Positive secondary ion spectra from Irganox 1010, sputtered by Ar+, Bi+, Bi3
+, and Bi5
+ primary ions at 25 keV impact energy, are analyzed in detail. Irganox 1010 consists of a central carbon atom with 4 identical side chains or “arms”, each of C18H27O3. First, it is shown that the previously established relation, in which the secondary ion yield of the molecular species is proportional to the square of the sputtering yield, is accurately validated but, this time, for the positive, protonated molecular secondary ion instead of the previous negative deprotonated molecular secondary ion. Next, it is shown, for the first time, that the spectral ratios for Bi+ primary ions to that for Ar+ primary ions, for Bi3
+ to Ar+ and Bi5
+ to Ar+, for 389 mass channels, are comprised of the product of two basic spectra called H
Irg
* and L
Irg
* raised to powers as defined in the text. These descriptions are valid to a remarkably low relative standard deviation of 2.3% over the 389 mass channels. The above squared dependence is inherent in both H
Irg
* and L
Irg
* so that it is likely that all similar primary ion sources will exhibit the same squared dependence on the sputtering yield as found earlier for the (M−H)− yields. The power of 2 is reduced for lower-mass secondary ion fragments, falling to ∼1.5 for fragments that have 3 or 4 of the 4 arms of the molecule largely intact and to unity for those fragments that are parts of an arm. This work also shows that, for the G-SIMS of peaks with m/z ≤ 300 u it is recommended to use Bi+ and Mn+ (or Ar+) whereas, for higher mass peaks, cluster primary ions, such as Bi3
+ or Bi5
+, should be used with either Bi+ or Mn+ (or Ar+) to obtain the best signal quality.