The Relationship between EUV Brightenings and Dark Mottles in the Quiet Sun

Details The Relationship between EUV Brightenings and Dark Mottles in the Quiet Sun The Relationship between EUV Brightenings and Dark Mottles in the Quiet Sun

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..257k&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

The relationship between EUV brightenings in the transition region and dark mottles in the chromosphere is studied using data obtained in an observational campaign between the Coronal Diagnostic Spectrometer (CDS) on SOHO and the Domeless Solar Telescope (DST) at Hida Observatory. We found several examples of EUV brightenings accompanied by upflowing dark mottles in the chromosphere. This suggests that EUV blinkers are formed by the heating of dark mottles or spicules.

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