Speaker
Mr
Timothy Mohlolo
(North West University)
Abstract content <br> (Max 300 words)<br><a href="http://events.saip.org.za/getFile.py/access?resId=0&materialId=0&confId=34" target="_blank">Formatting &<br>Special chars</a>
This work studies modulation of galactic cosmic rays in the heliosphere by using a state-of-the-art, time dependent numerical modulation model to calculate cosmic ray transport inside the heliosphere. Results will be compared to different spacecraft observations, in particular observations from Voyager 1 and 2. It will be shown that when incorporating the most recent theoretical advances of the transport coefficients in such a model, which solve the Parker transport equation, that the model result in compatibility with spacecraft observations on a global scale.
Primary author
Mr
Timothy Mohlolo
(North West University)
Co-authors
Prof.
Marius Potgieter
(NWU)
Prof.
Stefan Ferreira
(NWU)