CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2

N. U. Crooker; J. T. Gosling; V. Bothmer; R. J. Forsyth; P. R. Gazis; A. Hewish; T. S. Horbury; D. S. Intriligator; J. R. Jokipii; J. Kóta; A. J. Lazarus; M. A. Lee; E. Lucek; E. Marsch; A. Posner; I. G. Richardson; E. C. Roelof; J. M. Schmidt; G. L. Siscoe; B. T. Tsurutani; R. F. Wimmer-Schweingruber

doi:10.1023/a:1005253526438

CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2

N. U. Crooker, J. T. Gosling, V. Bothmer, R. J. Forsyth, P. R. Gazis, A. Hewish, T. S. Horbury, D. S. Intriligator, J. R. Jokipii, J. Kóta, A. J. Lazarus, M. A. Lee, E. Lucek, E. Marsch, A. Posner, I. G. Richardson, E. C. Roelof, J. M. Schmidt, G. L. Siscoe, B. T. TsurutaniR. F. Wimmer-Schweingruber

Lunar and Planetary Lab

Research output: Contribution to journal › Article › peer-review

93 Scopus citations

Abstract

Corotating interaction regions (CIRs) in the middle heliosphere have distinct morphological features and associated patterns of turbulence and energetic particles. This report summarizes current understanding of those features and patterns, discusses how they can vary from case to case and with distance from the Sun and possible causes of those variations, presents an analytical model of the morphological features found in earlier qualitative models and numerical simulations, and identifies aspects of the features and patterns that have yet to be resolved.

Original language	English (US)
Pages (from-to)	179-220
Number of pages	42
Journal	Space Science Reviews
Volume	89
Issue number	1-2
DOIs	https://doi.org/10.1023/a:1005253526438
State	Published - 1999

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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Crooker, N. U., Gosling, J. T., Bothmer, V., Forsyth, R. J., Gazis, P. R., Hewish, A., Horbury, T. S., Intriligator, D. S., Jokipii, J. R., Kóta, J., Lazarus, A. J., Lee, M. A., Lucek, E., Marsch, E., Posner, A., Richardson, I. G., Roelof, E. C., Schmidt, J. M., Siscoe, G. L., ... Wimmer-Schweingruber, R. F. (1999). CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2. Space Science Reviews, 89(1-2), 179-220. https://doi.org/10.1023/a:1005253526438

Crooker, NU, Gosling, JT, Bothmer, V, Forsyth, RJ, Gazis, PR, Hewish, A, Horbury, TS, Intriligator, DS, Jokipii, JR, Kóta, J, Lazarus, AJ, Lee, MA, Lucek, E, Marsch, E, Posner, A, Richardson, IG, Roelof, EC, Schmidt, JM, Siscoe, GL, Tsurutani, BT & Wimmer-Schweingruber, RF 1999, 'CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2', Space Science Reviews, vol. 89, no. 1-2, pp. 179-220. https://doi.org/10.1023/a:1005253526438

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abstract = "Corotating interaction regions (CIRs) in the middle heliosphere have distinct morphological features and associated patterns of turbulence and energetic particles. This report summarizes current understanding of those features and patterns, discusses how they can vary from case to case and with distance from the Sun and possible causes of those variations, presents an analytical model of the morphological features found in earlier qualitative models and numerical simulations, and identifies aspects of the features and patterns that have yet to be resolved.",

author = "Crooker, {N. U.} and Gosling, {J. T.} and V. Bothmer and Forsyth, {R. J.} and Gazis, {P. R.} and A. Hewish and Horbury, {T. S.} and Intriligator, {D. S.} and Jokipii, {J. R.} and J. K{\'o}ta and Lazarus, {A. J.} and Lee, {M. A.} and E. Lucek and E. Marsch and A. Posner and Richardson, {I. G.} and Roelof, {E. C.} and Schmidt, {J. M.} and Siscoe, {G. L.} and Tsurutani, {B. T.} and Wimmer-Schweingruber, {R. F.}",

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T1 - CIR morphology, turbulence, discontinuities, and energetic particles

T2 - Report of Working Group 2

AU - Crooker, N. U.

AU - Gosling, J. T.

AU - Bothmer, V.

AU - Forsyth, R. J.

AU - Gazis, P. R.

AU - Hewish, A.

AU - Horbury, T. S.

AU - Intriligator, D. S.

AU - Jokipii, J. R.

AU - Kóta, J.

AU - Lazarus, A. J.

AU - Lee, M. A.

AU - Lucek, E.

AU - Marsch, E.

AU - Posner, A.

AU - Richardson, I. G.

AU - Roelof, E. C.

AU - Schmidt, J. M.

AU - Siscoe, G. L.

AU - Tsurutani, B. T.

AU - Wimmer-Schweingruber, R. F.

PY - 1999

Y1 - 1999

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AB - Corotating interaction regions (CIRs) in the middle heliosphere have distinct morphological features and associated patterns of turbulence and energetic particles. This report summarizes current understanding of those features and patterns, discusses how they can vary from case to case and with distance from the Sun and possible causes of those variations, presents an analytical model of the morphological features found in earlier qualitative models and numerical simulations, and identifies aspects of the features and patterns that have yet to be resolved.

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CIR morphology, turbulence, discontinuities, and energetic particles: Report of Working Group 2

Abstract

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