This paper presents the thicknesses and inclinations (i.e., the angle
between the galactic plane and the tangent plane) of 71 northern spira
l galaxies. The method for measuring the thickness has been proposed b
y Peng. It is based on the solution of Poisson's equation for a logari
thmic disturbance of density. The inclination is determined by assumin
g that the pattern of spiral structure is a logarithmic spiral. We fin
d that the thickness is correlated with color and with the H-alpha + [
NII] equivalent width.