Spatial Features of the Delayed Ionospheric Response During Low and High Solar Activity
Erik Schmölter,
Hanna Dühnen,
Jens Berdermann
et al.
Abstract:The ionospheric response to solar 27‐day signatures has complex temporal and spatial variations, which are driven by short‐ and long‐term changes of the solar activity among other processes (e.g., geomagnetic activity). A delay between these solar and ionospheric signatures occurs due to accumulation of plasma, which depends on the rates of photoionization, photodissociation and recombination in the upper atmosphere. The balance of these processes changes significantly at different solar activity levels. There… Show more
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