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The Sun and Heliosphere at Solar Maximum
DOI: 10.1126/science.1086295 Bibcode: 2003Sci...302.1165S

Krupp, N.; Balogh, A.; Geiss, J. +9 more

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,…

2003 Science
Ulysses 52