Transition region dynamics from SUMER/SOHO observations: shape of the emission spectral lines

Details Transition region dynamics from SUMER/SOHO observations: shape of the emission spectral lines Transition region dynamics from SUMER/SOHO observations: shape of the emission spectral lines

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..163r&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Computer Science

Solar Transition Region: Dynamics

Scientific paper

The quiet sun network/internetwork transition region line profiles of C II 1036.34 Å and O VI 1037.61 Å are outlined emphasizing the temporal/spatial behaviour of their deviations from the Gaussian shape. Systematic deviations of the line profiles from the single-Gaussian shape indicate that transition region emission lines consist of two Gaussian components over almost the whole quiet sun internetwork except their small innermost parts. This finding is in qualitative agreement with the transition region model of Peter (2001).

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