From Bobik et al. (2011): Comparison of Antiproton over proton ratio at 1AU

ASTRA2011 Fig2 3

From Bobik et al (2012): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 23

ApJ2012 Fig4 5ApJ2012 Fig7 8ApJ2012 Fig9 10

From Boschini et al (2017a): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 23 and 24 for Proton, Helium. Differential Intensity for PAMELA. Ratio between Proton and Helium in Bartel Rotation. Helium normalized counting rate measuered by Ulysses. 

BoschiniEtAl AdvSR Fig4BoschiniEtAl AdvSR Fig5BoschiniEtAl AdvSR Fig6BoschiniEtAl AdvSR Fig7BoschiniEtAl AdvSR Fig8

From Boschini et al (2017b): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 23 and 24 for Proton, Helium and Antiproton. Proton normalized counting rate measuered by Ulysses.

BoschiniEtAl ApJ2017 Fig6BoschiniEtAl ApJ2017 Fig7BoschiniEtAl ApJ2017 Fig8BoschiniEtAl ApJ2017 Fig9BoschiniEtAl ApJ2017 Fig11BoschiniEtAl ApJ2017 Fig12BoschiniEtAl ApJ2017 Fig14BoschiniEtAl ApJ2017 Fig15

 

 

From Della Torre et al. (2012): Magnetic drift effect for a typical sola minimum on electron and positron (opposite charge sign). Experimental effect on positron fraction in two consecutive solar minima of opposite magentic field polarity.

AdvSR2012 fig1AdvSR2012 fig5

From Bobik et al. (2013): latitudinal gradients in the inner heliosphere

AdvAstr2013 fig2

 

 From Bobik et al (2013): latitudinal relative galactic cosmic rays intensity along the ulysses orbit.

ICRC2013 fig1ICRC2013 fig2