Computational Electromagnetics: A Miscellany

The paper presents a miscellany of unorthodox and, in some cases, paradoxical or controversial items related to computational and applied electromagnetics. The topics include a definition of the magnetic source field via a line integral, losses in electric power transmission vs. losses in photonics, homogenization of periodic electromagnetic structures, spurious modes, models of plasmonic media, and more. It is hoped that this assortment of subjects will be of interest to a broad audience of scientists and engineers.

Visualization of magnetic field corresponding to acoustic signal and estimation of magnetic source based on symmetry of magnetic field distribution

A magnetic field corresponding to an acoustic signal is generated from an antenna, and by using a coil, can be again converted to an acoustic signal. It is possible to estimate where the invisible antenna is with the distribution of the received signal. The estimation is applied to a maintenance of a gas pipe on the situation that the distance from the entrance to a maintenance area is known, but piping route isn't. It is possible to identify maintenance areas of a gas pipe by inserting the antenna to it. The estimation has been done by listening to the received signal manually. However, it is difficult for people to identify accurate point because the difference in the volume for each places is subtle. To solve this problem, we visualized the distribution of the received signal, and estimated the magnetic field with only the acoustic signal. Then, we proposed a method to calculate where the invisible antenna is automatically by using symmetry of the distribution of the received signal.

Effect of Spatially Varying Magnetic Field on the Cooling of an Electronic Component by Natural Convection With Magnetic Nanofluids

Natural convection cooling of an electronic component in an electronic device using water-based Fe3O4 magnetic nanofluids is studied under the presence of the magnetic field. The heated vertical electronic component in an enclosure type electronic device with a magnetic field source is used as a model for the study. Different samples of Fe3O4-water nanofluid are prepared using different surfactants and the stability of those samples are estimated using visualization and zeta potential technique. Thermal properties of the stable sample of magnetic nanofluid are precisely measured. The experimentally measured properties are used for further theoretical study. The natural convection is characterized in terms of the relative position of the magnetic source and the electronic component, the strength of the magnetic field, and the magnetization of the nanofluids. Nine different combinations of the position of the magnetic source and the electronic component have been compared with the case in which there is an absence of the magnetic field. The dimensionless number used in this investigation are Rayleigh number (103 ≤ Ra ≤ 106), magnetic numbers (Mn = 100, 500, and 1000), and Hartmann Number (0 ≤ Ha ≤ 100). The position of the magnetic source with respect to the electronic component significantly affects the rate of heat transfer. The effect is more pronounced when the magnetic source is placed below any of the two vertical walls of the enclosure. The fluid flow is observed distorted near the magnetic source when the Ha is increased. The increment in the magnetic number strengthens the flow, which leads to the enhanced heat transfer rate.

The Use of Euler Deconvolution Technique in the Estimation of Depth to Magnetic Source Bodies around the Schist Belt Parts of Kano State, Nigeria

Depth estimation of magnetic source bodies in parts of the Schist Belt of Kano, using Euler Deconvolution is presented in this paper. Detail ground magnetic survey was carried out using SCINTREX proton precession magnetometer to produce the Total Magnetic Intensity (TMI) map and consequently the residual map. The TMI ranges from 34,261 nT to 34,365 nT, while the residual field ranges from -160 nT to 115 nT. The depth estimate for contacts ranges from 6.5 m to 39.8 m, while that of dyke ranges from 8.9 m to 51.3 m. The depth estimation presented in this work is compared with the results of aeromagnetic study carried out in the same area and found to agree fairly well. Further, this also ensures the validity of aeromagnetic investigation in such applications. Keywords: Contacts, Dykes, Euler Deconvolution, Schist Belt. PACS: 91.25.F and 91.25.Rt.