MAGNETOSPHERIC DISTURBANCES IN GNEVYSHEV GAPS: CASE OF SOLAR CYCLES 20 TO 24

Journal: International Journal of Advanced Research (Vol.12, No. 12)

Publication Date: 2024-12-18

Authors : Inza GNANOU Salfo KABORE Moustapha KONATE Abdoul Fatao CISSE Christian ZOUNDI Frederic OUATTARA;

Page : 459-468

Keywords : High-Speed Solar Wind Gnevyshev Gaps Interplanetary Magnetic Field Magnetospheric Convection Field Geomagnetic Activity;

Source : Download Find it from : Google Scholar

Abstract

Time dependence of many solar activity factors and related phenomena shows a highest double-peak structure around sunspot maximum during the maximum phase of the 11-year solar cycle. Highly variable conditions on the Sun persist throughout the phase maximum of solar activity.

Main Menu

Searching By

PARTNERS

MAGNETOSPHERIC DISTURBANCES IN GNEVYSHEV GAPS: CASE OF SOLAR CYCLES 20 TO 24

Abstract

Advertisement