Literature DB >> 15602555

An extreme distortion of the Van Allen belt arising from the 'Hallowe'en' solar storm in 2003.

D N Baker1, S G Kanekal, X Li, S P Monk, J Goldstein, J L Burch.   

Abstract

The Earth's radiation belts--also known as the Van Allen belts--contain high-energy electrons trapped on magnetic field lines. The centre of the outer belt is usually 20,000-25,000 km from Earth. The region between the belts is normally devoid of particles, and is accordingly favoured as a location for spacecraft operation because of the benign environment. Here we report that the outer Van Allen belt was compressed dramatically by a solar storm known as the 'Hallowe'en storm' of 2003. From 1 to 10 November, the outer belt had its centre only approximately 10,000 km from Earth's equatorial surface, and the plasmasphere was similarly displaced inwards. The region between the belts became the location of high particle radiation intensity. This remarkable deformation of the entire magnetosphere implies surprisingly powerful acceleration and loss processes deep within the magnetosphere.

Year:  2004        PMID: 15602555     DOI: 10.1038/nature03116

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  10 in total

1.  An impenetrable barrier to ultrarelativistic electrons in the Van Allen radiation belts.

Authors:  D N Baker; A N Jaynes; V C Hoxie; R M Thorne; J C Foster; X Li; J F Fennell; J R Wygant; S G Kanekal; P J Erickson; W Kurth; W Li; Q Ma; Q Schiller; L Blum; D M Malaspina; A Gerrard; L J Lanzerotti
Journal:  Nature       Date:  2014-11-27       Impact factor: 49.962

2.  Measurement of electrons from albedo neutron decay and neutron density in near-Earth space.

Authors:  Xinlin Li; Richard Selesnick; Quintin Schiller; Kun Zhang; Hong Zhao; Daniel N Baker; Michael A Temerin
Journal:  Nature       Date:  2017-12-13       Impact factor: 49.962

3.  Combined model of topside ionosphere and plasmasphere derived from radio-occultation and Van Allen Probes data.

Authors:  Fabricio S Prol; Artem G Smirnov; M Mainul Hoque; Yuri Y Shprits
Journal:  Sci Rep       Date:  2022-06-13       Impact factor: 4.996

4.  Upper limit on the inner radiation belt MeV electron intensity.

Authors:  X Li; R S Selesnick; D N Baker; A N Jaynes; S G Kanekal; Q Schiller; L Blum; J Fennell; J B Blake
Journal:  J Geophys Res Space Phys       Date:  2015-02-24       Impact factor: 2.811

5.  Enhanced radial transport and energization of radiation belt electrons due to drift orbit bifurcations.

Authors:  A Y Ukhorskiy; M I Sitnov; R M Millan; B T Kress; D C Smith
Journal:  J Geophys Res Space Phys       Date:  2014-01-08       Impact factor: 2.811

6.  Energy-dependent dynamics of keV to MeV electrons in the inner zone, outer zone, and slot regions.

Authors:  Geoffrey D Reeves; Reiner H W Friedel; Brian A Larsen; Ruth M Skoug; Herbert O Funsten; Seth G Claudepierre; Joseph F Fennell; Drew L Turner; Mick H Denton; Harlan E Spence; J Bernard Blake; Daniel N Baker
Journal:  J Geophys Res Space Phys       Date:  2016-01-28       Impact factor: 2.811

7.  Explaining the apparent impenetrable barrier to ultra-relativistic electrons in the outer Van Allen belt.

Authors:  Louis G Ozeke; Ian R Mann; Kyle R Murphy; Alex W Degeling; Seth G Claudepierre; Harlan E Spence
Journal:  Nat Commun       Date:  2018-05-10       Impact factor: 14.919

Review 8.  Vacuum-Ultraviolet Photon Detections.

Authors:  Wei Zheng; Lemin Jia; Feng Huang
Journal:  iScience       Date:  2020-05-08

9.  The Patterns of Male and Female Flowers in Flowering Stage May Not Be Optimal Resource Allocation for Fruit and Seed Growth.

Authors:  Lei Gao; Guozhu Yu; Fangyu Hu; Zhiqi Li; Weihua Li; Changlian Peng
Journal:  Plants (Basel)       Date:  2021-12-20

10.  A Climatology of Long-Duration High 2-MeV Electron Flux Periods in the Outer Radiation Belt.

Authors:  D Mourenas; O V Agapitov; A V Artemyev; X-J Zhang
Journal:  J Geophys Res Space Phys       Date:  2022-08-15       Impact factor: 3.111

  10 in total

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