Modeling Anomalous Transport of Cosmic Rays in the Heliosphere Using a Fractional Fokker–Planck Equation
Cosmic rays exhibit anomalous diffusion behaviors in the heliospheric environment that cannot be adequately described by classical diffusion models. In this paper, we develop a theoretical framework employing a fractional Fokker–Planck equation to model the anomalous transport of cosmic rays. This a...
Saved in:
| Main Author: | José Luis Díaz Palencia |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2025-01-01
|
| Series: | Fractal and Fractional |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2504-3110/9/1/24 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Thermoelastic Component of the Photoacoustic Response in a 3D-Printed Polyamide Coated with Pigment Dye: A Two-Layer Model Incorporating Fractional Heat Conduction Theories
by: Marica N. Popovic, et al.
Published: (2025-07-01) -
Adsorption–Desorption at Anomalous Diffusion: Fractional Calculus Approach
by: Ivan Bazhlekov, et al.
Published: (2025-06-01) -
Impact of Proton–Proton Collisions on the Cosmic-Ray Spectrum in Giant Clouds
by: Hao-Ran Ge, et al.
Published: (2025-01-01) -
Monogem’s Contribution to the Galactic Cosmic-Ray Spectrum
by: Xiang-Li Qian, et al.
Published: (2025-01-01) -
Cosmic ray propagation in a fractal galactic medium
by: Hamid Kermani, et al.
Published: (2011-01-01)