicidal effect was seen on C. glabrata and C. tropicalis (MFC: 0.62 and 0.125 mg/ml, respectively) and the lowest was for C. albicans (MFC: 2.5 mg/ml). The treatment of Aspergillus suspensions with Perganum extract showed a decreasing of growth and sporolation without definite inhibition. The alcoholic extract of P. harmala showed a fungicidal activity on opportunistic yeasts, Candida spp, and a decreasing sporolation for aspergillus most importamt species. © 2011 Academic Journals

ONE-TWO criteria: Improving the approach to electrocardiogram

The electrocardiogram (EKG) is one of the major Para-clinic exams for evaluating patients suspected to cardiac or non-cardiac disease which could be very informative especially when assessed by experienced clinicians. To improve and accelerate the approach to EKG interpretation, simple and accurate criteria are useful and save the physician's time especially in emergent situations. In this article, we introduce our criteria which determine whether the electrical axis of heart is normal or not and if abnormal, what kind of deviation it has. These criteria say that "if the mean QRS complex in leads I and II are positive, the axis will be accu-rately in the normal range (-30 to +90); unless, the axis is abnormal necessitating a more complex evaluation". These criteria could simplify the first step of the approach to EKG interpretation especially in emergent situations. They can also be proper substitute for current methods of heart axis determination in clinical practice and for educational goals. © 2010 Motaharsadat Hosseini et al

Medical Students’ View about the Effects of Practical Courses on Learning the General Theoretical Concepts of Basic Medical Sciences

Introduction: The basic medical sciences section requires 2.5 years in the medical education curriculum. Practical courses complement theoretical knowledge in this period to improve their appreciation. Despite spending lots of disbursement and time, this period’s efficacy is not clearly known. Methods: One hundred thirty-three General Practitioner (GP) students have been included in this descriptive cross-sectional study and were asked by questionnaire about the positive impact of practical courses on learning theoretical knowledge. Data were analyzed by descriptive statistics. Result: The agreement in “Practical Head and Neck Anatomy” was 40.91% ± 29.45, in “Practical Trunk Anatomy” was 63.62% ± 2.32 and in “Practical Anatomy of Extremities” was 56.16% ± 2.57. In “Practical Histology”, agreement was 69.50%±2.19; “Practical Biophysics” was 45.97%±2.25, “Practical Physiology” 61.75%±2.17; “Practical Biochemistry” 36.28%±2.42; “Practical Pathology” 59.80%±2.53; “Practical Immunology” 56.25%±26.40; “Practical Microbiology and Virology” 60.39%±2.27 and “Practical Mycology and Parasitology” 68.2%± 2.16.Conclusion: GP students in Tabriz University of Medical Sciences are not optimistic about the applicability of practical courses of basic medical sciences lessons

Interstellar absorptions towards the LMC: Small-scale density variations in Milky Way disc gas

Observations show that the ISM contains sub-structure on scales less than 1 pc, detected in the form of spatial and temporal variations in column densities or optical depth. Despite the number of detections, the nature and ubiquity of the small-scale structure in the ISM is not yet fully understood. We use UV absorption data mainly from FUSE and partly from STIS of six LMC stars (Sk-67{\deg}111, LH54-425, Sk-67{\deg}107, Sk-67{\deg}106, Sk-67{\deg}104, and Sk-67{\deg}101), all located within 5 arcmin of each other, and analyse the physical properties of the Galactic disc gas in front of the LMC on sub-pc scales. We analyse absorption lines of a number of ions within the UV spectral range. Most importantly, interstellar molecular hydrogen, neutral oxygen, and fine-structure levels of neutral carbon have been used in order to study changes in the density and the physical properties of the Galactic disc gas over small angular scales. While most species do not show any significant variation in their column densities, we find an enhancement of almost 2 dex for H_2 from Sk-67{\deg}111 to Sk-67{\deg}101, accompanied by only a small variation in the OI column density. Based on the formation-dissociation equilibrium, we trace these variations to the actual density variations in the molecular gas. On the smallest spatial scale of < 0.08 pc, between Sk-67{\deg}107 and LH54-425, we find a gas density variation of a factor of 1.8. The line of sight towards LH54-425 does not follow the relatively smooth change seen from Sk-67{\deg}101 to Sk-67{\deg}111, suggesting that sub-structure might exist on a smaller spatial scale than the linear extent of our sight-lines. Our observations suggest that the detected H_2 in these six lines of sight is not necessarily physically connected, but that we are sampling molecular cloudlets with pathlengths < 0.1-1.8 pc and possibly different densities.Comment: 17 pages, 8 figures. Accepted for publication in A&

Single Incision Laparoscopic Surgery: Review of Pros and Cons

Despite huge advances in minimally invasive surgeries, efforts still continue for finding less invasive methods of surgery. Patients desire less postoperative pain as well as better cosmetic outcomes. This may be achieved by decreasing the number of laparoscopic ports in which all the surgical maneuvers are performed through a single incision. However, surgeons should be also equipped to act well while avoiding adverse events of the new practicing approach. Along with increasing trends in performing of single incision laparoscopic surgery (SILS) in routine practice, the number of assessing the pros and cons of this new modality is also on the rise.&nbsp;Although it has been claimed that SILS is able to make the dream of invisible laparoscopy true for patients and surgeons, consecutive studies regarding postoperative outcomes questioned the benefits of the new evolved technique. Subsequent meta-analysis also revealed equal outcomes for SILS in comparison to the standard laparoscopy. Our review aimed to outline the pros and cons of SILS

Small-scale studies of the Milky Way disc and halo gas with absorption-line spectroscopy

Progressive studies in the last decades have shown that the interstellar medium (ISM) is more complex and dynamic than previously thought. The presence of the small-scale structures, structures on scales below 1 pc, has required a deeper understanding of the ISM and the physical processes involved in its evolution. Despite the number of detections, the nature of these small-scale structures is still poorly understood, and a systematic study on the subject is very difficult, as the sensitivity of absorption line spectroscopy is often required. The far-UV range of the spectrum in particular, provides a unique opportunity to study a number of present atoms and ions, and most importantly molecular hydrogen, which enable us to derive the physical properties of the gas. As the main results in this thesis, I present lines of sight of small angular separations in the direction of the Large Magellanic Cloud, where we find indication to small-scale structures in the Milky Way disc and halo gas. The molecular hydrogen structures, detected in this work as well as by others, are further compared with the low-column density halo structures detected in optical NaI absorption towards a number of quasars. The distribution of the detected molecular hydrogen as well as the NaI absorbers throughout the Galaxy further emphasises the role of turbulences and dynamical processes driven by Galactic fountains, which can produce high-density transient regions during the cooling and fragmentation phase