108 research outputs found
Estimation of the lightning performance of transmission lines with focus on mitigation of flashovers
The growth of transmission networks into remote areas due to renewable generation features new challenges with regard to the lightning protection of transmission systems. Up to now, standard transmission line designs kept outages resulting from lightning strokes to reasonable limits with minor impacts on the power grid stability. However, due to emerging problematic earthing conditions at towers, topographically exposed transmission towers and varying lightning activity, such as encountered at the 400 kV Beauly-Denny transmission line in Scotland, the assessment of the lightning performance of transmission lines in operation and in planning emerges as an important aspect in system planning and operations.
Therefore, a fresh approach is taken to the assessment of the lightning performance of transmission lines in planning and construction, as well as possible lightning performance improvements in more detail, based on the current UK/Scottish and Southern Energy 400 kV tower design and overhead line arrangements. The approach employs electromagnetic transient simulations where a novel mathematical description for positive, negative and negative subsequent lightning strokes, which are all scalable with stroke current, is applied. Furtermore, a novel tower foot earthing system model which combines soil ionisation and soil frequency-dependent effect is used. Novel lightning stroke distribution data for Scotland as well as novel cap-and-pin insulators with arcing horn flashover data derived from laboratory experiments are applied. For overhead lines, transmission towers, and flashover mitigation methods describing their physical behaviour in lightning stroke conditions state-of-the-art models are utilised. The investigation features a variety of tower and overhead line arrangements, soil conditions and earthing designs, as well as the evaluation of various measures to improve the performance. Results show that the lightning performance of a transmission line is less dependent on the tower earthing conditions, but more dependent on the degree of lightning activity and stroke amplitude distribution. The assessment of flashover mitigation methods shows that cost-effective and maintenance free solutions, such as underbuilt wires can effectively replace a costly improvement of the tower earthing system. However, in locations where challenging earthing conditions prevail, tower line arresters or counterpoise are the only options to maintain an effective lightning protection
Transformer Utilization in Medical Image Segmentation Networks
Owing to success in the data-rich domain of natural images, Transformers have
recently become popular in medical image segmentation. However, the pairing of
Transformers with convolutional blocks in varying architectural permutations
leaves their relative effectiveness to open interpretation. We introduce
Transformer Ablations that replace the Transformer blocks with plain linear
operators to quantify this effectiveness. With experiments on 8 models on 2
medical image segmentation tasks, we explore -- 1) the replaceable nature of
Transformer-learnt representations, 2) Transformer capacity alone cannot
prevent representational replaceability and works in tandem with effective
design, 3) The mere existence of explicit feature hierarchies in transformer
blocks is more beneficial than accompanying self-attention modules, 4) Major
spatial downsampling before Transformer modules should be used with caution.Comment: Accepted in NeurIPS 2022 workshop, Medical Imaging Meets NeurIPS
(MedNeurIPS
MedNeXt: Transformer-driven Scaling of ConvNets for Medical Image Segmentation
There has been exploding interest in embracing Transformer-based
architectures for medical image segmentation. However, the lack of large-scale
annotated medical datasets make achieving performances equivalent to those in
natural images challenging. Convolutional networks, in contrast, have higher
inductive biases and consequently, are easily trainable to high performance.
Recently, the ConvNeXt architecture attempted to modernize the standard ConvNet
by mirroring Transformer blocks. In this work, we improve upon this to design a
modernized and scalable convolutional architecture customized to challenges of
data-scarce medical settings. We introduce MedNeXt, a Transformer-inspired
large kernel segmentation network which introduces - 1) A fully ConvNeXt 3D
Encoder-Decoder Network for medical image segmentation, 2) Residual ConvNeXt up
and downsampling blocks to preserve semantic richness across scales, 3) A novel
technique to iteratively increase kernel sizes by upsampling small kernel
networks, to prevent performance saturation on limited medical data, 4)
Compound scaling at multiple levels (depth, width, kernel size) of MedNeXt.
