Page 24 - The "N" Series of Fusion Experiments

Welcome To Fusionpeery Homepage Page Two - VIDEO Understanding the Data Page Three - VIDEO Fusion Exp 1R Page Four - Fusion Letter Page Five - Companies Rx Letter Page Six - VIDEO of Fusion's Dilemma in Today's World Page Seven - Physics Dept Letter Page Eight - Gov. Officials Page Nine - Document Receipts Page Ten - Who Gains? Page Eleven - Who Looses? Page Twelve - VIDEO of EXP-BN-4 Page Thirteen - Wavelengths & Fusion Exp XX Page Fourteen - How Spectral Lines are Produced & Exp 1C Page Fifteen - Fusion Exp 2C Page Sixteen - Fusion Exp 3C Page Seventeen - Fusion Exp 1R Page Eighteen - Fusion Exp 2R Page Nineteen - Fusion Exp RW1 Page Twenty - Fusion Exp RW2 Page 21 Book Site Info Page 22 The Curse on Galileo & More Contacts Page 23 The Reactor & Other Images Page 24 "N" Series Fusions Page 25 "N" Fusion Series Continued Page 26 "A" Fusion Series Low H Page 27 EXP-46, P1, VTPR & BN 1&2 Page 28 EXP-BN High H Concentration Fusions Page 29 EXP-BN Fusions Continued

Photo Gallery of "N" Series of Common Hydrogen Fusion Experiments

This page contains extracted photos from Fusion Spectrum Videos of the "N" Series of experiments all of which used absolute minimum quantities of common Hydrogen to be fused into Helium.

The above and below photos show the Spectrums of this Experiment at Compative Times

The spectral lines produced by these fusion experiments are indicative of to which higher electron orbits the Helium atom's electrons were temporarily excited to occupy

The SDMER for experiment 1N of 19 June contained very small amounts of Hydrogen as fuel this is part of our manipulation of the experimantal variables to define the range within which the fusions can take place

Below EXP 3N of 19 June 08 Shows Helium Spectrum at expiments start and again 1 minute and five seconds later when the visible overall intensity has decreased

Below is the Helium Lamp Reference Spectrum for experiment 3N of 19 june 08 as compared to the Spectrum of the hot Helium gas ejected from the SDMER

The below spectral image was from a special experiment to capture hydrogen that did not enter the SDMER for Fusion

The only spectral line produced by the GT experiment was the Helium Yellow Line at 587.562 nanometers.

The directly below four composite images show the Spectrum from the SDMER's ejected Helium at various times during the course of fusion

Below - Experiment 2N of 19 June shows the great difference after just 5 seconds of the light radiation's increase and the increase in heat as is indicated by the continuios rainbow spectrum caused by the SDMER's incandesence

Below is the Helium Lamp Reference Spectrum for Exp 3N of 18 June 2008 This experiment had extremely low concentrations of common Hydrogen in the SDMER, as can be seen in the low intensity of the hot Helium spectrum

Below are a set of three composite images of the Helium Spectrums at different times of Experiment EXP-4N on 18 June 2008. Shown at experiment's beginning and Part II and Part III.

Below EXP-4N Part III

Below EXP-2N and the He Reference Lamp Spectrum of 19 June 08 The He spectrum shows a very weak line at 706.519 nanometers - This line is almost never seen as atmospheric Oxygen mixing with the hot Helium gas as it is ejected from the SDMER quenches this spectral line, as has been reported by other investigators, Kyoung OoK Lee, Thesis submetted to North Carolina State University - Master of Science Requirements - "Coaxial Atmospheric Pressure Plasma Discharge for Treatment of Filaments and Yarns - pdf file page 58.

The spectral line of Helium at 706.519 nm is seldom seen, because the hot Helium gas ejected from the SDMER mixes with Atmospheric Oxygen thus essentially eliminating that spectral line.