Articles | Volume 37, issue 4
https://doi.org/10.5194/angeo-37-765-2019
https://doi.org/10.5194/angeo-37-765-2019
Regular paper
 | 
30 Aug 2019
Regular paper |  | 30 Aug 2019

Signatures of red-shifted foot points in the quiescent coronal loop system

Yamini K. Rao, Abhishek K. Srivastava, Pradeep Kayshap, and Bhola N. Dwivedi

Viewed

Total article views: 1,488 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
923 522 43 1,488 56 52
  • HTML: 923
  • PDF: 522
  • XML: 43
  • Total: 1,488
  • BibTeX: 56
  • EndNote: 52
Views and downloads (calculated since 09 May 2019)
Cumulative views and downloads (calculated since 09 May 2019)

Viewed (geographical distribution)

Total article views: 1,488 (including HTML, PDF, and XML) Thereof 1,352 with geography defined and 136 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 20 Nov 2024
Download
Short summary
Chromospheric flows are of significant importance in understanding the mechanisms of transfer of plasma and energy from the lower atmosphere of the Sun to the corona through the transition region. We study the quiescent loop system in terms of Doppler velocities at the foot points of individual loop strands to understand the plausible heating mechanisms driving plasma flows in such loop systems.