Effect of polydispersity on the transport and sound absorbing properties of three-dimensional random fibrous structures

Sophisticated numerical approaches can predict the properties of composite nonwovens. However, for polydisperse random fibrous media, we need to identify microstructural descriptors for accurate predictions. We manufactured polydisperse composite felts with different fibrous structures and characterized them using scanning electron microscope images. The images showed a wide distribution of fiber diameters and a decreasing standard deviation of the azimuthal angle of fibers with increasing compression rate. Current models could not capture the evolution of their transport properties with compression rate. Therefore, we developed a fiber network model for the transport processes of transversely isotropic random fibrous media. The model relates the main visco-thermal dissipation mechanisms to the largest channels within the fluid phase, while the smallest channels lead the inertial behaviors. We estimated the viscous and thermal permeabilities from a representative elementary volume (REV) with a volume weighted average diameter, and the viscous and thermal characteristic lengths from a REV with inverse volume weighted average diameter. A unified empirical model was proposed. The model predictions agree with the experimental results.Comment: 29 pages, 19 figure

Once is an Instance, Twice is a Hobby: Multiple Optical and Near-Infrared Changing-Look Events in NGC 5273

NGC 5273 is a known optical and X-ray variable AGN. We analyze new and archival IR, optical, UV, and X-ray data in order to characterize its long-term variability from 2000 to 2022. At least one changing-look event occurred between 2011 and 2014, when the AGN changed from a Type 1.8/1.9 Seyfert to a Type 1. It then faded considerably at all wavelengths, followed by a dramatic but slow increase in UV/optical brightness between 2021 and 2022. We propose that NGC 5273 underwent multiple changing-look events between 2000 and 2022 -- starting as a Type 1.8/1.9, NGC 5273 changes-look to a Type 1 only temporarily in 2002 and again in 2014, reverting back to a Type 1.8/1.9 by 2005 and 2017, respectively. In 2022, it is again a Type 1 Seyfert with optical and NIR broad emission lines. We characterize the changing-look events and their connection to the dynamic accretion and radiative processes in NGC 5273.Comment: 18 pages, 13 figures, 4 tables, submitting to MNRA

Software effort prediction using regression rule extraction from neural networks

10.1109/ICTAI.2010.82Proceedings - International Conference on Tools with Artificial Intelligence, ICTAI245-52PCTI

Experimental determination of the macroscopic fatigue properties of metal hollow sphere structures

International audienc

Vertebral fractures after denosumab cessation.

status: publishe