We obtain new information on chromospheric oscillations from the appli
cation of wavelet analysis to observations of the quiet Sun in He I an
d Ca Pi lines. Using this analysing technique the temporal behaviour o
f oscillations at different frequencies is illustrated in two regions:
a magnetic element network and a non magnetic intra-network cell. The
results presented below show the duration of the chromospheric wavetr
ains and the correlation between the two lines, and also include a stu
dy of the lags between the signals.