EGU21-2555
https://doi.org/10.5194/egusphere-egu21-2555
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

A clock for the Sun's magnetic Hale cycle and 27 day recurrences in the aa geomagnetic index

Sandra Chapman1, Scott McIntosh2, Robert Leamon3,4, and Nicholas Watkins1,5,6
Sandra Chapman et al.
  • 1University of Warwick, Centre for Fusion, Space and Astrophysics, Physics, Coventry CV4 7AL, United Kingdom of Great Britain – England, Scotland, Wales (s.c.chapman@warwick.ac.uk)
  • 2National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, USA.
  • 3University of Maryland--Baltimore County, Goddard Planetary Heliophysics Institute, Baltimore, MD 21250, USA.
  • 4NASA Goddard Space Flight Center, Code 672, Greenbelt, MD~20771, USA
  • 5Grantham research Institute on Climate Change and the Environment, London School of Economics and Political Science, London, WC2A 2AE, UK
  • 6Faculty of Science, Technology, Engineering and Mathematics, The Open University, Milton Keynes, MK7 6AA, UK

We construct a new solar cycle phase clock which maps each of the last 18 solar cycles onto a single normalized epoch for the approximately 22 year Hale (magnetic polarity) cycle, using the Hilbert transform of daily sunspot numbers (SSN) since 1818. We use the clock to study solar and geomagnetic climatology as seen in datasets available over multiple solar cycles. The occurrence of solar maxima on the clock shows almost no Hale cycle dependence, confirming that the clock is synchronized with polarity reversals.  The odd cycle minima lead the even cycle minima by ~ 1.1 normalized years, whereas the odd cycle terminators (when sunspot bands from opposite hemispheres have moved to the equator and coincide, thus terminating the cycle, McIntosh(2019)) lag the even cycle terminators  by ~ 2.3 normalized years.  The average interval between each minimum and terminator  is thus relatively extended for odd cycles and shortened for even ones. We re-engineer the R27 index that was orignally proposed by Sargent(1985) to parameterize 27 day recurrences in the aa index. We perform an epoch analysis of autocovariance in the aa index using the Hale cycle clock to obtain a high time resolution parameter for 27 day recurrence, <acv(27)>. This reveals that the transition to recurrence, that is, to an ordered solar wind dominated by high speed streams, is fast, occurring within 2-3 solar rotations or less. It resolves an extended late declining phase which is approximately twice as long on even Schwabe cycles as odd ones. We find that Galactic Cosmic Ray flux rises in step with <acv(27)> but then stays high. Our analysis also identifies a slow timescale trend in SSN that simply tracks the Gleissberg cycle. We find that this trend is in phase with the slow timescale trend in the modulus of sunspot latitudes, and in antiphase with that of the R27 index.

How to cite: Chapman, S., McIntosh, S., Leamon, R., and Watkins, N.: A clock for the Sun's magnetic Hale cycle and 27 day recurrences in the aa geomagnetic index, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-2555, https://doi.org/10.5194/egusphere-egu21-2555, 2021.

Corresponding presentation materials formerly uploaded have been withdrawn.