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20032011
most citedDetermination of the Charged Pion Form Factor at Q2=1.60 and 2.45 (GeV/c)2

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astro-ph2003

Enhancement of the helium resonance lines in the solar atmosphere by suprathermal electron excitation II: non-Maxwellian electron distributions

G. R. Smith

In solar EUV spectra the He I and He II resonance lines show unusual behaviour and have anomalously high intensities compared with other transition region lines. The formation of t…