Articles | Volume 16
https://doi.org/10.5194/ars-16-157-2018
https://doi.org/10.5194/ars-16-157-2018
04 Sep 2018
 | 04 Sep 2018

Ionospheric response to solar EUV variations: Preliminary results

Rajesh Vaishnav, Christoph Jacobi, Jens Berdermann, Erik Schmölter, and Mihail Codrescu

Viewed

Total article views: 1,493 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
949 469 75 1,493 69 76
  • HTML: 949
  • PDF: 469
  • XML: 75
  • Total: 1,493
  • BibTeX: 69
  • EndNote: 76
Views and downloads (calculated since 04 Sep 2018)
Cumulative views and downloads (calculated since 04 Sep 2018)

Viewed (geographical distribution)

Total article views: 1,397 (including HTML, PDF, and XML) Thereof 1,391 with geography defined and 6 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 10 Oct 2024
Download
Short summary
We investigate the ionospheric response to solar Extreme Ultraviolet (EUV) variations using different solar proxies and IGS TEC maps. An ionospheric delay in GTEC is observed at the 27 days solar rotation period with the time scale of about ~ 1–2 days. Here we present preliminary results from the CTIPe model simulations which qualitatively reproduce the observed ~1-2 days delay in GTEC, which is might be due to vertical transport processes.