  We show that the time series of sunspot-group areas has a gap, the so-called
Gnevyshev gap (GG), between ascending and descending phases of the cycle and
especially so for the even-numbered cycles. For the odd cycles this gap is less
obvious, and is only a small decline after the maximum of the cycle. We
resample the cycles to have the same length of 3945 days (about 10.8 years),
and show that the decline is between 1445-1567 days after the start of the
cycle for the even cycles, and extending sometimes until 1725 days from the
start of the cycle. For the odd cycles the gap is a little earlier, 1332-1445
days after the start of the cycles with no extension. We analyze geomagnetic
disturbances for Solar Cycles 17-24 using the Dst-index, the related Dxt- and
Dcx-indices, and the Ap-index. In all of these time series there is a decline
at the time, or somewhat after, the GG in the solar indices, and it is as
deepest between 1567-1725 days for the even cycles and between 1445-1567 days
for the odd cycles. The averages of these indices for even cycles in the
interval 1445-1725 are 46%, 46%, 18%, and 29% smaller compared to surrounding
intervals of similar length for Dst, Dxt, Dcx, and Ap, respectively. For odd
cycles the averages of the Dst- and Dxt-indices between 1322-1567 days are 31%
and 12% smaller than the surrounding intervals, but not smaller for the
Dcx-index and only 4% smaller for the Ap-index. The declines are significant at
the 99% level for both even and odd cycles of the Dst-index and for Dxt-, Dcx-
and Ap-indices for even cycles. For odd cycles of the Dxt-index the
significance is 95%, but the decline is insignificant for odd cycles of the
Dcx- and Ap-indices.
