Abstract
The rates of ion production and loss processes in the lower ionosphere during solar and other astronomical ionizing events vary with height. This variations influence the time lags of the response in different ionospheric layers. Very Low Frequency (VLF) signals reflected from any of these layers follow this time lag or delay during a transient cosmic events. One of the easiest ways to study this property is to observe the shift in the peak of VLF signal amplitude with respect to the peak of solar flares. We numerically model to find ion densities and resulting VLF signal perturbations during some solar flares. We clearly find from the model that the delay in the peak of the electron densities (with respect to peak of the ionizing event) in the lower ionosphere varies from height to height. The result also depends on the properties of events, such as peak intensity and sharpness. We investigate analytically how the delay of electron density peak should depend on height varying chemical rate parameters as well as the nature of transient events. Our capability is demonstrated using three classes (namely, X, M and C) of solar flares. The work is a step forward in our goal to employ ionosphere as a natural detector for astronomical observations.
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Sourav Palit and Sujay Pal acknowledge a grant from MoES for financial support.
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Palit, S., Basak, T., Pal, S. et al. Theoretical study of lower ionospheric response to solar flares: sluggishness of D-region and peak time delay. Astrophys Space Sci 356, 19–28 (2015). https://doi.org/10.1007/s10509-014-2190-6
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DOI: https://doi.org/10.1007/s10509-014-2190-6