Nessy 7.0: entorno de inyección de fallos para Artix-7

El hardware reconfigurable es una tecnología emergente en aplicaciones espaciales.Debido a las características de este hardware, pues su configuración lógica queda almacenada en memoria RAM estática, es susceptible de diversos errores que pueden ocurrir con mayor frecuencia cuando es expuesta a entornos de mayor radiación, como en misiones de exploración espacial. Entre estos se encuentran los llamados SEU o Single Event Upset, y suelen ser generados por partículas cósmicas, pues pueden tener la capacidad de descargar un transistor y de este modo alterar un valor lógico en memoria, y por tanto la configuración lógica del circuito. Por ello que surge la necesidad de desarrollar técnicas que permitan estudiar las vulnerabilidades de diversos circuitos, de forma económica y rápida, además de técnicas de protección de los mismos. En este proyecto nos centraremos en desarrollar una herramienta con este propósito, Nessy 7.0. La plataforma nos permitirá emular, detectar y analizar posibles errores causados por la radiación en los sistemas digitales. Para ello utilizaremos como dispositivo controlador, una Raspberry Pi 3, que contendrá la herramienta principal, y controlará y se comunicará con la FPGA que implementará el diseño a testear, en este caso una placa Nexys 4 DDR con una FPGA Artix-7. Finalmente evaluaremos un par de circuitos con la plataforma.

An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302

Aims. We report results of an X-ray study of the supernova remnant (SNR) G344.7-0.1 and the point-like X-ray source located at the geometrical center of the SNR radio structure. Methods. The morphology and spectral properties of the remnant and the central X-ray point-like source were studied using data from the XMM-Newton and Chandra satellites. Archival radio data and infrared Spitzer observations at 8 and 24 mu m were used to compare and study its multi-band properties at different wavelengths. Results. The XMM-Newton and Chandra observations reveal that the overall X-ray emission of G344.7-0.1 is extended and correlates very well with regions of bright radio and infrared emission. The X-ray spectrum is dominated by prominent atomic emission lines. These characteristics suggest that the X-ray emission originated in a thin thermal plasma, whose radiation is represented well by a plane-parallel shock plasma model (PSHOCK). Our study favors the scenario in which G344.7-0.1 is a 6 x 10^3 year old SNR expanding in a medium with a high density gradient and is most likely encountering a molecular cloud on the western side. In addition, we report the discovery of a soft point-like X-ray source located at the geometrical center of the radio SNR structure. The object presents some characteristics of the so-called compact central objects (CCO). However, its neutral hydrogen absorption column (N_H) is inconsistent with that of the SNR. Coincident with the position of the source, we found infrared and optical objects with typical early-K star characteristics. The X-ray source may be a foreground star or the CCO associated with the SNR. If this latter possibility were confirmed, the point-like source would be the farthest CCO detected so far and the eighth member of the new population of isolated and weakly magnetized neutron stars.

Anomalous resistivity at the structural phase transition of polycrystalline SnTe

An excess resistivity has been observed in thin film polycrystalline samples of SnTe with low carrier concentration and is attributed to the additional scattering due to the phonon softening associated with the structural phase transition.