Diurnal variations in characteristics of sporadic layer Eₛ over Irkutsk

We have studied the morphological features of semidiurnal variations in the occurrence of the sporadic Es layer (PEs) and height of the layer (hEs), using data from the Irkutsk DPS-4 ionosonde (52.3° N, 104.3° E) for 2003–2021. By averaging over all the years, we calculate diurnal variations in PEs and hEs for each month. It is observed that the maximum of occurrence PEs is achieved when the height hEs decreases; and there is an asymmetry in the maximum of occurrence PEs: morning maxima are larger than evening ones. These features are interpreted based on the concept of the optimal height for Es formation and the role of photoionization in forming the sporadic layer.

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Publication Details

Journal
Solnechno-Zemnaya Fizika
Published
2025-03-26
DOI
https://doi.org/10.12737/szf-111202507
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Diurnal variations in characteristics of sporadic layer Eₛ over Irkutsk

Konstantin Ratovsky, Ekaterina Voronova
Solnechno-Zemnaya Fizika
Solar and Space Plasma Dynamics
article

Diurnal variations in characteristics of sporadic layer Eₛ over Irkutsk

Konstantin Ratovsky, Ekaterina Voronova
article en

Abstract

We have studied the morphological features of semidiurnal variations in the occurrence of the sporadic Es layer (PEs) and height of the layer (hEs), using data from the Irkutsk DPS-4 ionosonde (52.3° N, 104.3° E) for 2003–2021. By averaging over all the years, we calculate diurnal variations in PEs and hEs for each month. It is observed that the maximum of occurrence PEs is achieved when the height hEs decreases; and there is an asymmetry in the maximum of occurrence PEs: morning maxima are larger than evening ones. These features are interpreted based on the concept of the optimal height for Es formation and the role of photoionization in forming the sporadic layer.

Solnechno-Zemnaya Fizika
Institute of Solar-Terrestrial Physics (RU)
Openalex Percentile: Top 95%
Solar and Space Plasma Dynamics
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