Articles | Volume 37, issue 4
https://doi.org/10.5194/angeo-37-765-2019
© Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License.
Special issue:
Regular paper
| 
30 Aug 2019
Regular paper |
| 30 Aug 2019
| 30 Aug 2019
Signatures of red-shifted foot points in the quiescent coronal loop system
Related authors
Ann. Geophys., 37, 891–902, 2019
Cited articles
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Brooks, D. H., Warren, H. P., and Young, P. R.: EUV Spectral Line Formation and the Temperature Structure of Active Region Fan Loops: Observations with Hinode/EIS and SDO/AIA, Astrophys. J., 730, 85, https://doi.org/10.1088/0004-637X/730/2/85, 2011. a
Del Zanna, G.: Flows in active region loops observed by Hinode EIS, Astron. Astrophys., 481, L49, https://doi.org/10.1051/0004-6361:20079087, 2008. a, b
Del Zanna, G. and Mason, H. E.: Solar active regions: SOHO/CDS and TRACE observations of quiescent coronal loops Astron. Astrophys., 406, 1089, https://doi.org/10.1051/0004-6361:20030791, 2003. a
Del Zanna, G., O'Dwyer, B., and Mason, H. E.: SDO AIA and Hinode EIS observations of “warm” loops, Astron. Astrophys., 535, A46, https://doi.org/10.1051/0004-6361/201117470, 2011. a
