Profile: Kenyon

Your personal background.
Hey:
My Name is Kenyon. The Girls call me wolfy.
I\\\\\\\\\\\\\\'m 50 years old. I claim to be an amature Scientist. I\\\\\\\\\\\\\\'m into Amature Radio(Ham),
Radio Astronomy and Optical Astronomy. I operate 2 SIDs (Sudden Ionispheric Disturbance Recievers) One called VLF (Very Low Frequency) and one GYRATOR Reciever. The Gyrator Is a fancy VLF Reciever. Once I have found a means to send my data to the A.A.V.S.O. ( American Association Of Variable Star Observers) I too will be a Station on line to assist in forcasting.

I have a 12Ghz Radio Telescope. A High School Science Fair Project and a 1.2 Ghz Radio Telescope Reciever. I\\\\\\\\\\\\\\'m awaiting funds for an antenna for the 1.2 Ghz. I have a Homade Magnetometer and 3 Homade electronic Seismometers I\\\\\\\\\\\\\\'m experimenting with.

I live in the very small Mississippi town of St Martin. It sound exotic. Actually it\\\\\\\\\\\\\\'s kind of a \\\\\\\\\\\\\\'redneck\\\\\\\\\\\\\\' lil neighborhood.

I call my little niche \\\\\\\\\\\\\\'The Mississippi Gulf Coast SETI Station\\\\\\\\\\\\\\'. And I have been involved with the SETI@Home project for a couple of years now. I am ;by MUFON( Mutual UFO Network); a certified field investigator and am intrested in Ufology.

I\\\\\\\\\\\\\\'ve been intrested in Science and Technology as long as I can Remember. At one time I was studying to be an Astro Physcists but I have a very poor understanding of Mathematics.

I \\\\\\\\\\\\\\'endevor to perciveer\\\\\\\\\\\\\\'. LOL.

Thanks for the intrest

Kenyon Lenart
Your opinions about Einstein@Home
I think this is a very intresting project. To detect intergalatic Gauss. I can only guess as to the insturment of detection less the \\\\\\\\\\\\\\'Matehmatics\\\\\\\\\\\\\\' involved. If you have any plans for simple reciever for detection I could try to build and operate one of my own...LOL.

Like my 1.2 Ghz radio Telescope there must be some simple detection devices I could build at home.

If there are plans; send some soon.

Kenyon Lenart
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This material is based upon work supported by the National Science Foundation (NSF) under Grant NSF-0200852 and by the Max Planck Gesellschaft (MPG). Any opinions, findings, and conclusions or recommendations expressed in this material are those of the investigators and do not necessarily reflect the views of the NSF or the MPG.

Copyright © 2009 Bruce Allen for the LIGO Scientific Collaboration