ПРИМЕНЕНИЕ ГЛУБОКИХ НЕЙРОННЫХ СЕТЕЙ ДЛЯ КЛАССИФИКАЦИИ БОЛЬШИХ ОБЪЕМОВ АСТРОНОМИЧЕСКИХ ДАННЫХ
In the process of astronomical observations are collected vast amounts of data. BSA (Big Scanning Antenna) LPI used in the study of impulse phenomena, daily logs 87.5 GB of data (32 TB per year). Experts classified 83096 individual observations (on the segment of the study July 2012 - October 2013). Over 75% of the sample correspond to pulsars, twinkling springs and rapid radiotransmitter, and all other classes of observations belong to hardware failures, interference, the flight of the Earth satellite and aircraft. There were allocated 15 classes of observations.
Such a sample, divided into classes allows using the machine learning algorithms. It has become possible to develop an automated service for short-term/long-term monitoring of various classes of radio sources (including radiotransmitted different nature), monitoring the Earth's ionosphere, the interplanetary and the interstellar plasma, the search and monitoring of different classes of radio sources. Monitoring in this case refers to the automatic filtering and detection of a previously unclassified impulse phenomena.
Currently, for automatic filtering, statistical analysis methods are used. This report examines an alternative method supposed to be using neural network machine learning algorithm that processes the input into raw data and after processing by the hidden layer through the output layer determines the class of pulse phenomena.
Creating a neural network model, trained on a sample and performing a classification of previously unclassified impulse phenomena is performed using the cloud service Microsoft Azure Machine Learning Studio. The Web service has been created based on the model allows classifying single impulse phenomena in real time (Request / Reply) and data sampling for a certain period (Batch processing).