This leads to state-of-the-art performance on 4 tasks on CT and MRI modalities
and varying dataset sizes, representing a modernized deep architecture for
medical image segmentation. Our code is made publicly available at:
https://github.com/MIC-DKFZ/MedNeXt.Comment: Accepted at MICCAI 202
RecycleNet: Latent Feature Recycling Leads to Iterative Decision Refinement
Despite the remarkable success of deep learning systems over the last decade,
a key difference still remains between neural network and human
decision-making: As humans, we cannot only form a decision on the spot, but
also ponder, revisiting an initial guess from different angles, distilling
relevant information, arriving at a better decision. Here, we propose
RecycleNet, a latent feature recycling method, instilling the pondering
capability for neural networks to refine initial decisions over a number of
recycling steps, where outputs are fed back into earlier network layers in an
iterative fashion. This approach makes minimal assumptions about the neural
network architecture and thus can be implemented in a wide variety of contexts.
Using medical image segmentation as the evaluation environment, we show that
latent feature recycling enables the network to iteratively refine initial
predictions even beyond the iterations seen during training, converging towards
an improved decision. We evaluate this across a variety of segmentation
benchmarks and show consistent improvements even compared with top-performing
segmentation methods. This allows trading increased computation time for
improved performance, which can be beneficial, especially for safety-critical
applications.Comment: Accepted at 2024 Winter Conference on Applications of Computer Vision
(WACV
Whole-body x-ray dark-field radiography of a human cadaver
Background!#!Grating-based x-ray dark-field and phase-contrast imaging allow extracting information about refraction and small-angle scatter, beyond conventional attenuation. A step towards clinical translation has recently been achieved, allowing further investigation on humans.!##!Methods!#!After the ethics committee approval, we scanned the full body of a human cadaver in anterior-posterior orientation. Six measurements were stitched together to form the whole-body image. All radiographs were taken at a three-grating large-object x-ray dark-field scanner, each lasting about 40 s. Signal intensities of different anatomical regions were assessed. The magnitude of visibility reduction caused by beam hardening instead of small-angle scatter was analysed using different phantom materials. Maximal effective dose was 0.3 mSv for the abdomen.!##!Results!#!Combined attenuation and dark-field radiography are technically possible throughout a whole human body. High signal levels were found in several bony structures, foreign materials, and the lung. Signal levels were 0.25 ± 0.13 (mean ± standard deviation) for the lungs, 0.08 ± 0.06 for the bones, 0.023 ± 0.019 for soft tissue, and 0.30 ± 0.02 for an antibiotic bead chain. We found that phantom materials, which do not produce small-angle scatter, can generate a strong visibility reduction signal.!##!Conclusion!#!We acquired a whole-body x-ray dark-field radiograph of a human body in few minutes with an effective dose in a clinical acceptable range. Our findings suggest that the observed visibility reduction in the bone and metal is dominated by beam hardening and that the true dark-field signal in the lung is therefore much higher than that of the bone
Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
We model the cosmological co-evolution of galaxies and their central
supermassive black holes (BHs) within a semi-analytical framework developed on
the outputs of the Millennium Simulation. This model, described in detail in
Croton et al. (2006) and De Lucia & Blaizot (2007), introduces a `radio mode'
feedback from Active Galactic Nuclei (AGN) at the centre of X-ray emitting
atmospheres in galaxy groups and clusters. Thanks to this mechanism, the model
can simultaneously explain: (i) the low observed mass drop-out rate in cooling
flows; (ii) the exponential cut-off in the bright end of the galaxy luminosity
function; and (iii) the bulge-dominated morphologies and old stellar ages of
the most massive galaxies in clusters. This paper is the first of a series in
which we investigate how well this model can also reproduce the physical
properties of BHs and AGN. Here we analyze the scaling relations, the
fundamental plane and the mass function of BHs, and compare them with the most
recent observational data. Moreover, we extend the semi-analytic model to
follow the evolution of the BH mass accretion and its conversion into
radiation, and compare the derived AGN bolometric luminosity function with the
observed one. While we find for the most part a very good agreement between
predicted and observed BH properties, the semi-analytic model underestimates
the number density of luminous AGN at high redshifts, independently of the
adopted Eddington factor and accretion efficiency. However, an agreement with
the observations is possible within the framework of our model, provided it is
assumed that the cold gas fraction accreted by BHs at high redshifts is larger
than at low redshifts.Comment: 15 pages, 7 figures, MNRAS submitte
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