1,725,302 research outputs found
Analisa Penyebab Kerusakan Generator Seri 3516 Metode FTA
The Caterpillar 3516 series generator engine is an acronym for a generator set, which is a machine or device consisting of a power generator (generator) with a propulsion engine arranged into a single unit to produce electricity with a certain unit. 3516 series generator engine components located or attached to the top of the cylinder block and fastened by special bolts. Leakage or damage to the cylinder head (cylinder head) will result in compression leaks and the engine cannot operate. Fault Tree Analysis is a technique used to identify risks that contribute to failure. Damage that occurs in the cylinder head components of the generator engine series 3516 s/n.25z04978. Processing Results There are 4 causes of damage that often occurs in the 3516 series generator engine, namely Human Factors, Machine Factors and Component Factors. Injector Damage, Valve Damage and Insert Damage and human factors.Mesin generator caterpillar seri 3516 adalah akronim dari generator set,yaitu suatu mesin atau perangkat yang terdiri dari pembangkit listrik (Generator) dengan mesin penggerak yang disusun menjadi satu kesatuan untuk menghasilkan tenaga listrik dengan satu kesatuan tertentu. Komponen mesin generator seri 3516 yang terletak atau menempel diatas silinder block dan di ikat oleh baut kusus. Kebocoran atau kerusakan dari kepala silinder (cylinder head) ini akan mengakibatkan kebocoran kompresi dan mesin tidak bisa beroperasi. Fault Tree Analysis merupakan suatu teknik yang digunakan untuk mengidentifikasi resiko yang berperan terhadap terjadinya kegagalan. Kerusakan yang terjadi pada komponen kepala silinder (cylinder head) mesin generator seri 3516 s/n.25z04978. Hasil Pengolahan terdapat 4 penyebab kerusakan yang sering terjadi pada mesin generator seri 3516 yaitu Faktor Manusia, Faktor Mesin dan faktor Komponen. Kerusakan Injektor, Kerusakan Valve dan Kerusakan Insert dan faktor manusia
Whipple, Thelma Louise, b. 1912 (SC 3516)
Finding aid only for Manuscripts Small Collection 3516. School memory book of Thelma Louise Whipple, Hickman, Kentucky, containing autographs and names of teachers, classmates and friends
Block Card 3516 Havenhurst Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 3516 Havenhurst Avenue (Toledo, Ohio) | Dwelling | Glen Arbor (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Block Card 3516 Torrance Drive
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: dwelling | 3516 Torrance Drive (Toledo, Ohio) | Tudor Cottage style | Almeda Heights (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio
Block Card 3516 Golfgate Drive
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Garrison Colonial Style | 3516 Golfgate Drive (Toledo, Ohio) | duplexes | Byrne Way Subdivision (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Block Card 3516 Burton Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: dwelling | 3516 Burton Avenue (Toledo, Ohio) | Folk House Style | Almeda Heights Second Addition (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio
Block Card 3516 Muirfield Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | 3516 Muirfield Avenue (Toledo, Ohio) | Dwelling | Glen Arbor (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Tracing a Disk Wind in NGC 3516
X-ray spectra of AGN often contain signatures indicative of absorption in multiple layers of gas whose ionization-state and covering fraction may vary with time. It has been unclear to date how much of the observed X-ray spectral and timing behavior in AGN can be attributed to variations in absorption, versus variations in the strengths of emission or reflection components. Diagnostics of the inner regions of AGN cannot be reliably performed until the origin of observed effects is understood. We investigate the role of the X-ray absorbers in the Seyfert 1 galaxy NGC 3516. Time-averaged and flux-selected spectroscopy is used to examine the behavior of NGC 3516 observed in Chandra HETG and XMM data from Oct 2006. New H-like and He-like emission and absorption features discovered in the Fe K regime reveal a previously unknown zone of circumnuclear gas in NGC 3516 with log xi ~ 4.3 and column density 1E23 cm^-2. A lower-ionization layer with log xi ~2 and of similar column density is confirmed from previous observations, this layer has a covering fraction around 50%, and changes in covering provide a simple explanation of a deep dip in the light curve that we interpret as an eclipse of the continuum due to passage of a cloud across the sight line within half a day. These inner zones of absorbing gas are detected to have outflow velocities in the range 1000-2000 km/s, this, and constraints on radial location are consistent with an origin as part of a disk wind in NGC 3516
X-ray Characteristics of NGC 3516: A View through the Complex Absorber
We consider new Suzaku data for NGC 3516 taken during 2009, along with other recent X-ray observations of the source. The cumulative characteristics of NGC 3516 cannot be explained without invoking changes in the line-of-sight absorption. Contrary to many other well-studied Seyfert galaxies, NGC 3516 does not show a positive lag of hard X-ray photons relative to soft photons over the timescales sampled. In the context of reverberation models for the X-ray lags, the lack of such a signal in NGC 3516 is consistent with flux variations being dominated by absorption changes. The lack of any reverberation signal in such a highly variable source disfavors intrinsic continuum variability in this case. Instead, the colorless flux variations observed at high flux states for NGC 3516 are suggested to be a consequence of Compton-thick clumps of gas crossing the line-of-sight
Block Card 3516 Rushland Avenue
This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Garrison colonial | Dwelling | 3516 Rushland Avenue (Toledo, Ohio) | Forest View Addition (Toledo, Ohio) | Deveaux Area (Toledo, Ohio) | West Toledo (Toledo, Ohio
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