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On the question of coronal holes as sources of geomagnetic disturbances

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Summary

Using a more detailed geomagnetic activity Kp index, the finding in [3] that geomagnetic activity increases after the CMP of coronal holes, was verified; it was shown using individual activity patterns, that coronal holes apparently do not form a homogeneous class of phenomena, which must be respect in considerations of emissions of fast solar wind streams.

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References

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Authors and Affiliations

  1. Geophysical Institute, Czechosl. Acad. Sci., Prague

    Jaroslav Halenka

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  1. Jaroslav Halenka
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Halenka, J. On the question of coronal holes as sources of geomagnetic disturbances. Stud Geophys Geod 21, 365–370 (1977). https://doi.org/10.1007/BF01613269

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  • DOI: https://doi.org/10.1007/BF01613269

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