📄 ionosphere.arff
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%1. Title: Johns Hopkins University Ionosphere database%%2. Source Information:% -- Donor: Vince Sigillito (vgs@aplcen.apl.jhu.edu)% -- Date: 1989% -- Source: Space Physics Group% Applied Physics Laboratory% Johns Hopkins University% Johns Hopkins Road% Laurel, MD 20723 %%3. Past Usage:% -- Sigillito, V. G., Wing, S. P., Hutton, L. V., \& Baker, K. B. (1989).% Classification of radar returns from the ionosphere using neural % networks. Johns Hopkins APL Technical Digest, 10, 262-266.%% They investigated using backprop and the perceptron training algorithm% on this database. Using the first 200 instances for training, which% were carefully split almost 50% positive and 50% negative, they found% that a "linear" perceptron attained 90.7%, a "non-linear" perceptron% attained 92%, and backprop an average of over 96% accuracy on the % remaining 150 test instances, consisting of 123 "good" and only 24 "bad"% instances. (There was a counting error or some mistake somewhere; there% are a total of 351 rather than 350 instances in this domain.) Accuracy% on "good" instances was much higher than for "bad" instances. Backprop% was tested with several different numbers of hidden units (in [0,15])% and incremental results were also reported (corresponding to how well% the different variants of backprop did after a periodic number of % epochs).%% David Aha (aha@ics.uci.edu) briefly investigated this database.% He found that nearest neighbor attains an accuracy of 92.1%, that% Ross Quinlan's C4 algorithm attains 94.0% (no windowing), and that% IB3 (Aha \& Kibler, IJCAI-1989) attained 96.7% (parameter settings:% 70% and 80% for acceptance and dropping respectively).%%4. Relevant Information:% This radar data was collected by a system in Goose Bay, Labrador. This% system consists of a phased array of 16 high-frequency antennas with a% total transmitted power on the order of 6.4 kilowatts. See the paper% for more details. The targets were free electrons in the ionosphere.% "Good" radar returns are those showing evidence of some type of structure % in the ionosphere. "Bad" returns are those that do not; their signals pass% through the ionosphere. %% Received signals were processed using an autocorrelation function whose% arguments are the time of a pulse and the pulse number. There were 17% pulse numbers for the Goose Bay system. Instances in this databse are% described by 2 attributes per pulse number, corresponding to the complex% values returned by the function resulting from the complex electromagnetic% signal.%%5. Number of Instances: 351%%6. Number of Attributes: 34 plus the class attribute% -- All 34 predictor attributes are continuous%%7. Attribute Information: % -- All 34 are continuous, as described above% -- The 35th attribute is either "good" or "bad" according to the definition% summarized above. This is a binary classification task.%%8. Missing Values: None@relation ionosphere@attribute a01 real@attribute a02 real@attribute a03 real@attribute a04 real@attribute a05 real@attribute a06 real@attribute a07 real@attribute a08 real@attribute a09 real@attribute a10 real@attribute a11 real@attribute a12 real@attribute a13 real@attribute a14 real
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