Source In Absence Research Articles

Emergency Microscope Light Modification by External Source in Absence of Power Supply

Introduction: Microscope is an instrument for visualizing fine detail of an object so that observer can observe the object being examined in detail. The object of examination vary from cells (normal or pathologic), microorganism (such as parasite and bacterium), and even non biological part. There are several types of microscope, one of the oldest forms and still used today is the light microscope. A light microscope relied on continuous light source to operate. The most common source for today's microscopes is an incandescent tungsten-halogen bulb, which is solely electric dependent, positioned in a reflective housing that projects light through the collector lens and into the sub-stage condenser. Current situations sometimes require readiness for conducting microscopic examination anytime, anywhere. Unfortunately, problem occur if the electricity goes out, most people will not be able to continue their microscopic observations. This problem raises the question of what if in an emergency it is necessary to carry out a microscopic examination but unfortunately there is no power source. Below we propose emergency modification efforts so that the microscope can still be used even in conditions without a power source.
 Aims: to modify an electric light microscope in such a way that it can continue to be used in the absence of an electrical power source using external source of light.
 Discussion: Adding an external source of light is a brilliant approach in order to make the electric dependent light microscope still useable in emergency condition.
 Conclusion: it is possible to modify an electric light microscope in the condition of no electric source available and make it operable.

Neumann fractional [formula omitted]-Laplacian: Eigenvalues and existence results

We develop some properties of the p-Neumann derivative for the fractional p-Laplacian in bounded domains with general p>1. In particular, we prove the existence of a diverging sequence of eigenvalues and we introduce the evolution problem associated to such operators, studying the basic properties of solutions. Finally, we study a nonlinear problem with source in absence of the Ambrosetti–Rabinowitz condition.

Acoustic source localization in anisotropic plates with “Z” shaped sensor clusters

A new sensor cluster orientation is proposed to localize an acoustic source in a plate from the time difference of arrival (TDOA) with the help of only four to eight sensors. This technique requires neither a priori knowledge of the plate material properties nor a dense array of sensors to localize the acoustic source in isotropic as well as anisotropic plates. It is achieved by placing four sensors in a cluster in the shape of letter “Z” over a small region of the plate and a second Z-shaped cluster at another location of the plate. Experimental results show that it is possible to accurately localize the acoustic source with this new configuration. It reduces the number of sensors required for acoustic source localization in an anisotropic plate. Although one cluster in principle is capable of localizing the acoustic source in absence of any experimental error for accurate source localization in presence of experimental error two such Z-shaped clusters are needed. In the currently available technique three L-shaped clusters having a total of 9 sensors are needed to achieve the same level of confidence in the acoustic source localization. Thus, the proposed new technique reduces the number of sensors by 1 (from 9 to 8) for confidently and accurately predicting the acoustic source.

Mesoporous hybrid zirconium oxophenylphosphate synthesized in absence of any structure directing agent

A new organic–inorganic hybrid mesoporous zirconium oxophenylphosphate (ZPP-1) has been synthesized hydrothermally at 443 K by using phenylphosphonic acid (PPA) as phosphorus source in absence of any structure directing agent. Powder XRD, TEM, FE SEM, N 2 sorption, CHN and ICP-AES chemical analyses, 13C CP/MAS and 31P MAS NMR, UV–visible and FT IR spectroscopic tools and thermal analysis were employed to characterize this novel material. XRD, N 2 sorption and TEM image analysis suggested the existence of multi-lamellar structure of the pore wall with large micropores and mesopores having peak maximums of ca. 1.5 and 5.0–6.0 nm, respectively in this ZPP-1 material. Interestingly, this hybrid material showed very high thermal stability together with retention of nanostructure and phenyl group when heated upto 723 K. ZPP-1 showed fairly high H 2 adsorption capacity under atmospheric pressure at 77 K. Possible templating role played by the framework phenyl groups has been discussed.

Discovery of a Transient Magnetar: XTE J1810-197

We report the discovery of a new X-ray pulsar, XTE J1810-197, that was serendipitously discovered on 2003 July 15 by the Rossi X-Ray Timing Explorer (RXTE) while observing the soft gamma repeater SGR 1806-20. The pulsar has a 5.54 s spin period, a soft X-ray spectrum (with a photon index of approx. = 4). and is detectable in earlier RXTE observations back to 2003 January but not before. These show that a transient outburst began between 2002 November 17 and 2003 January 23 and that the source's persistent X-ray flux has been declining since then. The pulsar exhibits a high spin-down rate P approx.= l0(exp -11) s/s with no evidence of Doppler shifts due to a binary companion. The rapid spin-down rate and slow spin period imply a supercritical characteristic magnetic field B approx. = 3 x l0(exp 14) G and a young age tau less than or = 7600 yr. Follow-up Chandra observations provided an accurate position of the source. Within its error radius, the 1.5 m Russian-Turkish Optical Telescope found a limiting magnitude R(sub c) = 21.5. All such properties are strikingly similar to those of anomalous X-ray pulsars ad soft gamma repeaters, providing strong evidence that the source is a new magnetar. However, archival ASCA and ROSAT observations found the source nearly 2 orders of magnitude fainter. This transient behavior and the observed long-term flux variability of the source in absence of an observed SGR-like burst activity make it the first confirmed transient magnetar and suggest that other neutron stars that share the properties of XTE 51810- 197 during its inactive phase may be unidentified transient magnetars awaiting detection via a similar activity. This implies a larger population of magnetars than previously surmised and a possible evolutionary connection between magnetars and other neutron star families. Subject headings: pulsars: general -pulsars: individual (XTE 51810- 197) - stars: magnetic fields -