Articles | Volume 33, issue 1
https://doi.org/10.5194/angeo-33-25-2015
https://doi.org/10.5194/angeo-33-25-2015
Regular paper
 | 
07 Jan 2015
Regular paper |  | 07 Jan 2015

Physics of outflows near solar active regions

D. J. Price and Y. Taroyan

Viewed

Total article views: 1,357 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
784 536 37 1,357 54 51
  • HTML: 784
  • PDF: 536
  • XML: 37
  • Total: 1,357
  • BibTeX: 54
  • EndNote: 51
Views and downloads (calculated since 07 Jan 2015)
Cumulative views and downloads (calculated since 07 Jan 2015)

Cited

Latest update: 28 Mar 2024
Download
Short summary
Magnetic structures are important for studies of solar atmospheric heating. Combining computer simulations with observations of the Sun provides us with information not obtainable from pure observation. We use this to suggest and interpret the physical nature of a particular structure which is permeated by a continuous outflow of plasma. It is shown that the structure consists of multiple strands which undergo periodic heating and cooling.