Substituting a=rcosθ and b=rsinθ (where r=∣z∣ and θ=arg(z)) into z=a+ib gives the polar form z=r(cosθ+isinθ). The ordered pair (r,θ) is called the polar coordinates of the point representing z, describing the very same point that the Cartesian pair (a,b) describes, just measured as a distance-and-direction from the origin instead of as horizontal-and-vertical offsets. Converting from Cartesian to polar form means computing the modulus and the quadrant-corrected argument as usual and substituting them in; converting from polar back to Cartesian means evaluating cosθ and sinθ for the given angle and multiplying through by r. The polar form is especially convenient whenever a complex number's 'size' and 'direction' from the origin matter more than its individual real and imaginary parts.