Code Name: Total Eclipse

Code Name: Total Eclipse

Author: Gary L. Lucas

Publisher: Trafford Publishing

Published: 2012-11-21

Total Pages: 398

ISBN-13: 1466954310

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Lee Dunway, a hardened CIA undercover agent receives a frantic call from his ex-wife Julie informing him that their young daughter, Gail, has been kidnapped. Julie was warned not to notify the FBI or the police. She believes Lee is Gails best chance to be rescued alive. Lee is pulled into a connecting plot of intrigue and deadly sabotage. America is on the verge of producing cold fusion energy from the Helium-3 isotope that is secretly being mined on the moon. A space shuttle has launched from a top-secret base in Alaska to bring back the first twelve ton load of He-3, which must be left in earth orbit for a later descent. This knowledge has opened the door to a treasonous conspiracy involving members of the U.S. Congress and other high ranking officials called the Centurions. They plan to steal the high valued He-3 while it circles the earth as a means to manipulate world currency markets and finance their goal to form a one world government. Lee and two others must find a way to highjack the He-3 before they do. CODE NAME: TOTAL ECLIPSE is fused together by a bittersweet love story and a perplexing betrayal Lee must come to grips with to simultaneously rescue Gail and stop the Centurions.


Dictionary of Minor Planet Names

Dictionary of Minor Planet Names

Author: Lutz D. Schmadel

Publisher: Springer Science & Business Media

Published: 2009-06-23

Total Pages: 320

ISBN-13: 364201965X

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The history and rapid development of minor planet dis In addition to citing the bibliographic source of the nam coveries constitute a fascinating story and one with a ing, we also provide the source of numbering. A spe rather breathtaking evolution. By October 2005, the cial concordance list will enable the evaluation of the total of numbered planets exceeded the remarkable cor respective publication dates. The complete work is, nerstone of 100,000 objects and only three years later of course, a thoroughly revised and considerably en in November 2008 we are even faced with minor planet larged data collection and every e?ort has been made ( ) 200000 . This dramatic evolution must be compared to check and correct each single piece of information ( ) with the huge time span of two centuries 1801–2000 again. For even more detailed information on the dis that was necessary to detect and to re?ne the orbits of covery circumstances of numbered but unnamed plan only the ?rst 20,000 minor planets. Nowadays, we need ets, the reader is referred to the extensive data ?les even less than 13 months for the same quantity! At the compiled by the Minor Planet Center. end of 2005, we had achieved a total of 12,804 named ( According to a resolution of IAU Division III 2000, minor planets a fraction of less than 11 per cent of ) Manchester IAU General Assembly DMPN attained all numbered minor planets.


1965 Solar Eclipse Partial Reflection Experiment

1965 Solar Eclipse Partial Reflection Experiment

Author: Heinrich Andreas Von Biel

Publisher:

Published: 1965

Total Pages: 88

ISBN-13:

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A partial reflection experiment, conducted on Aitutaki, Cook Island, before, during and after the 1965 Solar Eclipse, is described. A small portion of the data collected during the expedition is presented in the form of ten electron density profiles collected between the times of 13 minutes before totality until two and one half hours after totality. Also included is a three day noon-time average electron density profile for comparison purposes. The statistics of D-region echoes are described and their implications are discussed. The general conclusion from the data is that the solar eclipse caused little, or no changes in the electron density distribution at altitudes below 75 km. The predominant eclipse effects were noticed at altitudes of 78 km and higher. The data presented also suggest that the D-region electron density recovered to near normal in a time interval of about 80 minutes after totality. Even though the data analyzed are too few to reach definite conclusions regarding the electron density history during the eclipse, the trends evident from the results are sufficiently well defined to establish the usefulness of the experimental technique for D-region investigation during a solar eclipse. (Author).