A frequency structure of the relation between the solar activity and the meteorological parameters for periods from 2 up to 30 years has been considered. The sets of data covering about 100 years have been used. The frequency characteristics of the relationship have been deduced separately for the high, middle and low latitudes as well as for different seasons to reveal the space-frequency inhomogenity of the relation. The data used are: W O - sunspot Wolf numbers; aa - index of the geomagnetic activity; - root mean square values of tropospheric sea-level temperature gradient modules. The main result is that the display of the 11-years cycle in latitude tropospheric characteristics depends on seasons and latitudes. The highest connection level is revealed for the winter season. It is higher toward the greater latitudes.