Non-thermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions

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Non-thermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions

Yao, X., Muñoz Sepúlveda, P. A., & Büchner, J. (2022). Non-thermal electron velocity distribution functions due to 3D kinetic magnetic reconnection for solar coronal plasma conditions. Physics of Plasmas, 29(2): 022104. doi:10.1063/5.0061151.

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Date of Discard: 2023-09-14

Comment: _Yao doppelt

Creators:
Yao, Xin¹
Muñoz Sepúlveda, Patricio A.¹
Büchner, Jörg¹

Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289

Dates: Published Online: 2022

Files: 0 Files

Locators: 0 Locators

version ID: item_3386838_1

Item State: Discarded

Name of Context: Publications of the MPI for Solar System Research, Affiliated to: Max Planck Institute for Solar System Research