Proportion of Glaucoma among Voluntary People Coming for Glaucoma Screening Program at Jimma University Department of Ophthalmology, Jimma, Ethiopia

BACKGROUND: Glaucoma is the second leading cause of blindness worldwide. Glaucoma screening has been controversial, and much of the controversy has centered on the value of mass or community screening.METHODS: The aim of this study was to determine the proportion of glaucoma among volunteer adults who were screened in Jimma University Department of Ophthalmology. A cross-sectional study was conducted among 459 volunteer residents of Jimma town and surrounding areas. The study subjects were aged 40 years and above, who came for community screening program after media announcement during the four consecutive weekends of November 2014. Comprehensive eye examination was done including best corrected visual acuity, intra-ocular pressure measurement, stereoscopic optic nerve evaluation, angle structure evaluation and visual field testing. Three diagnostic criteria for glaucoma were employed for all cases.RESULTS: Of all adults who came for screening, 47(10.24%) were diagnosed to have glaucoma, 59(12.85%) were glaucoma suspects, and 8(1.74%) had ocular hypertension. The proportion of glaucoma increased with increasing age, (P value= 0.001 (99%CI)). Primary open angle glaucoma was the most common form (42.55%) of all new cases while 4.4% of all screened adults were followed by normal tension glaucoma (29.79%), pseudoexfoliative glaucoma (19.15%), and primary angle closure glaucoma (6.38%) Around 5.7% of all glaucoma cases were found to be blind.CONCLUSION: The proportion of glaucoma in this community screening program in Southwest Ethiopia was 10.24% with primary open angle glaucoma being the commonest subtype. Glaucoma community screening should be promoted for early diagnosis and intervention to prevent irreversible blindness

Aplikasi Programmable Logic Controller (PLC) Pada Sistem Kontrol Proses Pengelasan Inner dan Outer Tabung Iradiasi

Pada proses pengelasan inner dan outer tabung iradiasi, diperlukan sumber daya manusia yang handal sehingga hasil pengelasan memenuhi persyaratan yang ditetapkan untuk dapat diiradiasi di reaktor nuklir. Karena adanya keterbatasan sumber daya manusia yang mampu melakukan pengelasan tabung iradiasi secara sempurna, maka dibuat sistem kontrol proses pengelasan inner dan outer tabung iradiasi. Dengan sistem kontrol tersebut maka pengelasan tabung iradiasi dapat dilakukan secara otomatis. Metoda yang digunakan yaitu dengan menggunakan Programmable Logic Controller (PLC) yang difungsikan untuk mengatur proses pengelasan secara otomatis melalui program yang ditanamkan di dalamnya. Hasil yang diperoleh berupa unit kontrol yang telah diuji secara simulasi, kemudian dirangkai pada unit mesin las, dan selanjutnya dilakukan uji pengelasan terhadap tabung iradiasi. Pada hasil pengelasan dilakukan juga uji kebocoran dengan metode bubble test. Sistem kontrol dapat dinyatakan berfungsi dengan baik, karena semua langkah dalam proses pengelasan sudah terpenuhi. Hasil pengelasan yang kurang maksimal lebih besar diakibatkan oleh kondisi tabung iradiasi yang kurang sempurna seperti bentuk kurang simetris dan permukaan tidak bersih, serta kondisi bagian mekanik pada pemutar tabung iradiasi yang tidak presisi

NASA Planetary Mission Concept Study: Assessing: Dwarf Planet Ceres' past and Present Habitability Potential

The Dawn mission revolutionized our understanding of Ceres during the same decade that has also witnessed the rise of ocean worlds as a research and exploration focus. We will report progress on the Planetary Mission Concept Study (PMCS) on the future exploration of Ceres under the New Frontiers or Flagship program that was selected for NASA funding in October 2019. At the time this writing, the study was just kicked off, hence this abstract reports the study plan as presented in the proposal

Summary of the Results from the Lunar Orbiter Laser Altimeter after Seven Years in Lunar Orbit

In June 2009 the Lunar Reconnaissance Orbiter (LRO) spacecraft was launched to the Moon. The payload consists of 7 science instruments selected to characterize sites for future robotic and human missions. Among them, the Lunar Orbiter Laser Altimeter (LOLA) was designed to obtain altimetry, surface roughness, and reflectance measurements. The primary phase of lunar exploration lasted one year, following a 3-month commissioning phase. On completion of its exploration objectives, the LRO mission transitioned to a science mission. After 7 years in lunar orbit, the LOLA instrument continues to map the lunar surface. The LOLA dataset is one of the foundational datasets acquired by the various LRO instruments. LOLA provided a high-accuracy global geodetic reference frame to which past, present and future lunar observations can be referenced. It also obtained high-resolution and accurate global topography that were used to determine regions in permanent shadow at the lunar poles. LOLA further contributed to the study of polar volatiles through its unique measurement of surface brightness at zero phase, which revealed anomalies in several polar craters that may indicate the presence of water ice. In this paper, we describe the many LOLA accomplishments to date and its contribution to lunar and planetary science

Science Opportunities offered by Mercury's Ice-Bearing Polar Deposits

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The fractured Moon: Production and saturation of porosity in the lunar highlands from impact cratering

We have analyzed the Bouguer anomaly (BA) of ~1200 complex craters in the lunar highlands from Gravity Recovery and Interior Laboratory observations. The BA of these craters is generally negative, though positive BA values are observed, particularly for smaller craters. Crater BA values scale inversely with crater diameter, quantifying how larger impacts produce more extensive fracturing and dilatant bulking. The Bouguer anomaly of craters larger than urn:x-wiley:00948276:media:grl53324:grl53324-math-0001 km in diameter is independent of crater size, indicating that there is a limiting depth to impact‐generated porosity, presumably from pore collapse associated with either overburden pressure or viscous flow. Impact‐generated porosity of the bulk lunar crust is likely in a state of equilibrium for craters smaller than ~30 km in diameter, consistent with an ~8 km thick lunar megaregolith, whereas the gravity signature of larger craters is still preserved and provides new insight into the cratering record of even the oldest lunar surfaces