Laboratorio de Ionosfera, Atmosfera Neutra y Magnetosfera (LIANM), Facultad de Ciencias Exactas y Tecnología (FACET), Universidad Nacional de Tucumán (UNT), San Miguel de Tucumán, Argentina
Instituto de Física del Noroeste Argentino (CONICET-UNT), San Miguel de Tucumán, Argentina
Yamila Daniela Melendi
Departamento de Física, Universidad Nacional del Sur (UNS), Bahía Blanca, Argentina
Instituto de Física del Sur (CONICET-UNS), Bahía Blanca, Argentina
Tucumán Space Weather Center (TSWC), San Miguel de Tucumán, Argentina
Blas Federico de Haro Barbas
Laboratorio de Ionosfera, Atmosfera Neutra y Magnetosfera (LIANM), Facultad de Ciencias Exactas y Tecnología (FACET), Universidad Nacional de Tucumán (UNT), San Miguel de Tucumán, Argentina
Instituto de Física del Noroeste Argentino (CONICET-UNT), San Miguel de Tucumán, Argentina
Fernando Salvador Buezas
Departamento de Física, Universidad Nacional del Sur (UNS), Bahía Blanca, Argentina
Instituto de Física del Sur (CONICET-UNS), Bahía Blanca, Argentina
Ana Georgina Elias
Laboratorio de Ionosfera, Atmosfera Neutra y Magnetosfera (LIANM), Facultad de Ciencias Exactas y Tecnología (FACET), Universidad Nacional de Tucumán (UNT), San Miguel de Tucumán, Argentina
Instituto de Física del Noroeste Argentino (CONICET-UNT), San Miguel de Tucumán, Argentina
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Total article views: 3,254 (including HTML, PDF, and XML)
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Our research investigates how different proxies of solar activity influence long-term trends in the Earth's ionosphere. By analyzing data from two mid-latitude stations up to 2022, we found that the choice of solar activity measures significantly affects trends in ionospheric electron density, while trends in ionospheric height remain more stable. Selecting the correct solar activity measure is crucial for accurate density trend predictions and improving space weather forecasting models.
Our research investigates how different proxies of solar activity influence long-term trends in...
