  The Ca-K spectroheliograms obtained at the Kodaikanal observatory (KO) are
used to generate a uniform time series using the equal contrast technique (ECT)
to study the long and short-term variation in the solar chromosphere. The
percentage of plage, Enhanced network (EN), Active network (AN), and Quiet
network (QN) area at various latitudes is compared with the activity at
35$^{\circ}$ latitude and also with the sunspot number for the period of 1907
-- 1984. The values of phase differences indicate that the activity begins at
$\sim$45$^{\circ}$ latitude and shift progressively to the lower latitude at a
speed of $\sim$~9.4~m~sec$^{-1}$ . The shift speed slows down gradually and
reaches $\sim$~3~m~sec$^{-1}$ at $\sim$5$^{\circ}$ latitude. No phase
difference between the variations of Ca-K activity at 55$^{\circ}$,
65$^{\circ}$, and 75$^{\circ}$ latitude belts implies that changes in the
activity are happening simultaneously. The analysis shows that the activity at
polar latitude belts is anti-correlated with the sunspot number. This study
indicates that a multi-cell meridional flow pattern could exist in the solar
convection zone. One type of cell could transport the magnetic elements from
mid-latitude to low-latitude belts through meridional flows, and the other one
could be operating in the polar region.
