Articles | Volume 43, issue 1
https://doi.org/10.5194/angeo-43-201-2025
https://doi.org/10.5194/angeo-43-201-2025
Regular paper
 | 
31 Mar 2025
Regular paper |  | 31 Mar 2025

Effects of supernova-induced soft X-rays on middle- and upper-atmospheric nitric oxide and stratospheric ozone

David E. Siskind, McArthur Jones Jr., and Jeffrey W. Reep

Viewed

Total article views: 3,753 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
2,983 349 421 3,753 185 257
  • HTML: 2,983
  • PDF: 349
  • XML: 421
  • Total: 3,753
  • BibTeX: 185
  • EndNote: 257
Views and downloads (calculated since 11 Sep 2024)
Cumulative views and downloads (calculated since 11 Sep 2024)

Viewed (geographical distribution)

Total article views: 3,753 (including HTML, PDF, and XML) Thereof 3,712 with geography defined and 41 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Dec 2025
Download
Short summary
This study tests a recent suggestion that multi-month soft X-ray emissions from supernovae can destroy planetary ozone layers. To test this, we assume a year-long solar flare and evaluate the production of nitric oxide in the upper atmosphere and its transport down to the stratosphere. Our results suggest widespread catalytic destruction of ozone; however, these effects are limited to the upper edge of the ozone layer (near 40 km). Thus, the total column is only slightly affected (1–2 %).
Share