Napkitörések alsó ionoszférára gyakorolt hatásának vizsgálata ionoszonda adatok segítségével(141967)
Funder: NKFIH
Űridőjárási események ionoszférikus hatásának vizsgálata közepes szélességeken(BO/00461/21)
Funder: Bolyai János Kutatási Ösztöndíj
As a result of the enhanced X-ray and EUV fluxes following large solar flares, the
electron density of the ionospheric layers increases. Furthermore, it causes higher
absorption or even partial or total fade-out of the emitted radio waves which can
be measured with ionosondes and Digisondes by studying the amplitude of the reflected
electromagnetic waves [1,2].
In the present study, the ionospheric response to large solar flares has been investigated
using the ionosonde data measured at the Průhonice (Czech Republic, 49.98° N, 14.55°
E) and San Vito (Italy, 40.6° N, 17.8° E) stations 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). Furthermore, the signal-to-noise ratio (SNR) measured by the Digisondes
was used as well to quantify and characterize the fade-out events and the ionospheric
absorption. The combination of these three 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