The heliospheric Hale cycle over the last 300 years and its implications for a “lost” late 18th century solar cycle

Mathew J. Owens; Ken G. McCracken; Mike Lockwood; Luke Barnard

doi:10.1051/swsc/2015032

All issues

Volume 5 (2015)

J. Space Weather Space Clim., 5 (2015) A30

References

Open Access

Issue		J. Space Weather Space Clim. Volume 5, 2015


Article Number		A30
Number of page(s)		9
DOI		https://doi.org/10.1051/swsc/2015032
Published online		09 September 2015

Babcock, H.W. The topology of the Sun’s magnetic field and the 22-year cycle. Astrophys. J., 133, 527–587, 1961. [NASA ADS] [CrossRef] [Google Scholar]
Beer, J., K.G. McCracken, and R. von Steiger. Cosmogenic Radionuclides: Theory and applications in the terrestrial and space environments, Berlin, Springer, 2012. [Google Scholar]
Beer, J., S. Tobias, and N. Weiss. An active sun throughout the maunder minimum. Sol. Phys., 181, 237–249, 1998. [NASA ADS] [CrossRef] [Google Scholar]
Charbonneau, P., G. Beaubien, and C. St-Jean. Fluctuations in Babcock-Leighton dynamos. II. Revisiting the Gnevyshev-Ohl rule. Astrophys. J., 658, 657, 2007. [NASA ADS] [CrossRef] [Google Scholar]
Clette, F., L. Svalgaard, J.M. Vaquero, and E.W. Cliver. Revisiting the sunspot number. Space Sci. Rev., 186, 35–103, 2014. [NASA ADS] [CrossRef] [Google Scholar]
Cliver, E.W., V. Boriakoff, and K.H. Bounar. The 22‐year cycle of geomagnetic and solar wind activity. J. Geophys. Res. [Space Phys.] (1978–2012), 101, 27091–27109, 1996. [CrossRef] [Google Scholar]
Cliver, E.W., and A.G. Ling. 22 Year patterns in the relationship of sunspot number and tilt angle to cosmic-ray intensity. Astrophys. J. Lett., 551, L189–L192, 2001, DOI: 10.1086/320022. [NASA ADS] [CrossRef] [Google Scholar]
Gnevyshev, M., and A. Ohl. On the 22-year cycle of solar activity. Astron. Zh., 25, 18, 1948. [Google Scholar]
Hale, G.E., and S.B. Nicholson. The law of sun-spot polarity. Astrophys. J., 62, 270–300, 1925. [NASA ADS] [CrossRef] [Google Scholar]
Hoyt, D.V., and K.H. Schatten. Group sunspot numbers: A new solar activity reconstruction. Sol. Phys., 181, 491–512, 1998. [NASA ADS] [CrossRef] [Google Scholar]
Jiang, J., R.H. Cameron, D. Schmitt, and M. Schüssler. The solar magnetic field since 1700-II. Physical reconstruction of total, polar and open flux. A&A, 528, A83, 2011. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Jokipii, J.R., E.H. Levy, and W.B. Hubbard. Effects of particle drift on cosmic-ray transport. I – General properties, application to solar modulation. Astrophys. J., 213, 861–868, 1977, DOI: 10.1086/155218. [NASA ADS] [CrossRef] [Google Scholar]
Karoff, C., F. Inceoglu, M.F. Knudsen, J. Olsen, and A. Fogtmann-Schulz. The lost sunspot cycle: New support from ¹⁰Be measurements. A&A, 575, A77, 2014, DOI: 10.1051/0004-6361/201424927. [CrossRef] [EDP Sciences] [Google Scholar]
Krüger, H., H. Moraal, J. Bieber, J. Clem, P. Evenson, K. Pyle, M. Duldig, and J. Humble. A calibration neutron monitor: Energy response and instrumental temperature sensitivity. J. Geophys. Res., 113, A08101, 2008, DOI: 10.1029/2008JA013229. [Google Scholar]
