Influence of geomagnetic activity on mesopause temperature over Yakutia

• Published in: Atmospheric Chemistry and Physics
• Main Authors: Gavrilyeva, Galina, Ammosov, Petr
• Format: Article in Journal/Newspaper
• Language: English
• Published: Copernicus Publications 2018
• Subjects: article; Verlagsveröffentlichung; Yakutia
• Online Access: https://doi.org/10.5194/acp-18-3363-2018; https://noa.gwlb.de/receive/cop_mods_00041904; https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00041524/acp-18-3363-2018.pdf; https://acp.copernicus.org/articles/18/3363/2018/acp-18-3363-2018.pdf

The long-term temperature changes of the mesopause region at the hydroxyl molecule OH (6-2) nighttime height and its connection with the geomagnetic activity during the 23rd and beginning of the 24th solar cycles are presented. Measurements were conducted with an infrared digital spectrograph at the Maimaga station (63∘ N, 129.5∘ E). The hydroxyl rotational temperature (TOH) is assumed to be equal to the neutral atmosphere temperature at the altitude of ∼ 87 km. The average temperatures obtained for the period 1999 to 2015 are considered. The season of observations starts at the beginning of August and lasts until the middle of May. The maximum of the seasonally averaged temperatures is delayed by 2 years relative to the maximum of the solar radio emission flux (wavelength of 10.7 cm), and correlates with a change in geomagnetic activity (Ap index). Temperature grouping in accordance with the geomagnetic activity level showed that in years with high activity (Ap > 8), the mesopause temperature from October to February is about 10 K higher than in years with low activity (Ap < = 8). Cross-correlation analysis showed no temporal shift between geomagnetic activity and temperature. The correlation coefficient is equal to 0.51 at the 95 % level.