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Abstract: The Parallel and Perpendicular Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic fields Measured by Parker Solar Probe. (AGU25)

The Parallel and Perpendicular Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic fields Measured by Parker Solar Probe.

Nibuna Madam Subashchandar1, Lingling Zhao2, Andreas Shalchi3, Gary Paul Zank4, Jakobus Albertus le Roux5, Hui Li6, Xingyu Zhu7, Ashok Silwal8 and Juan Gabriel Alonso Guzmán8, (1)University of Alabama in Huntsville, Space Science, Huntsville, United States, (2)Center for Space Plasma and Aeronomic Research, Huntsville, United States, (3)University of Manitoba, Winnipeg, MB, Canada, (4)Univ of Alabama, Huntsville, Huntsville, United States, (5)The University of Alabama in Huntsville, Huntsville, AL, USA, Department of Space Science, Huntsville, United States, (6)Los Alamos National Lab, Los Alamos, United States, (7)University of Alabama in Huntsville, Department of Space Science, Huntsville, United States, (8)University of Alabama in Huntsville, Huntsville, AL, United States
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