Abstract
The ‘tilt angle’ of the wavy current sheet in the hehosphere has been used very successfully as a proxy for solar activity in cosmic ray (CR) modulation models with particle drifts included. The “Hoeksema tilt angles α” are calculated using two potential field methods: (1) The classic ‘line-of-sight’ computation and (2) the more recent ‘radial’ photospheric field computation. The question of which set of ‘tilt angles’ is the more appropriate to use in modulation models is addressed by utilizing them in a comprehensive time-dependent drift model applied to the 22-year modulation cycle of 1.2 GeV cosmic ray electrons. We found that the ‘classic’ α are better suited than the ‘new’ α as a proxy for solar activity for periods of decreasing α and vice versa for periods of increasing α. By comparing the model with data it was shown that the set of α with the smallest rate of change over a period of decreasing or increasing solar activity provides the best compatibility with CR observations.
Published Version
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call