Annales Geophysicae
Annales Geophysicae
ANGEO
Articles | Volume 37, issue 5
Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-919-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Special issue:
https://doi.org/10.5194/angeo-37-919-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Articles | Volume 37, issue 5
Regular paper
 | 
09 Oct 2019
Regular paper |  | 09 Oct 2019

Wavelet analysis of the magnetotail response to solar wind fluctuations during HILDCAA events

Adriane Marques de Souza Franco, Ezequiel Echer, and Mauricio José Alves Bolzan

Viewed

Total article views: 1,695 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,028 616 51 1,695 44 44
  • HTML: 1,028
  • PDF: 616
  • XML: 51
  • Total: 1,695
  • BibTeX: 44
  • EndNote: 44
Views and downloads (calculated since 20 May 2019)
Cumulative views and downloads (calculated since 20 May 2019)

Viewed (geographical distribution)

Total article views: 1,695 (including HTML, PDF, and XML) Thereof 1,376 with geography defined and 319 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 

Cited

Latest update: 23 Apr 2024
Download
Short summary
The wavelet transform was employed in nine HILDCAA events for intervals in which the Cluster crossed the magnetotail in order to identify the most energetic periods of these events in the magnetotail. It was seen that 76 % of the periods identified are ≤4 h. Using the cross wavelet analysis technique between Bz–IMF components and the Bx geomagnetic components, it was identified that the coupling of energy is stronger in periods between 2 and 4 h, which are typical substorm periods.
Read more
Special issue
7th Brazilian meeting on space geophysics and aeronomy