Archimedean Spiral Distribution of Energetic Particles in Earth's Inner Radiation Belt

被引:3
作者
Sun, Weiqin [1 ,2 ]
Yang, Jian [2 ]
Wang, Wenrui [2 ]
Cui, Jun [1 ]
Toffoletto, Frank [3 ]
Yue, Chao [4 ]
Gkioulidou, Matina [5 ]
Gerrard, J. Andrew [6 ]
机构
[1] Sun Yat sen Univ, Sch Atmospher Sci, Zhuhai, Peoples R China
[2] Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen, Peoples R China
[3] Rice Univ, Dept Phys & Astron, Houston, TX USA
[4] Peking Univ, Inst Space Phys & Appl Technol, Beijing, Peoples R China
[5] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[6] New Jersey Inst Technol, Ctr Solar Terr Res, Newark, NJ USA
基金
中国国家自然科学基金;
关键词
archimedean spiral structures; ELECTRON ZEBRA STRIPES; MODEL; EVOLUTION;
D O I
10.1029/2023GL106859
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Archimedean spirals are common in various fields such as biology, engineering, astronomy, and space physics. Here we report the discovery of patterns resembling the general Archimedean spirals in particle distributions in the Earth radiation belt. Our analytic theory and numerical simulations demonstrate that electrons with initially asymmetric spatial distributions form such spirals in the inner magnetosphere, where particles at smaller radial distances move more slowly in angular velocity. These spirals result in time-varying peaks and valleys in particle fluxes, referred to as "zebra stripes," which are well consistent with Van Allen Probes measurements. Although the initial asymmetric distribution may be seeded by the electric field in the magnetosphere, the spiral formation does not require them. Furthermore, we show that, due to the same fundamental motion of charged particles in regions dominated by dipole fields, this spiral phenomenon may also appear in the proton distributions, as well as in planetary magnetospheres. The Archimedean spiral is named after the 3rd-century BC Greek mathematician Archimedes. Such spirals have been seen from the sunflower head, Iridogorgia to galactic arms. Throughout the solar system, the average configuration of the background magnetic field also aligns with Archimedean spirals, as it is dragged by charged particles that are ejected radially from the surface of the rotating Sun, a fundamental discovery made by E. N. Parker. However, it remains unknown whether an Archimedean spiral exists in the near-Earth space. Here we report for the first time the discovery of patterns similar to the general Archimedean spirals in particle distributions in the radiation belt, a region filled with energetic charged particles surrounding Earth. This happens because electrons closer to the Earth move slower in the angular direction. These spirals manifest as time-varying peaks and valleys in the electron spectagrams, named as "zebra stripes." Our theory and simulation results are well consistent with the measurements of the Van Allen Probes. Besides, our theory predicts that these spirals could occur on protons and other planets with similar magnetic fields. The first known discussion and discovery of Archimedean spiral structures in Earth's magnetosphere Electrons' general Archimedean spiral-like distribution results in the formation of "zebra stripes" in the inner radiation belt Our findings hold exciting implications for understanding magnetospheric physics beyond our planet
引用
收藏
页数:10
相关论文
共 45 条
  • [1] The GALAH survey and Gaia DR2: dissecting the stellar disc's phase space by age, action, chemistry, and location
    Bland-Hawthorn, Joss
    Sharma, Sanjib
    Tepper-Garcia, Thor
    Binney, James
    Freeman, Ken C.
    Hayden, Michael R.
    Kos, Janez
    De Silva, Gayandhi M.
    Ellis, Simon
    Lewis, Geraint F.
    Asplund, Martin
    Buder, Sven
    Casey, Andrew R.
    D'Orazi, Valentina
    Duong, Ly
    Khanna, Shourya
    Lin, Jane
    Lind, Karin
    Martell, Sarah L.
    Ness, Melissa K.
    Simpson, Jeffrey D.
    Zucker, Daniel B.
    Zwitter, Tomaz
    Kafle, Prajwal R.
    Quillen, Alice C.
    Ting, Yuan-Sen
    Wyse, Rosemary F. G.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 486 (01) : 1167 - 1191
  • [2] Comprehensive computational model of Earth's ring current
    Fok, MC
    Wolf, RA
    Spiro, RW
    Moore, TE
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2001, 106 (A5) : 8417 - 8424
  • [3] AE9, AP9 and SPM: New Models for Specifying the Trapped Energetic Particle and Space Plasma Environment
    Ginet, G. P.
    O'Brien, T. P.
    Huston, S. L.
    Johnston, W. R.
    Guild, T. B.
    Friedel, R.
    Lindstrom, C. D.
    Roth, C. J.
    Whelan, P.
    Quinn, R. A.
    Madden, D.
    Morley, S.
    Su, Yi-Jiun
    [J]. SPACE SCIENCE REVIEWS, 2013, 179 (1-4) : 579 - 615
  • [4] The Formation of Saturn's and Jupiter's Electron Radiation Belts by Magnetospheric Electric Fields
    Hao, Yi-Xin
    Sun, Yi-Xin
    Roussos, Elias
    Liu, Ying
    Kollmann, Peter
    Yuan, Chong-Jing
    Krupp, Norbert
    Paranicas, Chris
    Zhou, Xu-Zhi
    Murakami, Go
    Kita, Hajime
    Zong, Qiu-Gang
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2020, 905 (01)
  • [5] Very-Low-Frequency transmitters bifurcate energetic electron belt in near-earth space
    Hua, Man
    Li, Wen
    Ni, Binbin
    Ma, Qianli
    Green, Alex
    Shen, Xiaochen
    Claudepierre, Seth G.
    Bortnik, Jacob
    Gu, Xudong
    Fu, Song
    Xiang, Zheng
    Reeves, Geoffrey D.
    [J]. NATURE COMMUNICATIONS, 2020, 11 (01)
  • [6] Modeling the Electron Flux Enhancement and Butterfly Pitch Angle Distributions on L Shells <2.5
    Hua, Man
    Li, W.
    Ma, Qianli
    Ni, Binbin
    Nishimura, Yukitoshi
    Shen, Xiao-chen
    Li, Haimeng
    [J]. GEOPHYSICAL RESEARCH LETTERS, 2019, 46 (20) : 10967 - 10976
  • [7] Simulated Prompt Acceleration of Multi-MeV Electrons by the 17 March 2015 Interplanetary Shock
    Hudson, Mary
    Jaynes, Allison
    Kress, Brian
    Li, Zhao
    Patel, Maulik
    Shen, Xiao-Chen
    Thaller, Scott
    Wiltberger, Michael
    Wygant, John
    [J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2017, 122 (10) : 10036 - 10046
  • [8] ARCHIMEDES SPIRAL AND THE SURFACE DISTRIBUTION OF DARK CLOUDS IN M31 .3.
    ISSA, IA
    [J]. ASTROPHYSICS AND SPACE SCIENCE, 1991, 184 (02) : 227 - 234
  • [9] Kaiser J., 1960, IRE Transactions on Antennas and Propagation, V8, P312, DOI DOI 10.1109/TAP.1960.1144840
  • [10] The large-scale nebular pattern of a superwind binary in an eccentric orbit
    Kim, Hyosun
    Trejo, Alfonso
    Liu, Sheng-Yuan
    Sahai, Raghvendra
    Taam, Ronald E.
    Morris, Mark R.
    Hirano, Naomi
    Hsieh, I-Ta
    [J]. NATURE ASTRONOMY, 2017, 1 (03):