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• W2895219498 abstract "The ionosphere is an expansive natural detector and it characteristically reacts to ionizing influences coming from sun and other extraterrestrial energetic sources. In this article, first we give a brief review of earlier works performed specifically on Very Low Frequency (VLF) radio signal interaction with D-region ionosphere. Those are mainly related to the D-region ‘response time delay’ as experienced by VLF signal (△ t), effective recombination coefficient (αeff) and its connection with the D-region electron density (Ne) and other essential parameters during X-ray solar flares. Further, we present the measurement techniques and the observed results regarding the same time delay (△ t) experienced by VLF signal with respect to the X-ray flux variation of solar flares. Several research groups have developed many lower ionospheric models based on theoretical and experimental results to deal with those above mentioned quantities. We follow a rather simplified model proposed by J. Wait for D-region through the Long Wave Propagation Capability (LWPC) numerical code to estimate the Ne using flare induced amplitude-perturbation (△ A). Now, we use this △ t and Ne-profile for estimation of the effective recombination coefficient (αeff). Lastly, we analyse the results and conclude." @default.
• W2895219498 created "2018-10-12" @default.
• W2895219498 creator A5089290339 @default.
• W2895219498 date "2018-01-01" @default.
• W2895219498 modified "2023-09-27" @default.
• W2895219498 title "Quantitative Modeling of Lower Ionospheric Response Due to Solar X-ray Flare: A Propagating Radio Wave Simulation Approach" @default.
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• W2895219498 doi "https://doi.org/10.1007/978-3-319-94607-8_43" @default.
• W2895219498 hasPublicationYear "2018" @default.
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