File:157f2.png

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Left: up-scattered photon spectra at the Sun (photons per keV per second per electron) from anisotropic electron distributions along the line of sight in the ultra-relativistic regime. Right: up-scattered photon spectra at the Sun (photons per keV per second per electron) from a beamed electron distribution along the line of sight in the mildly relativistic regime. See the full paper for full details.

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Date/TimeThumbnailDimensionsUserComment
current14:29, 16 August 2011Thumbnail for version as of 14:29, 16 August 20113,404×1,824 (234 KB)Hhudson (Talk | contribs) (Reverted to version as of 14:12, 16 August 2011)
14:29, 16 August 2011Thumbnail for version as of 14:29, 16 August 2011489×255 (201 KB)Hhudson (Talk | contribs) (Left: up-scattered photon spectra at the Sun (photons per keV per second per electron) from anisotropic electron distributions along the line of sight in the ultra-relativistic regime. Right: up-scattered photon spectra at the Sun (photons per keV per sec)
14:25, 16 August 2011Thumbnail for version as of 14:25, 16 August 2011489×255 (201 KB)Hhudson (Talk | contribs) (A part of the sky seen at high energies by the [http://en.wikipedia.org/wiki/Enrico_Fermi] satellite observatory, as presented by [http://apod.nasa.gov/apod/ap090321.html APOD]. The bright parts of the image are the plane of our galaxy, and the streak sho)
14:12, 16 August 2011Thumbnail for version as of 14:12, 16 August 20113,404×1,824 (234 KB)Hhudson (Talk | contribs) (Left: up-scattered photon spectra at the Sun (photons per keV per second per electron) from anisotropic electron distributions along the line of sight in the ultra-relativistic regime. Right: up-scattered photon spectra at the Sun (photons per keV per sec)

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