By Paul D Bayless; Idaho National Engineering Laboratory.; U.S. Nuclear Regulatory Commission. Office of Nuclear Regulatory Research.; et al
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A poleward meridional ﬂow of predominantly following polarity ﬁelds accumulates a ﬁeld at the poles that reverses the polar ﬁeld polarities at about the time of cycle maximum. 6. Polar ﬁeld strengths from the Wilcox Solar Observatory. Daily measurements of the ﬁeld strength in the polemost aperture (latitudes above about 55 ) are smoothed to remove seasonal eﬀects. The ﬁelds reversed in 1980, 1990, and 2000, about the time of sunspot cycle maximum for each cycle. Both hemispheres are not perfectly synchronized.
Simpson, J. , and J. R. Wang (1967), Dimension of the Cosmic-Ray Modulation Region, Astrophys. J. , 149, L73. Simpson, J. , B. Rossi, A. R. Hibbs, R. Jastrow, F. L. Whipple, T. Gold, E. Parker, N. Christoﬁlos, and J. A. Van Allen (1959), Round table discussion, J. Geophys. , 64, 1691. 2 Solar cycle 23 David H. Hathaway and Steven T. 1 INTRODUCTION Ulysses’ launch in October of 1990 was at the maximum of solar activity cycle 22. The ﬁrst passages through the polar regions of the heliosphere came in 1994 and 1995, very near the minimum of activity between cycles 22 and 23.
In cycle 23 the tilt maximized in the southern hemisphere around maximum and stayed large for 2–3 years. Conversely, the tilt in the north began to decrease within a year of solar maximum, along with the formation of the larger ﬁelds in the north and the northern polar coronal hole. 12. The magnetic ﬁeld energy density is small compared with the kinetic energy of the solar wind. Therefore, the HCS is Sec. 14. The maximum extent of the HCS for the indicated dates/Carrington rotations, over approximately two solar cycles.