Statistical error for cosmic rays modulation evaluation by 1D and 2D models

Video Player is loading.
Loaded: 0%
Remaining Time 0:00
1x
  • Quality
    • 67 views

    • 0 favorites

    • uploaded July 5, 2021

    Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 18:00
    ZOOM-Meeting URL: https://icrc2021.desy.de/pf_access_abstracts
    Corresponding Session: https://icrc2021-venue.desy.de/channel/Presenter-Forum-1-Evening-All-Categories/48
    Abstract:
    "The propagation of cosmic rays through the heliosphere is solved for more than half a century by stochastic methods based on Ito's lemma. This work presents the estimation of statistical error of solution of Foker – Plank equation by 1D forward stochastic differential equations method. rnrnThe error dependence on simulation statistics and energy is presented for different combinations of input parameters. The 1% precision criterium in intensities and 1% criterium in standard deviation are defined as a function of solar wind velocity and diffusion coefficient value. The implications for 1D backward and 2D models are also discussed."

    Authors: Viacheslav Mykhailenko | Pavol Bobík
    Indico-ID: 451
    Proceeding URL: https://pos.sissa.it/395/1325

    Tags:
    Presenter:

    Viacheslav Mykhailenko


    Additional files

    More Media in "Solar & Heliospheric"