D.C. Ndiitwani

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The propagation of ultra low frequency (ULF) waves, in the frequency range of 1-100 mHz, from the mag- netosphere to the ground where they are usually detected is greatly affected by the Earth¿s ionosphere. The ionosphere presents a conducting interface between the magnetosphere and atmosphere. In this work magnetic field measurements observed in the(More)
Galactic cosmic rays are charged particles created in our galaxy and beyond. They propagate through interstellar space to eventually reach the heliosphere and Earth. Their transport in the heliosphere is subjected to four modulation processes: diffusion, convection, adiabatic energy changes and particle drifts. Time-dependent changes, caused by solar(More)
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