Articles | Volume 23, issue 4
https://doi.org/10.5194/npg-23-175-2016
https://doi.org/10.5194/npg-23-175-2016
Research article
 | Highlight paper
 | 
08 Jul 2016
Research article | Highlight paper |  | 08 Jul 2016

Multi-scale statistical analysis of coronal solar activity

Diana Gamborino, Diego del-Castillo-Negrete, and Julio J. Martinell

Viewed

Total article views: 5,507 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
4,195 1,028 284 5,507 226 296
  • HTML: 4,195
  • PDF: 1,028
  • XML: 284
  • Total: 5,507
  • BibTeX: 226
  • EndNote: 296
Views and downloads (calculated since 19 Jan 2016)
Cumulative views and downloads (calculated since 19 Jan 2016)

Cited

Latest update: 25 Apr 2024
Download
Short summary
We use temperature maps of the solar corona for three regions and use a technique that separates multiple timescales and space scales to show that the small-scale temperature fluctuations appear more frequently prior to the occurrence of a solar flare, in comparison with the same region after the flare and with a quiet region. We find that, during the flare, energy flows from large to small scales and heat transport associated with a heat front is convective along and diffusive across the front.