From Bobik et al. (2011): Comparison of Antiproton over proton ratio at 1AU
From Bobik et al (2012): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 23
From Boschini et al (2018a): 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.
From Boschini et al (2017a): 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.
From Boschini et al. (2018b): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 24 for Carbon and Oxygen. Modulated B/C and He/O ratio.
From Boschini et al. (2017): Forcast of protons and helium nuclei cosmic rays differential intensity up to the end of 2020:
From Spacemon, ESTEC, Dec 13-15 (2017): example of Helmod application on SREM detectors and ACE/CRIS.
From Boschini et al. (2019): Modulated Galactic Cosmic rays differential intensity at 1 AU during solar cycle 23 and 24 for Proton, Heliumm, Electron, Carbon and Oxygen. Modulated Galactic Cosmic rays differential intensity along Voyager probes trajectory. Proton over Helium, Carbon over Helium, Carbon over oxygen ratio along the solar cycles 23 and 24.
From Boschini et al. (2020): Modulated Galactic Cosmic rays differential intensity for Lithium, Beryllium, Boron and Nitrogen. Boron over Carbon ratio along the solar cycles 23 and 24.
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.
From Bobik et al. (2013): latitudinal gradients in the inner heliosphere
From Boschini et al (2018): Solar Modulation applied to Electron spectrum for AMS-02, PAMELA and Ulysses
From Bobik et al (2013): latitudinal relative galactic cosmic rays intensity along the ulysses orbit.
