Craster Parabolic Projections

Figure 1. The Craster parabolic projection in its uninterrupted form.

Along with the Mollweide, the Craster parabolic is the projection of choice for the aficionado of interrupted maps. It is widely used to build both parallel (Figure 2) and sinusoidal interrupted maps (Figure 3).
Figure 2. A parallel interrupted version of the Craster parabolic projection.

The earliest form of what is now known as the Craster parabolic projection was developed by John Evelyn Edmond Craster in 1929; it was refined into its modern form by Charles H. Deetz and O.S. Adams in 1934. Also in 1934, another geodetic scientist named Reinholds V. Putnins independently introduced a new projection that he called the P4. It turns out that the P4 was identical to the Craster parabolic, and since Craster introduced his projection first, he is typically given the credit for developing (and the right of naming) this projection.
Figure 3. A sinusoidal interrupted version of the Craster parabolic projection.