Website latest update on October 13, 2021
The website will be not accessible on November 6th and 7th due to electrical maintenance
Welcome to the HelMod Website. In these pages you can find information about the Solar Modulation Model for the propagation of Galactic Cosmic Rays through the Heliosphere from the Termination shock down to Earth.
As advertised on the GALPROP website, HelMod website can be used as a a service package to seamlessly calculate the effects of the heliospheric modulation for GALPROP output files.
HelMod is a 2D Monte Carlo model to simulate the solar modulation of galactic cosmic rays. The model is based on the Parker transport equation which contains diffusion, convection, particle drift and energy loss. Following the evolution of the solar activity in time, we are able to modulate the local interstellar spectra (LIS) of cosmic ray species, assuming their isotropy beyond the termination shock, down to the Earth's location inside the heliosphere.
The current HelMod Version is the result from a continous development since 1998 (Monte-Carlo approach to Galactic Cosmic Ray propagation in the Heliosphere, Nucl. Phys B-Proc Sup). The latest review on HelMod was published in 2018 (Propagation of Cosmic Rays in Heliosphere: the HelMod Model. Adv. Space Res. 62(10):2859 - 2879, 2018)
In the present website version, a solar modulation calculator is available for Cosmic Rays experiments carried out during solar Cycle 23 and 24.
In the 2D-HelMod code version 1 was implemented the standard Parker field with modification in the polar region, the dependence on the particle drift, the Solar Wind description revisited for high and low activity periods, the Heliosphere divided in regions related to spatial propagation of turbulence from Sun, and, finally, it was introduced the possiblity to evaluate solar modulation for electrons and positrons.
From version 2 the heliospheric magnetic field and the spatial depenence of parallel diffusion coefficient evisited according to Ulysses measurements of time variation cosmic rays counting rate to accounts for different latitudinal gradients in opposite solar polarities
From version 3.0 The numerical scheme was revisited and a backward-in-time approach adopted. The rigidity dependence of parallel diffusion coefficient revisited according to PAMELA and AMS-02 data. Introduced the possibility of evaluate solar modulation of ions. Developed an additional python module to link GALPROP LIS (and plain text file) with HelMod results.
In HelMod, from version 3.5.0 it is implemented a forecasting capability for protons and ions fluxes, which will result in a better GCR flux estimation for future space missions (e.g., see asif website).
From version 4.0 the time dependent Termination Shock and Heliopause in included in the model.
Relevant result pictures from HelMod publications can be found in Results page.
This project is part of the activities on going at the sr-niel/ASIF/AMS-02 Milano-Bicocca (Italy) group and IEP-SAS space physic (Kosice, Slovakia). Local Interstellar Spectra (LISs) used in HelMod are those obtained from the join GalProp-HelMod effort.
Currently (see ASIF implementation agreements 2017-22-HD.0 ASI-ENEA, 2017-15-HD.0 ASI-INFN and ASIF implementation agreement involving ASI and Milano-Bicocca University), sr-niel, helmod and geomagsphere websites are supported within the space radiation environment activities of ASIF framework; their websevers are located in ASIF support center at the Physics Department of Milano-Bicocca University.