[http://smtp.antelecom.net/blogs/bsmrapaiva/ (Marquis Who's Who In America; Who's Who In Science and Engineering; Who's Who in the World 2014)]
http://smtp.antelecom.net/blogs/bsmrapaiva/
Email: clifford.paiva@gmail.com
Baseline Bridge .8 micron video of Crab Pulsar was taken using a LUCKY IMAGING camera from Cambridge University
http://apod.nasa.gov/apod/ap950624.html
http://en.wikipedia.org/wiki/Crab_Pulsar [as shown on Wikipedia...minus the embarrassing EMHD (electromagneto-hydrodynamic) bridge of course...]
These stellar explosion resulted in angular momentum proportionately remained in the high angular velocity star core and outer rotating hot gas. The Crab Nebula was observed in X-ray light by Chandra (left, blue) and optical light (right, red) from Hubble Space Telescope. This was then correlated using image processing at BSM Research, to LUCKY CAM (Cambridge University) video [optical band-pass (.39 - .78 microns) for confirmation of the discharge bridge.
If published nominal distance values are used (Geminga = 850 lyrs; Crab Nebula resultant spinning core = 6,500 lyrs) the minimum linear distance between the pulsars = 5650 lyrs. This means that the approximate November 2000 -- April 2001 duration of the Chandra video requires the plasma discharge velocity (between Geminga and Crab Nebula core) to be:
(5650 lyr) /(.42 year) = 13452.38 lyr/yr = 36.86 lyr/day = 1.54 lyr/3600 second = 4.28(10)^(-4) lyr/second; or 2.52e^9 miles/second; or 2.52(10)^9 miles/second. Dividing this by 186000 mi/s (light speed): 2.52(10)^9 / 186000 mi/s = 13526.88 times faster the light speed for the Geminga/Crab Nebula Pulsars' plasma discharge.
