Articles | Volume 38, issue 3
https://doi.org/10.5194/angeo-38-657-2020
https://doi.org/10.5194/angeo-38-657-2020
Regular paper
 | 
05 Jun 2020
Regular paper |  | 05 Jun 2020

Development of a formalism for computing in situ transits of Earth-directed CMEs – Part 2: Towards a forecasting tool

Pedro Corona-Romero and Pete Riley

Viewed

Total article views: 2,022 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,597 398 27 2,022 33 37
  • HTML: 1,597
  • PDF: 398
  • XML: 27
  • Total: 2,022
  • BibTeX: 33
  • EndNote: 37
Views and downloads (calculated since 02 Jan 2020)
Cumulative views and downloads (calculated since 02 Jan 2020)

Viewed (geographical distribution)

Total article views: 2,022 (including HTML, PDF, and XML) Thereof 1,724 with geography defined and 298 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 24 Apr 2024
Download
Short summary
Solar storms are natural phenomena that affect technologies on which our societies are highly dependent. The understanding of solar storms and the capability to anticipate their effects on our technologies is of main interest to shield our societies. In this work we present a semi-empirical approach to increase our understanding of solar storms when they hit our planet. Additionally, we also preset a possible pathway to forecast the transits of solar storms by our planet's orbit.