Volume 444 -
38th International Cosmic Ray Conference (ICRC2023) -
Solar & Heliospheric Physics (SH)
The uniqueness of the Parker equation solution
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Pre-published on:
August 16, 2023
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Abstract
The Parker equation is widely used to describe the modulation of cosmic rays in the heliosphere. In this article, we present a test of the uniqueness of the solution of the Parker equation for 1D and 2D models of heliospheric modulation. Namely for the 1D B-p model and Geliosphere 2D model. The dependence of solution uniqueness on the selected model's input parameters is presented and discussed.
DOI: https://doi.org/10.22323/1.444.1274
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.