HONORE MESSANGA ETOUNDI

Dr. HONORE MESSANGA ETOUNDI

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Research Focus & Metrics

Academic Career Length

4Years (2023-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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5 December 2023 in Atmosphere
Verified
Journal Article
Open access
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PBP Baki
P Baki
BRBabatunde Rabiu
Babatunde Rabiu
Christine Amory-MazaudierChristine Amory-Mazaudier
Christine Amory-Mazaudier
RFRolland Fleury
Rolland Fleury
PCPierre Cilliers
Pierre Cilliers
JZJean-Louis Zerbo
Jean-Louis Zerbo
Space weather science has been a growing field in Africa since 2007. This growth in infrastructure and human capital development has been accompanied by the deployment of ground-based observing infrastructure, most of which was donated by foreign institutions or installed and operated by foreign establishments. However, some of this equipment is no longer operational due to several factors, which are examined in this paper. It was observed that there are considerable gaps in ground-based space-weather-observing infrastructure in many African countries, a situation that hampers the data acquisition necessary for space weather research, hence limiting possible development of space weather products and services that could help address socio-economic challenges. This paper presents the current status of space weather science in Africa from the point of view of some key leaders in this field, focusing on infrastructure, situation, human capital development, and the research landscape.

21 April 2025 in Space Weather
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Journal Article
Open access
PAPaul Obiakara AMAECHI
Paul Obiakara AMAECHI
HEHONORE MESSANGA ETOUNDI
HONORE MESSANGA ETOUNDI
FGFrank O. Grodji
Frank O. Grodji
AAAndrew Akala
Andrew Akala
IDIrina Despirak
Irina Despirak
Christine Amory-MazaudierChristine Amory-Mazaudier
Christine Amory-Mazaudier
We analyzed the solar origin and ground response during the severe geomagnetic storms (GSs) of 23–24 March (GS1) and 23–24 April 2023 (GS2) using Geomagnetically Induced Currents Indices (GIC indices) computed from geomagnetic field data. The GSs were initiated by erupting filaments and associated slow (fast) halo coronal mass ejections on 20 March (21 April) 2023. GS1 was also influenced by coronal hole high speed streams (CR HSSs) while substorm onsets drove the most intense GICX (GICY) of 86 (70) in Abisko, Sweden. GS2 was marked by strong negative Bz in a sheath and magnetic cloud with larger GIC indices of 84 (69) driven by magnetic pulsations, as evident at Abisko. This posed a moderate risk to power networks in Sweden. The threat however, reached only a low/moderate risk level in Boulder during the Sudden Impulse (SI)/main phase of GS1. For GS2, a low risk level was attained in Vernadsky and Eyrewell. As expected, at low latitude, GIC indices constituted a very low risk to ground infrastructures during both storms. The results also revealed longitudinal features with larger GIC indices in Boulder (Vernadsky) during the GS1 (GS2), and a North South Asymmetry characterized by a higher risk level in the northern (southern) hemisphere at the American longitude. Additionally, this study provides evidence that the equatorial electrojet can enhance GIC indices at the magnetic equator in the presence of sufficiently strong dH/dt. Finally, we relate GIC indices at high latitudes to the CR HSS on 23 March, and a magnetic cloud during the recovery phase on 24 April 2023.

22 June 2026 in Advances In Space Research
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Journal Article
Closed access
PAPaul Obiakara AMAECHI
Paul Obiakara AMAECHI
FGFranck O. Grodji
Franck O. Grodji
HEHONORE MESSANGA ETOUNDI
HONORE MESSANGA ETOUNDI
IDIrina Despirak
Irina Despirak
CNChigomezyo M. Ngwira
Chigomezyo M. Ngwira
JWJames M. Weygand
James M. Weygand