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- W4310256087 abstract "The D-region ionosphere is sluggish in nature while responding to the incoming solar radiation. We study the altitude ( h ) profile of mid-latitude D-region response time delay (Δ t ) during three chosen solar flares, namely, C5.2, M5.2, and X2.2 classes. We solve “electron continuity equation” numerically at each and every h to obtain Δ t - h profile. We investigate the 1) latitudinal variation (over both Northern and Southern hemispheres) and 2) seasonal variation (throughout the year) of Δ t - h profiles of each of these solar flares separately. We go over noteworthy variations of Δ t - h profile for both 1) and 2) with reasonably different results over different hemispheres. Also, we study some contrasting behaviours of Δ t - h profile of X2.2 class for both 1) and 2) in comparison to C5.2 or M5.2 classes. We conclude the outcome with possible explanations." @default.
- W4310256087 created "2022-11-30" @default.
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- W4310256087 date "2022-11-28" @default.
- W4310256087 modified "2023-10-16" @default.
- W4310256087 title "On the altitude profile of lower ionospheric D-region response time delay during solar flares" @default.
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- W4310256087 doi "https://doi.org/10.3389/fenvs.2022.1020137" @default.
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