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Numerical studies of azimuthal modulations of the solar wind with magnetic fields

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Abstract

The evolution of azimuthal modulation of the solar wind is examined by numerical integration of the basic equations governing supersonic, super-Alfvénic, polytropic one fluid flow in the equatorial plane of the Sun with radial as well as azumuthal magnetic fields. The computations are started by introducing various sets of finite amplitude perturbations stationary with respect to the Sun. It is shown that for a properly chosen set of simultaneous perturbations of the radial velocity and temperature, quantitative agreement with the averaged observational results at 1 AU can be obtained, including the advance of the density modulation with respect to those of velocity and temperature. It is further shown that modulations at 1 AU depend on the relative azimuthal positions between the Sun and the Earth.

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References

  • Barnes, A.: 1969, Astrophys. J. 155, 311.

    Google Scholar 

  • Brandt, J. C., Wolff, C., and Cassinelli, J. P.: 1969, Astrophys. J. 156, 1117.

    Google Scholar 

  • Burlaga, L. F. and Ogilvie, K. W.: 1970, Astrophys. J. 159, 659.

    Google Scholar 

  • Burlaga, L. F., Ogilvie, K. W., Fairfield, D. H., and Montgomery, M. D.: 1971, Astrophys. J. 164, 137

    Google Scholar 

  • Cuperman, S., Harten, A., and Dryer, M.: 1962, Astrophys. J. 177, 555.

    Google Scholar 

  • Dryer, M.: 1970, Cosmic Electrodyn. 1, 348.

    Google Scholar 

  • Gosling, J. T., Hundhausen, A. J., Pizzo, V., and Ashbridge, J.: 1972, J. Geophys. Res. 77, 5442.

    Google Scholar 

  • Hartle, R. E. and Barnes, A.: 1970, J. Geophys. Res. 75, 6915.

    Google Scholar 

  • Hartle, R. E. and Sturrock, P. A.: 1968, Astrophys. J. 151, 1155.

    Google Scholar 

  • Hollweg, J. V.: 1973, J. Geophys. Res. (in press).

  • Hundhausen, A. J.: 1972, Coronal Expansion and Solar Wind, Springer-Verlag, New York.

    Google Scholar 

  • Hundhausen, A. J.: 1973, J. Geophys. Res. (in press).

  • Hundhausen, A. J. and Gentry, R. A.: 1969, J. Geophys. Res. 74, 2908.

    Google Scholar 

  • Keppenheuer, K. O.: 1953, in G. P. Kuiper (ed.), The Sun, Univ. Chicago Press, Chap. 6.

  • Korobeinikov, V. P.: 1969, Solar Phys. 7, 463.

    Google Scholar 

  • Lee, T. S. and Balwanz, W. W.: 1968, Solar Phys. 4, 240.

    Google Scholar 

  • Matsuda, T. and Sakurai, T.: 1972, Cosmic Electrodyn. 3, 97.

    Google Scholar 

  • Parker, E. N.: 1963, Interplanetary Dynamical Processes, Interscience Publisher, New York.

    Google Scholar 

  • Sakurai, T.: 1971, Cosmic Electrodyn. 1, 460.

    Google Scholar 

  • Siscoe, G. L. and Finley, L. T.: 1972, J. Geophys. Res. 77, 35.

    Google Scholar 

  • Weber, E. J. and Davis, L., 1967, Astrophys. J. 148, 217.

    Google Scholar 

  • Weber, E. J. and Davis, L.: 1970, J. Geophys. Res. 75, 2419.

    Google Scholar 

  • Whang, Y. C. and Chang, C. C.: 1965, J. Geophys. Res. 70, 4175.

    Google Scholar 

  • Whang, Y. C., Liu, C. K., and Chang, C. C.: 1966, Astrophys. J. 145, 255.

    Google Scholar 

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The National Center for Atmospheric Research is sponsored by the National Science Foundation.

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Nakagawa, Y., Wellck, R.E. Numerical studies of azimuthal modulations of the solar wind with magnetic fields. Sol Phys 32, 257–270 (1973). https://doi.org/10.1007/BF00152741

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  • DOI: https://doi.org/10.1007/BF00152741

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