A Contribution to the Understanding of Chromospheric Oscillations

Details A Contribution to the Understanding of Chromospheric Oscillations A Contribution to the Understanding of Chromospheric Oscillations

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007soph..241...39b&link_type=abstract

Solar Physics, Volume 241, Issue 1, pp.39-51

Physics

3

Scientific paper

We present SUMER/SOHO UV measurements of chromospheric oscillations of intensity, velocity, and linewidth observed in C I, S I, O I, and C II lines, which are formed in the altitude range from 1000 km to 2000 km above τ 500=1. Oscillations in lines originating at similar altitudes exhibit different behaviors which we discuss in terms of the formation of the lines.

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