File:Shareetal2004.jpg

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Shareetal2004.jpg(768 × 527 pixels, file size: 63 KB, MIME type: image/jpeg)

RHESSI count spectra of the solar 511 keV annihilation line (instrumentally broadened) derived by subtracting bremsstrahlung and nuclear contributions during the 2003 October 28 flare when the solar line was broad (11:06–11:16 UT) and narrow (11:18–11:30 UT). The solid curve is the best-fitting model that includes a Gaussian line and positronium continuum.

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current14:35, 1 November 2024Thumbnail for version as of 14:35, 1 November 2024768 × 527 (63 KB)Maintenance script (talk | contribs)== Summary == Importing file

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