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Maunder minimum

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Maunder minimum

The Maunder minimum in a 400 year history of sunspot numbers

The Maunder Minimum, also known as the "prolonged sunspot minimum", is the name used for the period starting in about 1645 and continuing to about 1715 when sunspots became exceedingly rare, as noted by solar observers of the time.

The term was introduced after John A. Eddy published a landmark 1976 paper in Science.[1] Astronomers before Eddy had also named the period after the solar astronomers Annie (1868-1947) and E. Walter Maunder (1851–1928) who studied how sunspot latitudes changed with time.[2] The period the husband and wife team examined included the second half of the 17th century. Two papers were published in Edward Maunder's name in 1890 and 1894, and he cited earlier papers written by Gustav Spörer.[3] Due to the social climate of the time, Annie's contribution was not publicly recognized.[4]

During one 30-year period within the Maunder Minimum, Spörer observed fewer than 50 sunspots, as opposed to a more typical 40,000–50,000 spots in modern times.[5]

Like the Dalton Minimum and Spörer Minimum, the Maunder Minimum coincided with a period of lower-than-average European temperatures.

Sunspot observations

The Maunder Minimum occurred between 1645 and 1715 when very few sunspots were observed. This was not due to a lack of observations; during the 17th century, Giovanni Domenico Cassini carried out a systematic program of solar observations at the Observatoire de Paris, thanks to the astronomers Jean Picard and Philippe de La Hire. Johannes Hevelius also performed observations on his own. The total numbers of sunspots (but not Wolf numbers) in different years were as follows:

Year Sunspots
1610 9
1620 6
1630 9
1640 0
1650 3
1660 Some sunspots reported by Jan Heweliusz in Machina Coelestis
1670 0
1680 1 huge sunspot observed by Giovanni Domenico Cassini

During the Maunder Minimum enough sunspots were sighted so that 11-year cycles could be extrapolated from the count. The maxima occurred in 1676, 1684, 1695, 1705 and 1716.

The sunspot activity was then concentrated in the southern hemisphere of the Sun, except for the last cycle when the sunspots appeared in the northern hemisphere, too.

According to Spörer's law, at the start of a cycle, spots appear at ever lower latitudes until they average at about latitude 15° at solar maximum. The average then continues to drift lower to about 7° and after that, while spots of the old cycle fade, new cycle spots start appearing again at high latitudes.

The visibility of these spots is also affected by the velocity of the sun's surface rotation at various latitudes:

Solar latitude Rotation period
35° 26.7
40° 28.0
75° 33.0

Visibility is somewhat affected by observations being done from the ecliptic. The ecliptic is inclined 7° from the plane of the Sun's equator (latitude 0°).

Little Ice Age

Comparison of group sunspot numbers (top), Central England Temperature (CET) observations (middle) and reconstructions and modeling of Northern Hemisphere Temperatures (NHT). The CET in red are summer averages (for June, July and August) and in blue winter averages (for December of previous year, January and February). NHT in grey is the distribution from basket of paleoclimate reconstructions (darker grey showing higher probability values) and in red are from model simulations that account for solar and volcanic variations. By way of comparison, on the same scales the anomaly for modern data (after 31 December 1999) for summer CET is +0.65oC, for winter CET is +1.34oC, and for NHT is +1.08oC. Sunspot data are as in supplementary data to [6] and Central England Temperature data are as published by the UK Met Office [7] The NHT data are described in box TS.5, Figure 1 of the IPCC AR5 report of Working Group 1.[8]

The Maunder Minimum coincided with the middle part of the Little Ice Age, during which Europe and North America were subjected to very cold winters. A causal connection between low sunspot activity and cold European winters has recently been made using the longest existing surface temperature record, the Central England Temperature record [9] and also using the ERA-40 re-analysis dataset.[10] A potential explanation of this has been offered by observations by NASA's Solar Radiation and Climate Experiment which suggest that solar UV output is more variable over the course of the solar cycle than scientists had previously thought.[11] In 2011 an article was published in the Nature Geoscience journal that uses a climate model with stratospheric layers and the SORCE data to tie low solar activity to jet stream behavior and mild winters in some places (southern Europe and Canada/Greenland) and colder winters in others (northern Europe and the United States).[12] In Europe, examples of very cold winters are 1683-4, 1694-5, and the winter of 1708–9.[13] In such years River Thames frost fairs were held. That the Thames ceased to freeze in the 19th. century has been argued to be evidence both for, and against, anthropogenic climate change. In fact it is neither, being caused by the removal of the "Old" (medieval) London Bridge in 1825 (which was a weir which slowed the river flow and prevented salt water reaching upstream) and the construction of the river embankments which also increased the river flow.

