In [9], all possible electron inter-shell transitions for the "normal" orbitals, were analysed for permissability and presented as a series of tables, i.e. [9], Section 4.0, Tables (i), (ii) and (iii). Here, those tables are consolidated and extended to incorporate the hyperfine orbitals. To simplify matters, the quadrant numbers are omitted in order to make way for details concerning the status of the proton.

The nomenclature adopted for the type numbers are as those in [9], Section 4.0, Tables (i), (ii) and (iii), with the bracketted sense of D_pn_sp added to distinguish the hyperfine orbitals. In the "Status" column, Ö.K". means this transition is permitted by the Selection Rules. "N.P." means the transition is not.

Note 1 in Table C.1 below.

This transition is into a spin-up quadrant in which the spin induction mechanism and the external stimulus are complementary for the proton. It cannot therefore change proton spin from spin-up to spin-down. Hence the transition is "N.P", {Selection Rule (2.6)}

In the downloadable spreadsheet Hydrogen Spectra, in Appendix A, the algorithm for Selection Rule (2.6) has been truncated to omit the status of _en_sp in the receiving orbital, because transition type 6(-) does not occur between orbit shells 3 & 2 to 2 & 1.

Although not shown in the table below, it is noted for interest that the hyperfine transition 1s_h2(-) Þ 1s(+), is a type 2 transition.

It is important to note that as a result of the Selection Rule extensions in this paper, transitions into some orbitals are more prevalent than into others. This will affect the distribution of spectral relative intensities.