Collective phenomena in the inner magnetosphere

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Collective phenomena in the inner magnetosphere. / Baker, DN; Kanekal, SG; Klimas, AJ; Vassiliadis, D; Pulkkinen, T.I.

In: Physics of Plasmas, Vol. 6, No. 11, 11.1999, p. 4195-4199.

Research output: Contribution to journalArticle

Harvard

Baker, DN, Kanekal, SG, Klimas, AJ, Vassiliadis, D & Pulkkinen, TI 1999, 'Collective phenomena in the inner magnetosphere', Physics of Plasmas, vol. 6, no. 11, pp. 4195-4199. https://doi.org/10.1063/1.873685

APA

Baker, DN., Kanekal, SG., Klimas, AJ., Vassiliadis, D., & Pulkkinen, T. I. (1999). Collective phenomena in the inner magnetosphere. Physics of Plasmas, 6(11), 4195-4199. https://doi.org/10.1063/1.873685

Vancouver

Baker DN, Kanekal SG, Klimas AJ, Vassiliadis D, Pulkkinen TI. Collective phenomena in the inner magnetosphere. Physics of Plasmas. 1999 Nov;6(11):4195-4199. https://doi.org/10.1063/1.873685

Author

Baker, DN ; Kanekal, SG ; Klimas, AJ ; Vassiliadis, D ; Pulkkinen, T.I. / Collective phenomena in the inner magnetosphere. In: Physics of Plasmas. 1999 ; Vol. 6, No. 11. pp. 4195-4199.

Bibtex - Download

@article{03f0810cf15d4286859c68ea915b4362,
title = "Collective phenomena in the inner magnetosphere",
abstract = "The Earth's magnetosphere exhibits substantial complexity in many of its physical properties. Particle populations wax and wane and magnetic fields fluctuate on virtually all observed time scales, from less than 1 minute to many days. Much of the variability of the magnetosphere and its interaction with the ionosphere can be ascribed to the phenomena termed {"}substorms{"} and {"}storms.{"} Ample evidence is found that these geospace disturbances, though exhibiting event-to-event differences, are remarkably repetitive and have basic underlying similarities. The ring current development, radiation belt particle changes, and basic substorm patterns suggest a high degree of coherence in the phenomena. Observations, modeling, and basic physical properties are discussed here that point to a relatively ordered, low-dimensional underlying dynamics in the magnetosphere. These results suggest that nonlinear processes and couplings introduce much of the observed complexity in magnetospheric particle and field changes. (C) 1999 American Institute of Physics. [S1070-664X(99)03311-X].",
keywords = "DYNAMICS, MODEL",
author = "DN Baker and SG Kanekal and AJ Klimas and D Vassiliadis and T.I. Pulkkinen",
year = "1999",
month = "11",
doi = "10.1063/1.873685",
language = "English",
volume = "6",
pages = "4195--4199",
journal = "Physics of Plasmas",
issn = "1070-664X",
number = "11",

}

RIS - Download

TY - JOUR

T1 - Collective phenomena in the inner magnetosphere

AU - Baker, DN

AU - Kanekal, SG

AU - Klimas, AJ

AU - Vassiliadis, D

AU - Pulkkinen, T.I.

PY - 1999/11

Y1 - 1999/11

N2 - The Earth's magnetosphere exhibits substantial complexity in many of its physical properties. Particle populations wax and wane and magnetic fields fluctuate on virtually all observed time scales, from less than 1 minute to many days. Much of the variability of the magnetosphere and its interaction with the ionosphere can be ascribed to the phenomena termed "substorms" and "storms." Ample evidence is found that these geospace disturbances, though exhibiting event-to-event differences, are remarkably repetitive and have basic underlying similarities. The ring current development, radiation belt particle changes, and basic substorm patterns suggest a high degree of coherence in the phenomena. Observations, modeling, and basic physical properties are discussed here that point to a relatively ordered, low-dimensional underlying dynamics in the magnetosphere. These results suggest that nonlinear processes and couplings introduce much of the observed complexity in magnetospheric particle and field changes. (C) 1999 American Institute of Physics. [S1070-664X(99)03311-X].

AB - The Earth's magnetosphere exhibits substantial complexity in many of its physical properties. Particle populations wax and wane and magnetic fields fluctuate on virtually all observed time scales, from less than 1 minute to many days. Much of the variability of the magnetosphere and its interaction with the ionosphere can be ascribed to the phenomena termed "substorms" and "storms." Ample evidence is found that these geospace disturbances, though exhibiting event-to-event differences, are remarkably repetitive and have basic underlying similarities. The ring current development, radiation belt particle changes, and basic substorm patterns suggest a high degree of coherence in the phenomena. Observations, modeling, and basic physical properties are discussed here that point to a relatively ordered, low-dimensional underlying dynamics in the magnetosphere. These results suggest that nonlinear processes and couplings introduce much of the observed complexity in magnetospheric particle and field changes. (C) 1999 American Institute of Physics. [S1070-664X(99)03311-X].

KW - DYNAMICS

KW - MODEL

U2 - 10.1063/1.873685

DO - 10.1063/1.873685

M3 - Article

VL - 6

SP - 4195

EP - 4199

JO - Physics of Plasmas

JF - Physics of Plasmas

SN - 1070-664X

IS - 11

ER -

ID: 3011004