AAS 196th Meeting, June 2000 Session 54. Because the model is stochastic, we cannot directly compare a simulated light-curve with the observed. Data gaps and deadtime corrections derived for the data set are applied to the simulations before making the comparisons.
Many criteria are available to characterize the level of agreement of a model and data.
We show examples of application to EUVE Deep Survey observations of several late-type stars and discuss the results in the context of flare contributions to coronal heating.