An Optimized Iterative Partitioning Model for Predicting Computer System Failures Based on Deep Learning

Author(s):  
Mohammed El Fouki ◽  
Noura Aknin ◽  
Kamal Eddine El Kadiri
2021 ◽  
Vol 3 (1) ◽  
pp. 66-74
Author(s):  
Ranganathan G

In the near future, deep learning algorithms will be incorporated in several applications for assisting the human beings. The deep learning algorithms have the tendency to allow a computer to work on its assumption. Most of the deep learning algorithms mimic the human brain’s neuron connection to leverage an artificial intelligence to the computer system. This helps to improve the operational speed and accuracy on several critical tasks. This paper projects the blocks, which are required for the incorporation of deep learning based algorithm. Also, the paper attempts to deeply analyze the necessity of the preprocessing step over several deep learning based applications.


1986 ◽  
Vol 5 (3) ◽  
pp. 211-217 ◽  
Author(s):  
Lance J. Hoffman ◽  
Lucy M. Moran

2021 ◽  
Author(s):  
Amirhossein Mostajabi ◽  
Ehsan Mansouri ◽  
Pedram Pad ◽  
Marcos Rubinstein ◽  
Andrea Dunbar ◽  
...  

<p>Lightning is  responsible directly or indirectly, for significant human casualties and property damage worldwide. <sup>1,2</sup>  It can cause injury and death in humans and animals, ignite fires, affect and destroy electronic devices, and cause electrical surges and system failures in airplanes and rockets.<sup>3–5</sup> These severe and costly outcomes can be averted by predicting the lightning occurrence in advance and taking preventive actions accordingly. Therefore, a practical and fast lightning prediction method is of considerable value.</p><p>Lightning is formed in the atmosphere through the combination of complex dynamic and microphysical processes, making it difficult to predict its occurrence using analytical or probabilistic approaches. In this work, we aim at leveraging advances in machine learning, deep learning, and pattern recognition to develop a lightning nowcasting model. Current numerical weather models rely on lightning parametrization. These models suffer from two drawbacks; the sequential nature of the model limits the computation speed, especially for nowcasting, and the recorded data are only used in the parametrization step and not in the prediction.<sup>6,7</sup></p><p>To cope with these drawbacks, we propose to leverage the large amounts of available data to develop a fully data-driven approach with enhanced prediction speed based on deep neural networks. The developed lightning nowcasting model is based on a residual U-net architecture.<sup>8</sup> The model consists of two paths from the input to the output: (i) a highway path copying the input to the output in the same way as the persistent baseline model does, and (ii) a fully convolutional U-net which learns to adjust the former path to reach the desired output. The U-net itself consists of a contracting part with alternating convolution, and max pooling layers followed by an expanding part of alternating upsampling, convolution, and concatenation layers.<sup>9–11</sup></p><p>Our dataset consists of post-processed data of recorded lightning occurrences in 15-minute intervals over 60 days obtained from the GOES satellite over the Americas. We have optimized the model using data from the northern part of South America, a region characterized by high lightning activity. The model was then applied to other regions of the Americas. We are using 70-15-15% separation for training, validation, and test datasets. Upon completion of the training process, the model can achieve an overall F1 score of 70% with a lead time of 30 minutes over South America in fractions of a second. This is more than 25% increase in the F1 score compared to the persistent model which is used as our baseline forecast method.</p><p>To the best of our knowledge, our model is the first data-driven approach for lightning prediction. The developed model can pave the way to large-scale, efficient, and practical lightning prediction, which in turn can protect lives and save resources.</p>


Author(s):  
Volodymyr Kindratenko ◽  
Dawei Mu ◽  
Yan Zhan ◽  
John Maloney ◽  
Sayed Hadi Hashemi ◽  
...  

Author(s):  
Ivan Bozhikov ◽  
Rumen Popov ◽  
Slavi Lyubomirov ◽  
Daniela Shehova

1979 ◽  
Vol 44 ◽  
pp. 41-47
Author(s):  
Donald A. Landman

This paper describes some recent results of our quiescent prominence spectrometry program at the Mees Solar Observatory on Haleakala. The observations were made with the 25 cm coronagraph/coudé spectrograph system using a silicon vidicon detector. This detector consists of 500 contiguous channels covering approximately 6 or 80 Å, depending on the grating used. The instrument is interfaced to the Observatory’s PDP 11/45 computer system, and has the important advantages of wide spectral response, linearity and signal-averaging with real-time display. Its principal drawback is the relatively small target size. For the present work, the aperture was about 3″ × 5″. Absolute intensity calibrations were made by measuring quiet regions near sun center.


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