Evidence for Wave Dissipation through EUV Emission Line Narrowing

Details Evidence for Wave Dissipation through EUV Emission Line Narrowing Evidence for Wave Dissipation through EUV Emission Line Narrowing

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..229h&link_type=abstract

Proceedings of 'SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO a

Computer Science

Scientific paper

Using long-duration observations over closed-field, quiet Sun regions
above the solar equator, evidence has been found for the narrowing of
coronal emission lines with increasing altitude. This is interpreted as
evidence for wave dissipation in the quiet Sun corona.

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