The three-dimensional solar wind around solar maximum

D. J. McComas, H. A. Elliott, N. A. Schwadron, J. T. Gosling, R. M. Skoug, B. E. Goldstein

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Abstract

Ulysses is now completing its second solar polar orbit, dropping back down in latitude as the Sun passes through its post-maximum phase of the solar cycle. A mid-sized circumpolar coronal hole that formed around solar maximum in the northern hemisphere has persisted and produced a highly inclined CIR, which was observed from ∼70°N down to ∼30°N. We find that the speed maxima in the high-speed streams follow the same slow drop in speed with decreasing latitude observed in the large polar coronal holes around solar minimum. These results suggest a solar wind acceleration effect that is related to heliolatitude or solar rotation. We also find that the solar wind dynamic pressure is significantly lower in the post-maximum phase of this solar cycle than during the previous one, indicating that while the heliosphere is larger than near solar minimum, it should be smaller than during or after the previous maximum.

Original languageEnglish (US)
Pages (from-to)24-1 - 24-4
JournalGeophysical Research Letters
Volume30
Issue number10
DOIs
StatePublished - May 15 2003

All Science Journal Classification (ASJC) codes

  • Geophysics
  • Earth and Planetary Sciences(all)

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    McComas, D. J., Elliott, H. A., Schwadron, N. A., Gosling, J. T., Skoug, R. M., & Goldstein, B. E. (2003). The three-dimensional solar wind around solar maximum. Geophysical Research Letters, 30(10), 24-1 - 24-4. https://doi.org/10.1029/2003gl017136