Intense Blinker in Active Regions

Details Intense Blinker in Active Regions Intense Blinker in Active Regions

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.547..257y&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

2

The Sun, Active Regions, Blinkers

Scientific paper

A particular class of active region brightenings seen with the Coronal Diagnostic Spectrometer on SOHO show transition region emission lines enhanced by factors of around 1000 over quiet Sun values. The brightenings have high density ( 1012 cm-3 ) and are estimated to be around 0.1-0.2 arcsec in size. They are predominantly found in active regions whose magnetic structure is rapidly evolving. High cadence time sequences yield lifetimes of around 5 mins.

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