Articles | Volume 37, issue 4
https://doi.org/10.5194/angeo-37-561-2019
https://doi.org/10.5194/angeo-37-561-2019
Regular paper
 | 
11 Jul 2019
Regular paper |  | 11 Jul 2019

GUMICS-4 analysis of interplanetary coronal mass ejection impact on Earth during low and typical Mach number solar winds

Antti Lakka, Tuija I. Pulkkinen, Andrew P. Dimmock, Emilia Kilpua, Matti Ala-Lahti, Ilja Honkonen, Minna Palmroth, and Osku Raukunen

Viewed

Total article views: 3,746 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
2,703 951 92 3,746 184 127 159
  • HTML: 2,703
  • PDF: 951
  • XML: 92
  • Total: 3,746
  • Supplement: 184
  • BibTeX: 127
  • EndNote: 159
Views and downloads (calculated since 13 Jul 2018)
Cumulative views and downloads (calculated since 13 Jul 2018)

Viewed (geographical distribution)

Total article views: 3,746 (including HTML, PDF, and XML) Thereof 3,565 with geography defined and 181 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 07 Mar 2026
Download
Short summary
We study how the Earth's space environment responds to two different amplitude interplanetary coronal mass ejection (ICME) events that occurred in 2012 and 2014 by using the GUMICS-4 global MHD model. We examine local and large-scale dynamics of the Earth's space environment and compare simulation results to in situ data. It is shown that during moderate driving simulation agrees well with the measurements; however, GMHD results should be interpreted cautiously during strong driving.
Share