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Joshua, B. W., Adeniyi, J. O., Adimula, I. A., Oladipo, O. A., Olawepo, O. A., & Adebiyi, S. J. (2014). Ionospheric Response to the Storm-Time Disturbance of 29 May, 2010. Advances in Space Research, 53, 219-225.
https://doi.org/10.1016/j.asr.2013.11.003

has been cited by the following article:

• TITLE: Parameter Characterization of High Latitude Geomagnetic Storms in 2010

  AUTHORS: Ye Su

  KEYWORDS: Magnetic Storm, High Latitude, Temperature, Density

  JOURNAL NAME: Journal of Geoscience and Environment Protection, Vol.7 No.12, December 23, 2019

  ABSTRACT: Geomagnetic storm is a kind of severe disturbance that lasts for more than ten hours to several tens of hours in the entire Earth’s magnetosphere. This paper uses the NRLMSISE-00 model to calculate the temperature and density data. According to the surveyed medium magnetic storm events, the characteristics of daily average density and temperature in the occurrence of magnetic storms in 2010 were studied. At the same time, high latitude meridians were taken as research objects. Divide the temperature and density characteristics at different heights. Results showed that the annual trend of density is the same for different heights, and there is an average of the average density every day on the six medium magnetic storm mountains. For the average daily temperature, each medium magnetic storm event corresponds to a temperature peak. The peak temperature on April 5 was the highest temperature throughout the year, consistent with the annual average density distribution. Due to the intensity of the magnetic storm, the temperature of a large area of bright areas rose sharply on April 12, which is also the highest in the year. At 18:00 on May 2, it was the peak time of the moderate magnetic storm event caused by CIR, but May 3 was the date of the peak temperature. This peak delay is reasonable.