We discuss the results of recent collaborative investigations of the Sun that combine Very Large Array (VLA) images at 91.6 cm wavelength with SOHO/EIT and TRACE EUV spectroheliograms at several wavelengths. The main objective of these observations was to investigate the spatial and temporal relationship between nonthermal decimetric burst activity and small-scale transient EUV events in active regions. Our VLA 91 cm observations show changes in the intensity of overlying Type I noise storms a few minutes after five of seven transient brightenings observed by SOHO and TRACE. This suggests that these evolving EUV sources may have played a role in the production of nonthermal electrons eventually seen in the noise storm emission at greater heights.