the new fuels with magnecular structure - Institute for Basic Research

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74 RUGGERO MARIA SANTILLI analysts Louis A. Dee, Branch Manager, and Norman Wade who operated an HP GC model 5890, an HP MS model 5972, equipped with an HP IRD model 5965. Upon inspection at arrival, the instrument met all conditions indicated in the preceding sections then, and only then, measurements were permitted. Thanks to a professional cooperation by the NTS analysts, the equipment was set at all the unusual conditions indicated later on. In particular, the equipment was set for the analytic method VOC IRMS.M utilizing an HP Ultra 2 column 25 m long with a 0.32 mm ID and a film thickness of 0.52 µm. It was also requested to conduct the analysis from 40 a.m.u. to the instrument limit of 500 a.m.u. This condition was necessary to avoid the expected large CO peak of magnegas at 28 a.m.u. Moreover, the GC-MS/IRD was set at the low temperature of 10 ◦ C; the biggest possible feeding line with an ID of 0.5 mm was installed; the feeding line itself was cryogenically cooled; the equipment was set at the longest possible ramp time of 26 minutes; and a linear flow velocity of 50 cm/sec was selected. A number of other technical requirements are available in the complete documentation of the measurements. The analysts first secured a documentation of the background of the instrument prior to any injection of magnegas (also called blank). Following a final control that all requested conditions were implemented, the tests were initiated. The results, reported in part via the representative scans of Figs. 21 to 26, constitute the first direct experimental evidence of the existence of magnecules in gases. After waiting for 26 minutes, sixteen large peaks appeared on the MS screen between 40 and 500 a.m.u. as shown in Fig. 21. Each of these sixteen MS peaks resulted to be “unknown,” following a computer search of database on all known molecules available at McClellan Air Force Base, as illustrated in Fig. 22 No identifiable CO 2 peak was detected at all in the MS spectrum between 40 and 500 a.m.u., contrary to the presence of 9% of such a molecule in magnegas as per conventional analyses (4.11). Upon the completion of the MS measurements, exactly the same range of 40 to 500 a.m.u. was subjected to IR detection. As expected, none of the sixteen peaks had any infrared signature at all, as shown in Fig. 23. Furthermore, the IR scan for these MS peaks shows only one peak, that belonging to CO 2 , with additional small peaks possibly denoting traces of other substances. Note that the IR signature of the other components, such as CO or O 2 cannot be detectable in this IR test because their atomic weights are below the left
THE NEW FUELS WITH MAGNECULAR STRUCTURE 75 Figure 22. A reproduction of the MS peaks providing the first experimental evidence of the existence of magnecules identified on June 19, 1998, by analysts Louis A. Dee and Norman Wade of the branch of National Technical; Systems (NTS) located at the McClellan Air Force Base in North Highland, near Sacramento, California, with support from Toups Technologies Licensing, Inc. (TTL) of Largo, Florida. The scan is restricted from 40 a.m.u to 500 a.m.u. The peaks refer to magnegas produced via an electric arc between consumable carbon electrodes within ordinary tap water with conventional chemical composition (8.20). Therefore, only the CO 2 peak was expected to appear in the scan with any macroscopic percentage, while no CO 2 was detected at all in the MS scan.
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THE NEW FUELS WITH MAGNECULAR STRUC
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Contents Preface 1 THE INCREASINGLY
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HADRONIC MATHEMATICS, MECHANICS AND
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190 RUGGERO MARIA SANTILLI Ethereal
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192 RUGGERO MARIA SANTILLI Isodual
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194 RUGGERO MARIA SANTILLI Newton-S
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the new fuels with magnecular structure - Institute for Basic Research

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