Ionospheric electron content (IEC) observed at Delhi (geographic co-ordinat
es: 28.63 degreesN, 77.22 degreesE; geomagnetic co-ordinates: 19.08 degrees
N, 148.91 degreesE; dip Latitude 24.8 degreesN), India, for the period 1975
-80 and 1986-89 belonging to an ascending phase of solar activity during fi
rst halves of solar cycles 21 and 22 respectively have been used to study t
he diurnal, seasonal, solar and magnetic activity variations. The diurnal v
ariation of seasonal mean of IEC on quiet days shows a secondary peak compa
rable to the daytime peak in equinox and winter in high solar activity. IEC
max (daytime maximum value of IEC, one per day) shows winter anomaly only d
uring high solar activity at Delhi. Further, IECmax shows positive correlat
ion with F-10.7 Up to about 200 flux units at equinox and 340 units both in
winter and summer; for greater F10.7 values, IECmax is substantially const
ant in all the seasons. IECmax and magnetic activity (A(p)) are found to be
positively correlated in summer in high solar activity. Winter IECmax show
s positive correlation with A(p) in low solar activity and negative correla
tion in high solar activity in both the solar cycles. In equinox IECmax is
independent of A(p) in both solar cycles in low solar activity. A study of
day-to-day variations in IECmax shows single day and alternate day abnormal
ities, semi-annual and annual variations controlled by the equatorial elect
rojet strength, and 27-day periodicity attributable to the solar rotation.