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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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current14:34, 1 November 2024Thumbnail for version as of 14:34, 1 November 20243,404 × 1,824 (234 KB)Maintenance script (talk | contribs)== Summary == Importing file

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