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.

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