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Three-Dimensional Gradients of Solar Particles Inside 5 AU

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The Sun and the Heliosphere in Three Dimensions

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 123))

Abstract

The spatial gradients (field-aligned, longitudinal and latitudinal) in solar flare energetic particle events are described in terms of their occurrence in the three phases of the event (rise, maximum and decay). The information that can be derived from these phases is discussed in the context of the Ulysses mission.

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References

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Author information

Authors and Affiliations

  1. Applied Physics Laboratory, Johns Hopkins University, Johns Hopkins Road, Laurel, Maryland, 20707, USA

    Edmond C. Roelof

Authors
  1. Edmond C. Roelof
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Editor information

Editors and Affiliations

  1. Solar and Heliospheric Science Division, Space Science Department of ESA, Noordwijk, The Netherlands

    R. G. Marsden

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© 1986 D. Reidel Publishing Company

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Roelof, E.C. (1986). Three-Dimensional Gradients of Solar Particles Inside 5 AU. In: Marsden, R.G. (eds) The Sun and the Heliosphere in Three Dimensions. Astrophysics and Space Science Library, vol 123. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4612-5_40

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  • DOI: https://doi.org/10.1007/978-94-009-4612-5_40

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8549-6

  • Online ISBN: 978-94-009-4612-5

  • eBook Packages: Springer Book Archive

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