EGU24-16216, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-16216
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The extreme geomagnetic storm on 13–15 May 1921: a study based on hourly means, including observations at Stará Ďala (Hurbanovo)

Eduard Koči1,2 and Fridrich Valach2
Eduard Koči and Fridrich Valach
  • 1Slovak Central Observatory Hurbanovo, Publishing Department, Slovakia (quazy80@gmail.com)
  • 2Geomagnetic Observatory, Earth Science Institute, Slovak Academy of Sciences, Hurbanovo, Slovakia

The magnetic storm that occurred in May 1921 ranks among the most extreme events ever observed by magnetic observatories. Some parts of this storm were also recorded in declination and vertical intensity by the variation station at the Stará Ďala observatory (present-day Hurbanovo in Slovakia). However, the magnetogram on photographic paper for this event not only contained data gaps, it also did not have a marked timeline, and the values of the divisions for the geomagnetic elements were not known. We identified timestamps using global variations observed by other observatories and estimated the values of the divisions based on data from before and after the studied event. Then, the magnetograms were digitized. To interpret the obtained data, we compared them with hourly averages from other observatories in different parts of the globe. Our results seem to confirm the expected assumption that, in the morning hours of 15 May 1921, the equatorward boundary of the auroral oval extended to the European mid-latitude observatories.

How to cite: Koči, E. and Valach, F.: The extreme geomagnetic storm on 13–15 May 1921: a study based on hourly means, including observations at Stará Ďala (Hurbanovo), EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-16216, https://doi.org/10.5194/egusphere-egu24-16216, 2024.