The influence of negative-ion changes in the D-region during sudden ionospheric disturbances

1973 ◽  
Vol 35 (3) ◽  
pp. 385-395 ◽  
Author(s):  
L Thomas ◽  
P.M Gondhalekar ◽  
M.R Bowman
2017 ◽  
Vol 122 (5) ◽  
pp. 5816-5824
Author(s):  
Yun Gong ◽  
Zheng Ma ◽  
Yanlin Li ◽  
Qihou Zhou ◽  
Shaodong Zhang ◽  
...  

1975 ◽  
Vol 18 (8) ◽  
pp. 806-809
Author(s):  
V. V. Belikovich ◽  
E. A. Benediktov ◽  
L. V. Grishkevich ◽  
V. A. Ivanov

1973 ◽  
Vol 35 (3) ◽  
pp. 397-404 ◽  
Author(s):  
L Thomas ◽  
P.M Gondhalekar ◽  
M.R Bowman

2021 ◽  
Vol 67 (1) ◽  
pp. 75-86
Author(s):  
Bakul Das ◽  
Shubham Sarkar ◽  
Prabir Kumar Haldar ◽  
Subrata Kumar Midya ◽  
Sujay Pal

2021 ◽  
Vol 11 (16) ◽  
pp. 7194
Author(s):  
Vladimir A. Srećković ◽  
Desanka M. Šulić ◽  
Ljubinko Ignjatović ◽  
Veljko Vujčić

Solar flares (SFs) and intense radiation can generate additional ionization in the Earth’s atmosphere and affect its structure. These types of solar radiation and activity create sudden ionospheric disturbances (SIDs), affect electronic equipment on the ground along with signals from space, and potentially induce various natural disasters. Focus of this work is on the study of SIDs induced by X-ray SFs using very low frequency (VLF) radio signals in order to predict the impact of SFs on Earth and analyze ionosphere plasmas and its parameters. All data are recorded by VLF BEL stations and the model computation is used to obtain the daytime atmosphere parameters induced by this extreme radiation. The obtained ionospheric parameters are compared with results of other authors. For the first time we analyzed physics of the D-region—during consecutive huge SFs which continuously perturbed this layer for a few hours—in detail. We have developed an empirical model of the D-region plasma density and gave a simple approximative formula for electron density.


2021 ◽  
Author(s):  
Paolo Redoblado ◽  
Sarwan Kumar ◽  
Abhikesh Kumar ◽  
Sushil Kumar

Abstract In this paper, we present the D-region ionospheric response during the lifespan (10–19 December 2020) of a severe category 5 tropical cyclone (TC) Yasa in the South Pacific by using the very low frequency (VLF, 3-30 kHz) signals from NPM, NLK, and JJI transmitters recorded at Suva, Fiji. Results indicate enhanced lightning and convective activity in all three regions (eyewall, inner rainbands, and outer rainbands) during the TC Yasa that are also linked to the wave sensitive zones of these transmitter-receiver great circle paths. Of the three regions, the outer rainbands showed the maximum lightning occurrence; hence convective activity. Prominent eyewall lightning was observed just before the TC started to weaken following its peak intensity. Analysis of VLF signal amplitudes showed both negative and positive perturbations (amplitudes exceeding ±3σ mark) lasting for more than 2 hours with maximum change in the daytime and nighttime signal amplitudes of -4.9 dB (NPM) and -19.8 dB (NLK), respectively. The signal perturbations were wave-like, exhibiting periods of oscillations between ~2.2-5.5 hours as revealed by the Morlet wavelet analysis. Additionally, the LWPC modeling of the signal perturbations indicated a 10 km increase in daytime D-region reference height, H¢, and a 12 km decrease in nighttime D-region H¢ during TC Yasa. The D-region density gradients (sharpness), b, showed small perturbations of 0.01–0.14 km-1 from its normal values. We suggest that the observed changes to the D-region parameters are due to the enhanced convection during TC Yasa which excites atmospheric gravity waves producing travelling ionospheric disturbances to the D-region.


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