EGU21-7756, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-7756
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Seasonal behavior of H component during solar cycle 24

Yasmina Bouderba, Ener Aganou, and Abdenaceur Lemgharbi
Yasmina Bouderba et al.
  • Center of Research on Astronomy, Astrophysics and Geophysics (CRAAG), Tamanrasset, Algeria (yasminabdb@hotmail.com)

In this work we will show the behavior of the horizontal component H of the Earth Magnetic Field (EMF) along the seasons during the period of solar cycle 24 lasting from 2009 to 2019. By means of  continuous measurements of geomagnetic components (X, Y) of the EMF, we compute the horizontal component H at the Earth’s surface. The data are recorded with a time resolution of one minute at Tamanrasset observatory in Algeria at the geographical coordinates of 22.79° North and 5.53° East. These data are available from the INTERMAGNET network. We find that the variation in amplitude of the hourly average of H component at low latitude changes from a season to another and it is greater at the maximum solar activity than at the minimum solar activity.

Keywords: Solar cycle 24, Season, Horizontal component H. 

How to cite: Bouderba, Y., Aganou, E., and Lemgharbi, A.: Seasonal behavior of H component during solar cycle 24, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-7756, https://doi.org/10.5194/egusphere-egu21-7756, 2021.

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