2.3579% 1958 3.959783 0.252539 2.0623% 1957 0.133368 7.498023 3.5571% 1956 3.797279 0.263346 3.3098% 1955 0.184529 5.419200 3.4226% 1954 0.120536 8.296288 1.5421% 1953 0.358732 2.787599 1.5703% 1952 0.112375 8.898780 1.5948% 1951 4.183200 0.239051 5.0183% 1950 0.513983 1.945589 1.7034% 1949 3.133166 0.319166 -0.4250% 1948 1.605472 0.622870 6.7886% 1947 0.235107 4.253391 13.9149% 1946 2.487351 0.402034 22.7896% 1945 0.084712 11.804649 3.2661% 1944 0.405836 2.464049 1.3234% 1943 0.224373 4.456873 2.7232% 1942 0.051197 19.532409 6.5229% 1941 0.419445 2.384105 6.1527% 1940 0.138297 7.230814 -8.4517% 1930 0.082348 12.143577 -2.7367% 1929 1.972893 0.506870 -0.6823% 1927 2.013740 0.496589 6.5229% 1941 1.724919 0.579737 6.1527% 1940 1.756721 0.569242 -8.4517% 1930 0.438269 2.281706 -2.7367% 1929 0.120359 8.308458 0.0000% 1928 1.158665 0.863062 2.8137% 1921 1.972124 0.507067 -2.7367% 1929 0.954220 1.047976 0.0000% 1922 0.536751 1.863062 -0.6823% 1927 0.505155 1.979591 0.0000% 1926 1.122112 0.891177 6.5229% 1941 0.453936 2.202955 6.1527% 1940 0.064442 15.517785
telescoped