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The Sun and Heliosphere at Solar Maximum
Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to,...
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Published in: | Science (American Association for the Advancement of Science) 2003-11, Vol.302 (5648), p.1165-1169 |
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creator | Smith, E. J. Marsden, R. G. Balogh, A. Gloeckler, G. Geiss, J. McComas, D. J. McKibben, R. B. MacDowall, R. J. Lanzerotti, L. J. Krupp, N. Krueger, H. Landgraf, M. |
description | Recent Ulysses observations from the Sun's equator to the poles reveal fundamental properties of the three-dimensional heliosphere at the maximum in solar activity. The heliospheric magnetic field originates from a magnetic dipole oriented nearly perpendicular to, instead of nearly parallel to, the Sun's rotation axis. Magnetic fields, solar wind, and energetic charged particles from low-latitude sources reach all latitudes, including the polar caps. The very fast high-latitude wind and polar coronal holes disappear and reappear together. Solar wind speed continues to be inversely correlated with coronal temperature. The cosmic ray flux is reduced symmetrically at all latitudes. |
doi_str_mv | 10.1126/science.1086295 |
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subjects | Astronomy Charged particles Cosmic rays Earth, ocean, space Exact sciences and technology Geophysics Heliosphere Magnetic fields Magnetic flux Magnetic polarity Observations Particle radiation, solar wind Polar caps Review Solar energy Solar flares Solar physics Solar system Solar wind Sun Sunspots Tropical regions |
title | The Sun and Heliosphere at Solar Maximum |
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