**Solar Flare Data Set**
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*Jinyan Li and Guozhu Dong and Kotagiri Ramamohanarao and Limsoon Wong. DeEPs: A New Instance-based Discovery and Classification System. Proceedings of the Fourth European Conference on Principles and Practice of Knowledge Discovery in Databases. 2001. *
(This will be explained in Section 8.3). Note that for data sets such as chess, **flare** splice, mushroom, voting, soybean-l, t-t-t, and zoo which do not contain any continuous attributes, DeEPs does not require an ff. The accuracies of k-nearest neighbor and C5.0
*Nir Friedman and Daphne Koller. Being Bayesian about Network Structure. UAI. 2000. *
Edges Figure 2: Comparison of posterior probabilities using true posterior over orderings (x-axis) versus ordering-MCMC (y-axis). The figures show Markov features and Edge features in the **Flare** dataset with 100 samples. ordering obtained by flipping i j and i k . Now, consider the terms in Eq. (6); those terms corresponding to nodes i ` in the ordering # that precede i j or succeed i k do not
*Jinyan Li and Guozhu Dong and Kotagiri Ramamohanarao. Instance-Based Classification by Emerging Patterns. PKDD. 2000. *
(as explained in [10]). Note that for the datasets such as chess, **flare** nursery, splice, mushroom, voting, soybean-l, t-t-t, and zoo which do not contain any continuous attributes, DeEPs does not need ff. Columns 5, 6, 7, 8, and 9 give the
*Sally A. Goldman and Yan Zhou. Enhancing Supervised Learning with Unlabeled Data. ICML. 2000. *
we used for our empirical tests as well as a summary of our results. Figure 1 shows the results from one of our runs using the **Flare** data in graphical form. For this data set HOODG performed better than ID3 when using just the initial labeled data (i.e. round 0). Our cotraining procedure helped both algorithms to improve their performance. Figure 2 shows the results from
*Christophe G. Giraud-Carrier and Tony R. Martinez. An Integrated Framework for Learning and Reasoning. J. Artif. Intell. Res. (JAIR, 3. 1995. *
by Lifschitz (1988) and the UCI repository (Murphy & Aha, 1992) contains many useful training sets for inductive learning. This section reports results obtained with **FLARE** on several of these datasets. Results on a number of other uses of the framework, including two expert systems, are also presented. Finally, some of the limitations of the system are described. One artifact of the
*C. Titus Brown and Harry W. Bullen and Sean P. Kelly and Robert K. Xiao and Steven G. Satterfield and John G. Hagedorn and Judith E. Devaney. Visualization and Data Mining in an 3D Immersive Environment: Summer Project 2003. *
whole floor from above; extended semicircular layout. 42 4.12 **Solar ****Flare** /b> The Solar Flare data set was processed by Harry Bullen. This data set has been made up of only descrete variables. Unfortunately the 3D visualization did not produce interesting results. This is because most of the data
*Nir Friedman and Daphne Koller (koller@cs. stanford. edu. A Bayesian Approach to Structure Discovery in Bayesian Networks. School of Computer Science & Engineering Hebrew University. *
0.6 0.8 1 MCMC Exact 5 samples 20 samples 50 samples Markov Edges Figure 1. Comparison of posterior probabilities for the exact posterior over orders (x-axis) versus order-MCMC (y-axis) in the **Flare** dataset with 100 instances. The figures show the probabilities for all Markov features and edge features. 5. Experimental Results We evaluated our approach in a variety of ways. We first compare it with a
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