Origin of two-band chorus in the radiation belt of Earth.


Journal

Nature communications
ISSN: 2041-1723
Titre abrégé: Nat Commun
Pays: England
ID NLM: 101528555

Informations de publication

Date de publication:
14 10 2019
Historique:
received: 15 03 2019
accepted: 09 09 2019
entrez: 16 10 2019
pubmed: 16 10 2019
medline: 16 10 2019
Statut: epublish

Résumé

Naturally occurring chorus emissions are a class of electromagnetic waves found in the space environments of the Earth and other magnetized planets. They play an essential role in accelerating high-energy electrons forming the hazardous radiation belt environment. Chorus typically occurs in two distinct frequency bands separated by a gap. The origin of this two-band structure remains a 50-year old question. Here we report, using NASA's Van Allen Probe measurements, that banded chorus waves are commonly accompanied by two separate anisotropic electron components. Using numerical simulations, we show that the initially excited single-band chorus waves alter the electron distribution immediately via Landau resonance, and suppress the electron anisotropy at medium energies. This naturally divides the electron anisotropy into a low and a high energy components which excite the upper-band and lower-band chorus waves, respectively. This mechanism may also apply to the generation of chorus waves in other magnetized planetary magnetospheres.

Identifiants

pubmed: 31611553
doi: 10.1038/s41467-019-12561-3
pii: 10.1038/s41467-019-12561-3
pmc: PMC6791895
doi:

Types de publication

Journal Article Research Support, Non-U.S. Gov't Research Support, U.S. Gov't, Non-P.H.S.

Langues

eng

Sous-ensembles de citation

IM

Pagination

4672

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Auteurs

Jinxing Li (J)

Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, 90095, USA. jinxing.li.87@gmail.com.

Jacob Bortnik (J)

Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, 90095, USA. jbortnik@gmail.com.

Xin An (X)

Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, 90095, USA.

Wen Li (W)

Center for Space Physics, Boston University, Boston, MA, USA.

Vassilis Angelopoulos (V)

Department of Earth, Space and Planetary Sciences, University of California, Los Angeles, CA, 90095, USA.

Richard M Thorne (RM)

Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, 90095, USA.

Christopher T Russell (CT)

Department of Earth, Space and Planetary Sciences, University of California, Los Angeles, CA, 90095, USA.

Binbin Ni (B)

Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan, Hubei, 430072, China.
CAS Center for Excellence in Comparative Planetology, Heifei, Anhui, 230026, China.

Xiaochen Shen (X)

Center for Space Physics, Boston University, Boston, MA, USA.

William S Kurth (WS)

Department of Physics and Astronomy, University of Iowa, Iowa City, IA, 52242-1479, USA.

George B Hospodarsky (GB)

Department of Physics and Astronomy, University of Iowa, Iowa City, IA, 52242-1479, USA.

David P Hartley (DP)

Department of Physics and Astronomy, University of Iowa, Iowa City, IA, 52242-1479, USA.

Herbert O Funsten (HO)

Los Alamos National Laboratory, MS-D466, PO Box 1663, Los Alamos, NM, 87545, USA.

Harlan E Spence (HE)

Institute for the Study of Earth, Oceans, and Space, University of New Hampshire, Durham, NH, 03824-3525, USA.

Daniel N Baker (DN)

Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA.

Classifications MeSH