Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/15201
Authors: Scotto, Carlo* 
Sabbagh, Dario* 
Title: Climatology of Spread F over Tucumán from Massive Statistical Analysis of Autoscaled Data
Journal: Atmosphere 
Series/Report no.: /12 (2021)
Publisher: MDPI
Issue Date: 2021
DOI: 10.3390/atmos12101351
URL: https://www.mdpi.com/2073-4433/12/10/1351
Keywords: equatorial spread F (ESF); ionosonde; ionograms; automatic scaling
Subject ClassificationSpread F climatology at equatorial latitudes from ionosonde data (statistic limited to the ionospheric station of Tucuman)
Abstract: Automatic ionogram interpretation methods developed for real-time ionospheric monitoring can be applied in retrospective studies to analyze large quantities of data. The Autoscala software, implemented for such a purpose, includes a routine for automatic detection of diffused echoes known as spread F, which appear in ionograms due to the presence of ionospheric irregularities along the radio signal path. The main objective of this routine is to reject bad quality ionograms. This new capability was used in a climatological study including a large number of ionograms recorded at the low-latitude ionospheric station of Tucumán (26.9° S, 294.6° E, magnetic latitude 15.5° S, Argentina). The study took into account different levels of geomagnetic and solar activity from 2012 to 2020. The results demonstrate the capability of Autoscala to capture the main signature characteristics of spread F and the temporal evolution of the ionosphere peak heigh hmF2, capturing the post-sunset plasma surge that precedes development of spread F. Maximum occurrence of spread F is observed in local summer, with a tendency to shift before midnight with increasing solar activity. Other new climatological details that emerged from the study are illustrated and briefly discussed, dealing with connection with geomagnetic activity, and morning hmF2 behavior after extremely marked nighttime spread F occurrence.
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