Leussu, R., I.G. Usoskin, R. Arlt, and K. Mursula. Inconsistency of the Wolf sunspot number series around 1848. A&A, 559, A28, 2013, DOI: 10.1051/0004-6361/201322373. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Lockwood, M. Solar influence on global and regional climates. Surv. Geophys., 33, 503–534, 2012, DOI: 10.1007/s10712-012-9181-3. [NASA ADS] [CrossRef] [Google Scholar]
Lockwood, M. Reconstruction and prediction of variations in the open solar magnetic flux and interplanetary conditions. Living Rev. Sol. Phys., 10, 4, 2013, DOI: 10.12942/lrsp-2013-4. [Google Scholar]
Lockwood, M., and L. Barnard. An arch seen in the UK: a new catalogue of auroral observations made in the British Isles and Ireland, Astron. Geophys., 56, 4–25, 2015. [CrossRef] [Google Scholar]
Lockwood, M., H. Nevanlinna, L. Barnard, M.J. Owens, R.G. Harrison, A.P. Rouillard, and C.J. Scott. Reconstruction of geomagnetic activity and near-Earth interplanetary conditions over the past 167 yr – Part 4: Near-Earth solar wind speed, IMF, and open solar flux. Ann. Geophys., 32, 383–399, 2014a, DOI: 10.5194/angeo-32-383-2014. [NASA ADS] [CrossRef] [Google Scholar]
Lockwood, M., and M.J. Owens. Centennial variations in sunspot number, open solar flux and streamer belt width: 3. Modeling. J. Geophys. Res., 119, 5193–5209, 2014, DOI: 10.1002/2014JA019973. [CrossRef] [Google Scholar]
Lockwood, M., M.J. Owens, and L. Barnard. Centennial variations in sunspot number, open solar flux, and streamer belt width: 1. Correction of the sunspot number record since 1874. J. Geophys. Res., 119, 5172–5182, 2014b, DOI: 10.1002/2014JA019970. [NASA ADS] [CrossRef] [Google Scholar]
McCracken, K. Variations in the production of ¹⁰Be due to the 11 year modulation of the cosmic radiation, and variations in the vector geomagnetic dipole. Proc. Int. Conf. Cosmic Rays, 4129–4132, 2001. [Google Scholar]
McCracken, K.G., and J. Beer. The Annual Cosmic-radiation Intensities 1391–2014; the annual Heliospheric Magnetic Field Strengths 1391–1983; and identification of solar cosmic ray events in the cosmogenic record 1800–1983. Sol. Phys., 2015, in press. [Google Scholar]
Owens, M.J., and N.U. Crooker. Coronal mass ejections and magnetic flux buildup in the heliosphere. J. Geophys. Res., 111, A10104, 2006, DOI: 10.1029/2006JA011641. [NASA ADS] [CrossRef] [Google Scholar]
Owens, M.J., N.U. Crooker, and M. Lockwood. How is open solar magnetic flux lost over the solar cycle? J. Geophys. Res., 116, A04111, 2011a, DOI: 10.1029/2010JA016039. [Google Scholar]
Owens, M.J., and R.J. Forsyth. The heliospheric magnetic field. Living Rev. Sol. Phys., 10, 5, 2013, DOI: 10.12942/lrsp-2013-5. [Google Scholar]
Owens, M.J., and M. Lockwood. Cyclic loss of open solar flux since 1868: the link to heliospheric current sheet tilt and implications for the Maunder Minimum. J. Geophys. Res., 117, A04102, 2012, DOI: 10.1029/2011JA017193. [Google Scholar]
Owens, M.J., M. Lockwood, C.J. Davis, and L. Barnard. Solar cycle 24: implications for energetic particles and long-term space climate change. Geophys. Res. Lett., 38, L19106, 2011b, DOI: 10.1029/2011GL049328. [CrossRef] [Google Scholar]
