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HelMod-4

The Heliospheric Modulation Model

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Proton High AMS02 small

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 (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. 

BoschiniEtAl AdvSR Fig4BoschiniEtAl AdvSR Fig5BoschiniEtAl AdvSR Fig6BoschiniEtAl AdvSR Fig7BoschiniEtAl AdvSR Fig8

 

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.

BoschiniEtAl ApJ2017 Fig6BoschiniEtAl ApJ2017 Fig7BoschiniEtAl ApJ2017 Fig8BoschiniEtAl ApJ2017 Fig9BoschiniEtAl ApJ2017 Fig11BoschiniEtAl ApJ2017 Fig12BoschiniEtAl ApJ2017 Fig14

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.

Apj2018b fig4

Apj2018b fig5

Apj2018b fig6

Apj2018b fig8

From Boschini et al. (2017): Forcast of protons and helium nuclei cosmic rays  differential intensity up to the end of 2020:

 

 IAUSymp2017 a

IAUSymp2017 b

 

 

From Spacemon, ESTEC, Dec 13-15 (2017): example of Helmod  application on SREM detectors and ACE/CRIS.

SPACEMON HelMod Rosetta 2017 12 14 a

SPACEMON HelMod Rosetta 2017 12 14 b

 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.

AsvSR2019 fig1

 

AsvSR2019 fig6

AsvSR2019 fig7

AsvSR2019 fig8

AsvSR2019 fig9

AsvSR2019 fig10 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.

ApJ2020a Fig1

ApJ2020a Fig4ApJ2020a Fig5 ApJ2020a Fig10

 

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 Boschini et al (2018): Solar Modulation applied to Electron spectrum for AMS-02, PAMELA and Ulysses

Apj2018 ElectronPaper 1

ApJ2018 ElectronPaper 2

ApJ2018 ElectronPaper 3

 

 

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

ICRC2013 fig1ICRC2013 fig2