| 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 g,b antenna1: continuous antenna2: continuous antenna3: continuous antenna4: continuous antenna5: continuous antenna6: continuous antenna7: continuous antenna8: continuous antenna9: continuous antenna10: continuous antenna11: continuous antenna12: continuous antenna13: continuous antenna14: continuous antenna15: continuous antenna16: continuous antenna17: continuous antenna18: continuous antenna19: continuous antenna20: continuous antenna21: continuous antenna22: continuous antenna23: continuous antenna24: continuous antenna25: continuous antenna26: continuous antenna27: continuous antenna28: continuous antenna29: continuous antenna30: continuous antenna31: continuous antenna32: continuous antenna33: continuous antenna34: continuous