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Correlation Dependences Determined by Simultaneous Multispacecraft Observations of Solar Wind and IMF Structures

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Abstract

Solar wind measurements on board several spacecraft were used to study the two-points correlations of the solar wind plasma structures. The factor shaving the most influence on the correlation level are the density variability and IMF cone angle. The characteristic length of large solar wind structures is estimated at 500–1000 R E.

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References

  • Paularena, K.I., Zastenker, G.N., Lazarus, A.J. and Dalin, P.A.: 1998, J. Geophys. Res. A7 103, 14601.

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  • Zastenker, G.N., Dalin, P.A., Petrukovich, A.A, Nozdrachev, M.N., Romanov, S.A., Paularena, K.I., Richardson, J.D., Lazarus, A.J., Lepping, R.P. and Szabo, A.: 2000, Phys. Chem. Earth 25 (1-2), 137.

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Authors and Affiliations

  1. Space Research Institute, Profsojuznaia 84/32, Moscow, 117810, Russia

    P.A. Dalin & G.N. Zastenker

  2. Center for Space Research, M.I.T., Cambridge, MA, 02139, U.S.A

    K.I. Paularena & J.D. Richardson

Authors
  1. P.A. Dalin
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  2. G.N. Zastenker
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  3. K.I. Paularena
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  4. J.D. Richardson
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Dalin, P., Zastenker, G., Paularena, K. et al. Correlation Dependences Determined by Simultaneous Multispacecraft Observations of Solar Wind and IMF Structures. Astrophysics and Space Science 277, 323–324 (2001). https://doi.org/10.1023/A:1012202418764

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  • DOI: https://doi.org/10.1023/A:1012202418764

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