Modeling of the cold electron plasma density for radiation belt physics

被引:7
|
作者
Ripoll, J. -F. [1 ,2 ]
Pierrard, V. [3 ,4 ,5 ]
Cunningham, G. S. [6 ]
Chu, X. [7 ]
Sorathia, K. A. [8 ]
Hartley, D. P. [9 ]
Thaller, S. A. [10 ]
Merkin, V. G. [8 ]
Delzanno, G. L. [11 ]
De Pascuale, S.
Ukhorskiy, A. Y. [8 ]
机构
[1] CEA, DAM, DIF, Bruyeres LeChatel, France
[2] CEA, UPS, LMCE, Bruyeres LeChatel, France
[3] Royal Belgian Inst Space Aeron, STCE & Space Phys, Brussels, Belgium
[4] Univ Catholique Louvain UCLouvain, Ctr Space Radiat CSR, Louvain La Neuve, Belgium
[5] Earth & Life Inst ELI, Georges Lemaitre Ctr Earth & Climate Res TECLIM, Louvain La Neuve, Belgium
[6] Los Alamos Natl Lab, Space Sci & Applicat Grp, Los Alamos, NM USA
[7] Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO USA
[8] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[9] Univ Iowa, Dept Phys & Astron, Iowa City, IA USA
[10] Orion Space Solut, Louisville, CO USA
[11] Los Alamos Natl Lab, Theoret Div, Los Alamos, NM USA
基金
欧盟地平线“2020”; 美国国家科学基金会;
关键词
electron density; plasmasphere; plasmapause; empirical models; physical models; machine learning; radiation belts; INTERNATIONAL REFERENCE IONOSPHERE; HISS WAVE POWER; SOLAR-WIND; SAMI3-RCM SIMULATION; GEOMAGNETIC-ACTIVITY; EARTHS PLASMASPHERE; WHISTLER; STORM; MAGNETOSPHERE; DYNAMICS;
D O I
10.3389/fspas.2023.1096595
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This review focusses strictly on existing plasma density models, including ionospheric source models, empirical density models, physics-based and machine-learning density models. This review is framed in the context of radiation belt physics and space weather codes. The review is limited to the most commonly used models or to models recently developed and promising. A great variety of conditions is considered such as the magnetic local time variation, geomagnetic conditions, ionospheric source regions, radial and latitudinal dependence, and collisional vs. collisionless conditions. These models can serve to complement satellite observations of the electron plasma density when data are lacking, are for most of them commonly used in radiation belt physics simulations, and can improve our understanding of the plasmasphere dynamics.
引用
收藏
页数:18
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