A Signature of 27 day Solar Rotation in the Concentration of Metallic Ions within the Terrestrial Ionosphere

• Published in: The Astrophysical journal 2021-08, Vol.916 (2), p.106
• Main Authors: Yu, Bingkun, Scott, Christopher J., Xue, Xianghui, Yue, Xinan, Chi, Yutian, Dou, Xiankang, Lockwood, Mike
• Format: Article
• Language: English
• Subjects: Astrophysics; Coronal holes; E layer; Earth ionosphere; Geomagnetic activity; Ground-based observation; Ionosondes; Ionosphere; Ionospheric scintillation; Ions; Latitude; Metal concentrations; Oscillations; Periodicities; Solar corona; Solar cycle; Solar maximum; Solar minimum; Solar rotation; Solar wind; Solar wind velocity; Solar-terrestrial interactions; Terrestrial environments; Upper atmosphere; Wavelet analysis
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ac0886

We present observations during the interval 2006–2014 of 27 day and 13.5 day periodic oscillations in the ionospheric sporadic E (Es) layer. This is a thin, dense layer composed of metallic ions in the Earth’s upper atmosphere between 90 and 130 km. Lomb–Scargle spectral and wavelet analyses reveal that these pronounced periodicities observed from ground-based ionosondes and GPS/GNSS radio occultations are associated with high-speed solar winds generated from persistent coronal holes on successive 27 day solar rotations. The 27 day and 13.5 day oscillations in the Es layers are dependent on latitude, showing a higher magnitude of periodicities at low latitudes between 0° and 15° and at high latitudes between 45° and 90° (10%–14%) than those at midlatitudes between 15° and 45° (4%–10%). The 27 day and 13.5 day oscillations in the high-latitude Es layers correlate well with the geomagnetic activity Dst and Ap indices, and these periodic oscillations become more significant at the solar maximum (2000–2003 and 2011–2014) than at the solar minimum.