EGU2020-2924
https://doi.org/10.5194/egusphere-egu2020-2924
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Studying the ionospheric absorption during large solar flare events in September 2017

Attila Buzas1,2, Veronika Barta1, and Daniel Kouba3
Attila Buzas et al.
  • 1Geodetic and Geophysical Institute, Sopron, Hungary (atteus645@gmail.com)
  • 2Doctoral School of Earth Sciences, Eötvös Loránd University, Budapest, Hungary
  • 3Institute of Atmospheric Physics, Czech Academy of Sciences, Prague, Czech Republic

The most intense external force affecting the ionosphere from above is related to large solar flare events, therefore it is of particular importance to study their impact on the ionosphere. During solar flares, the suddenly increased radiation causes increased ionization and enhanced absorption of radio waves leading to partial or even total radio fade-out lasting for hours in some cases (e. g. [1] [2]).

 

The ionospheric response to large solar flares have been investigated using the ionosonde data measured at Pruhonice (PQ052, 50°, 14.5°) in September 2017, the most active solar period of Solar Cycle 24. A novel method [3] to calculate and investigate the absorption of radio waves propagating in the ionosphere is used to determine the absorption during large solar flare events (M and X class). Subsequently, the absorption data are compared with the indicators derived from the fmin method (fmin, the minimum frequency is considered as a qualitative proxy for the “nondeviative” radio wave absorption occurring in the D-layer). Total and partial radio fade-out and increased values (with 2-5 MHz) of the fmin parameter were experienced during and after the intense solar flares (> M3). The combination of these two methods may prove to be an efficient approach to monitor the ionospheric response to solar flares.

 

[1] Sripathi, S., Balachandran, N., Veenadhari, B., Singh, R., and Emperumal, K.: Response of the equatorial and low-latitude ionosphere to an intense X-class solar flare (X7/2B) as observed on 09 August 2011, J. Geophys. Res.-Space, 118, 2648–2659, 2013.

[2] Barta, V., Sátori, G., Berényi, K. A., Kis, Á., and Williams, E. (2019). Effects of solar flares on the ionosphere as shown by the dynamics of ionograms recorded in Europe and South Africa. Annales Geophysicae, Vol. 37, No. 4, pp. 747-761

[3] Sales, G. S., 2009, HF absorption measurements using routine digisonde data, Conference material, XII. International Digisonde Forum, University of Massachusetts

How to cite: Buzas, A., Barta, V., and Kouba, D.: Studying the ionospheric absorption during large solar flare events in September 2017, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-2924, https://doi.org/10.5194/egusphere-egu2020-2924, 2020

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