In a quiescent coronal loop system, Si IV line profiles show transition-region downflows of about 1 to 7 km/s at moss footpoints, while photospheric and chromospheric lines show negligible flows.
E.: Solar active regions: SOHO/CDS and TRACE observations of quiescent coronal loops A&A
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Signatures of red-shifted footpoints in the quiescent coronal loop system
In a quiescent coronal loop system, Si IV line profiles show transition-region downflows of about 1 to 7 km/s at moss footpoints, while photospheric and chromospheric lines show negligible flows.