There are too many lines predicted. Where are they identified and described?
The emission lines now consist of several sets that represent the archeological past of the code. This link gives some of the more prominent strong lines and their identification in the code. Each line is identified by a four character label and an integer wavelength. This strategy is outlined in Part IV, pages 612-614. Often the line label is the spectroscopic designation of the spectrum, such as H 1 or Fe19. For many lines various contributors are also indicated, and these will have different labels but the same wavelength. The integer wavelength can be in various units, depending on its order of magnitude. This is described on page 626 of Part IV. Only the strongest lines are printed to save space, and not all contributors to lines are printed. You change the threshold for the faintest line to print with the print faint command described on page 99 of Part I. You can print various contributors to many lines with the print line options commands described on pages 99-100 of Part I. I
