Characteristics of quiet Sun cell and network brightenings

Extreme ultraviolet observations of the quiet Sun are made with the Coronal Diagnostic Spectrometer (CDS) on board the Solar and Heliospheric Observat ory (SOHO). It has been previously noted that frequent transition region br ightenings occur in both the bright network and dark cell regions. Analysin g 1125 events, we determined the characteristics of the brightenings in the cell and network regions which include the duration, energy, and intensity increase above the background. Network brightenings are found to be larger than cell events occurring with a mean duration of 150 s and releasing an average of 10(26.9) ergs per event. Cell brightenings, on the other hand, l ast for an average of 96 s and release 10(25.8) ergs per event. It has also been found that the distribution of energy is a power-law which is differe nt in the cell (gamma =2.5) and network (gamma =1.5) regions. When the enti re quiet Sun region is analysed the value of gamma is 1.7. The number of ev ents per CDS pixel is approximately the same, and a histogram of the ratio ([peak value - background]/background) shows similar values for both the ce ll and network. It is important to analyse the cell and network regions sep arately in the context of coronal heating by such small flare-like events.