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the new fuels with magnecular structure - Institute for Basic Research

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THE NEW FUELS WITH MAGNECULAR STRUCTURE 133<br />

Figure 53. A sample of various additional scans conducted by SunLabs on <strong>the</strong> HHO gas detecting<br />

anomalous peaks at 33, 34 and 40 amu that cannot possibly have a consistent molecular<br />

interpretation. Intriguingly, <strong>the</strong> peak at 35 amu detected in o<strong>the</strong>r tests did not appear sequentially<br />

in this scan, and appeared instead in o<strong>the</strong>r scans here not reported <strong>for</strong> brevity, thus<br />

indicating that <strong>the</strong> peaks of this and of <strong>the</strong> preceding scans conducted by SunLabs are, in actuality,<br />

<strong>the</strong> constituents of <strong>the</strong> clusters composing <strong>the</strong> HHO gas, and not <strong>the</strong> actual constituents<br />

<strong>the</strong>mselves.<br />

2/3 H 2 and 1/3 O 2 cannot melt instantly tungsten and bricks , as any interested<br />

chemist is encouraged to verify.<br />

It should be indicated that a number of species in <strong>the</strong> HHO gas, particularly<br />

those <strong>with</strong> higher specific weight, are expected to be unstable and, as such, decomposed<br />

by <strong>the</strong> analytic instrument itself. In different terms, by no means GC,<br />

IR and o<strong>the</strong>r scans should be expected to detect all constituents of <strong>the</strong> HHO<br />

gas, since a number of <strong>the</strong>m are expected to be decomposed or altered by <strong>the</strong><br />

ionization and o<strong>the</strong>r processes connected to <strong>the</strong> scans <strong>the</strong>mselves.

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