Nowadays, Field-Programmable Gate Arrays (FP-GAs) are increasingly used in critical applications. In these scenarios fault tolerance techniques are needed to increase system dependability and lifetime. This paper proposes a novel methodology to achieve autonomous fault tolerance in FPGA-based systems affected by permanent faults. A design flow is defined to help designers to build a system with increased lifetime and availability. The methodology exploits Dynamic Partial Reconfiguration (DPR) to relocate at run-time faulty modules implemented onto the FPGA. A partitioning method is also presented to provide a solution which maximizes the number of permanent faults the system can tolerate. Experimental results highlight the negligible performance degradation introduced by applying the proposed methodology, and the improvements with respect to state-of-the-art solutions.

Nowadays, Video-Based Navigation (VBN) is increasingly used in space-applications. The future space-missions will include this approach during the Entry, Descent and Landing (EDL) phase, in order to increase the landing point precision. This paper presents FEMIP: a high performance FPGA-based features extractor and matcher tuned for space applications. It outperforms the current state-of-the-art, ensuring a higher throughput and a lower hardware resources usage.

The presence of noise in images can significantly impact the performances of digital image processing and computer vision algorithms. Thus, it should be removed to improve the robustness of the entire processing flow. The noise estimation in an image is also a key factor, since, to be more effective, algorithms and denoising filters should be tuned to the actual level of noise. Moreover, the complexity of these algorithms brings a new challenge in real-time image processing applications, requiring high computing capacity. In this context, hardware acceleration is crucial, and Field Programmable Gate Arrays (FPGAs) best fit the growing demand of computational capabilities. This paper presents an Adaptive Image Denoising IP-core (AIDI) for realtime applications. The core first estimates the level of noise in the input image, then applies an adaptive Gaussian smoothing filter to remove the estimated noise. The filtering parameters are computed on-the-fly, adapting them to the level of noise in the image, and pixel by pixel, to preserve image information (e.g., edges or corners). The FPGA-based architecture is presented, highlighting its improvements w.r.t. a standard static filtering approach.

The 2-D Convolution is an algorithm widely used in image and video processing. Although its computation is simple, its implementation requires a high computational power and an intensive use of memory. Field Programmable Gate Arrays (FPGA) architectures were proposed to accelerate calculations of 2-D Convolution and the use of buffers implemented on FPGAs are used to avoid direct memory access. In this paper we present an implementation of the 2-D Convolution algorithm on a FPGA architecture designed to support this operation in space applications. This proposed solution dramatically decreases the area needed keeping good performance, making it appropriate for embedded systems in critical space applications.

Nowadays, Graphical Processing Units (GPUs) have become increasingly popular due to their high computational power and low prices. This makes them particularly suitable for high-performance computing applications, like data elaboration and financial computation. In these fields, high efficient test methodologies are mandatory. One of the most effective ways to detect and localize hardware faults in GPUs is a Software-Based-Self-Test methodology (SBST). In this paper a fully comprehensive SBST and fault localization methodology for GPUs is presented. This novel approach exploits different custom test strategies for each component inside the GPU architecture. Such strategies guarantee both permanent fault detection and accurate fault localization.