C. Paizis et al., Rigidity dependence and time response of cosmic rays to the modulation steps in the rising part of Solar cycle 23. COSPIN/KET results, SPACE SCI R, 97(1-4), 2001, pp. 349-354
Previous work on the latitudinal gradient and on the amplitude of the recur
rent cosmic ray decreases, has shown that their magnitude does not decrease
monotonically with the particle rigidity, but it presents a broad maximun
around 1-2 GV. We have extended this analysis to study the behaviour of cos
mic-ray particles during the modulation steps in the rising part of the sol
ar activity of the present Solar cycle. We found that the `depth' of the mo
dulation step decreases monotonically with increasing rigidity and that the
least energetic particles are the last to reach their minimum intensity va
lue. We also considered in this analysis electrons of equal rigidity to stu
dy the influence of the charge sign on the particle behaviour during the mo
dulation steps.