Owens, M.J., I. Usoskin, and M. Lockwood. Heliospheric modulation of galactic cosmic rays during grand solar minima: past and future variations. Geophys. Res. Lett., 39, L19102, 2012, DOI: 10.1029/2012GL053151. [NASA ADS] [CrossRef] [Google Scholar]
Potgieter, M., and H. Moraal. A drift model for the modulation of galactic cosmic rays. Astrophys. J., 294, 425–440, 1985. [NASA ADS] [CrossRef] [Google Scholar]
Riley, P., H. Moraal, H. Moraal, et al. Inferring the structure of the solar corona and inner heliosphere during the maunder minimum using global thermodynamic magnetohydrodynamic simulations. Astrophys. J., 802, 105, 2015, DOI: 10.1088/0004-637X/802/2/105. [NASA ADS] [CrossRef] [Google Scholar]
Roth, R., and F. Joos. A reconstruction of radiocarbon production and total solar irradiance from the Holocene ¹⁴C and CO₂ records: implications of data and model uncertainties. Climate of the Past, 9, 1879–1909, 2013. [NASA ADS] [CrossRef] [Google Scholar]
Rouillard, A., and M. Lockwood. Oscillations in the open solar magnetic flux with a period of 1.68 years: imprint on galactic cosmic rays and implications for heliospheric shielding. Ann. Geophys., 22, 4381–4395, 2004, DOI: 1432-0576/ag/2004-22-4381. [CrossRef] [Google Scholar]
Solanki, S.K., M. Schüssler, and M. Fligge. Evolution of the Sun’s large-scale magnetic field since the Maunder minimum. Nature, 408, 445–447, 2000, DOI: 10.1038/35044027. [NASA ADS] [CrossRef] [PubMed] [Google Scholar]
Steinhilber, F., J.A. Abreu, J. Beer, et al. 9,400 years of cosmic radiation and solar activity from ice cores and tree rings. Proceedings of the National Academy of Science, 109, 5967–5971, 2012, DOI: 10.1073/pnas.1118965109. [NASA ADS] [CrossRef] [Google Scholar]
Thomas, S.R., M.J. Owens, and M. Lockwood. The 22-year hale cycle in cosmic ray flux – evidence for direct heliospheric modulation. Sol. Phys., 289, 407–421, 2013, DOI: 10.1007/s11207-013-0341-5. [CrossRef] [Google Scholar]
Usoskin, I., R. Arlt, E. Asvestari, et al. The Maunder minimum (1645–1715) was indeed a Grand minimum: A reassessment of multiple datasets. A&A, 2015, in press, DOI: 10.1051/0004-6361/201526652. [Google Scholar]
Usoskin, I.G. A history of solar activity over millennia. Living Rev. Sol. Phys., 10, 2013, DOI: 10.12942/lrsp-2013-1. [Google Scholar]
Usoskin, I.G., K. Mursula, R. Arlt, and G.A. Kovaltsov. A solar cycle lost in 1793–1800: Early sunspot observations resolve the old mystery. Astrophys. J. Lett., 700, L154, 2009. [NASA ADS] [CrossRef] [Google Scholar]
Usoskin, I.G., K. Mursula, and G.A. Kovaltsov. Was one sunspot cycle lost in late XVIII century? A&A, 370, L31–L34, 2001. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Usoskin, I.G., K. Mursula, and G.A. Kovaltsov. Lost sunspot cycle in the beginning of Dalton minimum: New evidence and consequences. Geophys. Res. Lett., 29, 2183, 2002. [NASA ADS] [CrossRef] [Google Scholar]
Waldmeier, M. The beginning of a new cycle of solar activity. Nature, 253, 419, 1975. [CrossRef] [Google Scholar]
Wolf, R.A. Abstracts of his latest results, Mon. Not. R. Astron. Soc., 21, 77, 1861. [CrossRef] [Google Scholar]
Zolotova, N., and D. Ponyavin. Enigma of the solar cycle 4 still not resolved. Astrophys. J., 736, 115, 2011. [CrossRef] [Google Scholar]

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