the new fuels with magnecular structure - Institute for Basic Research

THE NEW FUELS WITH MAGNECULAR STRUCTURE 77
Figure 24. The first experimental evidence at NTS of the lack of IR signature of MS peaks.
The evidence establishes the existence of large peaks in the MS that have no IR signature at
all. The only identified IR signature, that for CO 2, refers to the constituents of the peaks of
Fig. 22. In the above figure only the IR signature of CO 2 appears because the scan was from
40 a.m.u. to 500 a.m.u. and, as such, could not include the IR signatures of other molecules
such as O 2 and CO (H 2 has no IR signature).
Note also in Fig. 24 that the computer interprets the IR signature as that
belonging to CO which interpretation is evidently erroneous because CO is outside
of the selected range of a.m.u.
All remaining small peaks of the IR scan resulted to be “unknown,” thus being
possible magnecules, following computer search in the database of IR signatures
of all known molecules available at the McClellan Air Force Base, as illustrated
in Fig. 25.
Following the removal of magnegas from the GC-MS/IRD, the background
continued to show the same anomalous peaks of Fig. 21, and reached the configuration
of Fig. 26 only after a weekend bakeout with an inert gas. Note that
the latter background is itself anomalous because the slope should have been the
opposite of that shown. The background finally recovered the conventional shape
only after flushing the instrument with an inert gas at high temperature.