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Gamma Rays in Pulsars

This animation takes us into a spinning pulsar, with its strong magnetic field rotating along with it. Clouds of charged particles move along the field lines and their gamma-rays are beamed like a lighthouse beacon by the magnetic fields. As our line of sight moves into the beam, we see the pulsations once every rotation of the neutron star.
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This animation shows gamma-rays from a pulsar    This animation shows gamma-rays from a pulsar
Duration: 39.2 seconds
Available formats:
  1280x720   Frames
  512x288     MPEG-1   13 MB
  1280x720   MPEG-2   82 MB
  1280x720   QT         1 GB
  640x360     MPEG-4   6 MB
  960x540     WEBM         23 MB
  320x180     PNG           228 KB
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Short URL to This Page:http://svs.gsfc.nasa.gov/goto?20136
Animation Number:20136
Completed:2008-04-16
Animator:Walt Feimer (HTSI) (Lead)
Scientists:Alice Harding (NASA/GSFC)
 Steven Ritz (NASA/GSFC)
Platform/Sensor/Data Set:Fermi/LAT
Series:Astrophysics Animations
Please give credit for this item to:
NASA/Goddard Space Flight Center Conceptual Image Lab
 
Keywords:
SVS >> Gamma Ray
SVS >> HDTV
DLESE >> Space science
SVS >> Astrophysics
SVS >> Universe
SVS >> Pulsar
SVS >> GLAST
SVS >> Space
SVS >> Fermi
 
 


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Many of our multimedia items use the GCMD keywords. These keywords can be found on the Internet with the following citation:
Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0

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