Note that the term "Little Ice Age" applied to the Maunder minimum is something of a misnomer as it implies a period of unremitting cold (and on a global scale) which is not the case. For example, the coldest winter in the Central England Temperature record is 1683-4 but the winter just 2 years later (both in the middle of the Maunder minimum) was the fifth warmest in the whole 350-year CET record. Furthermore, summers during the Maunder minimum were not significantly different to those seen in subsequent years. The drop in global average temperatures in paleoclimate reconstructions at the start of the Little Ice Age was between about 1560 and 1600, whereas the Maunder minimum began almost 50 years later.

Other observations

Solar activity events recorded in radiocarbon.
Graph showing proxies of solar activity, including changes in sunspot number and cosmogenic isotope production.

Some scientists hypothesize that the dense wood used in Stradivarius instruments was caused by slow tree growth during the cooler period. Instrument maker Antonio Stradivari was born a year before the start of the Maunder Minimum.[14]

Past solar activity may be recorded by various proxies including carbon-14 and beryllium-10.[15] These indicate lower solar activity during the Maunder Minimum. The scale of changes resulting in the production of carbon-14 in one cycle is small (about one percent of medium abundance) and can be taken into account when radiocarbon dating is used to determine the age of archaeological artifacts. The interpretation of the beryllium-10 and carbon-14 cosmogenic isotope abundance records stored in terrestrial reservoirs such as ice sheets and tree rings has been greatly aided by reconstructions of solar and heliospheric magnetic fields based on historic data on Geomagnetic storm activity, which bridge the time gap between the end of the usable cosmogenic isotope data and the start of modern spacecraft data.[16][17]

Other historical sunspot minima have been detected either directly or by the analysis of the cosmogenic isotopes; these include the Spörer Minimum (1450–1540), and less markedly the Dalton Minimum (1790–1820). In a 2012 study, sunspot minima have been detected by analysis of carbon-14 in lake sediments.[18] In total there seem to have been 18 periods of sunspot minima in the last 8,000 years, and studies indicate that the sun currently spends up to a quarter of its time in these minima.

A paper based on an analysis of a Flamsteed drawing, suggests that the Sun's surface rotation slowed in the deep Maunder minimum (1684).[19]

During the Maunder Minimum aurorae had been observed seemingly normally, with a regular decadal-scale cycle.[20][21] This is somewhat surprising because the later, and less deep, Dalton sunspot minimum is clearly seen in auroral occurrence frequency, at least at lower geomagnetic latitudes.[22] Because geomagnetic latitude is an important factor in auroral occurrence, (lower-latitude aurorae requiring higher levels of solar-terrestrial activity) it becomes important to allow for population migration and other factors that may have influenced the number of reliable auroral observers at a given magnetic latitude for the earlier dates.[23] Decadal-scale cycles during the Maunder minimum can also be seen in the abundances of the beryllium-10 cosmogenic isotope (which unlike carbon-14 can be studied with annual resolution) [24] but these appear to be in antiphase with any remnant sunspot activity. An explanation in terms of solar cycles in loss of solar magnetic flux was proposed in 2012.[25]

The fundamental papers on the Maunder minimum (Eddy, Legrand, Gleissberg, Schröder, Landsberg et al.) have been published in Case studies on the Spörer, Maunder and Dalton Minima.[26]

See also


  1. ^ Eddy J.A. (June 1976). "The Maunder Minimum". Science 192 (4245): 1189–1202.   PDF Copy
  2. ^ Who named the Maunder Minimum?
  3. ^ See:
    • E.W.M. (1890) "Professor Spoerer's researches on sun-spots," Monthly Notices of the Royal Astronomical Society, 50 : 251-252.
    • E. Walter Maunder (August 1, 1894) "A prolonged sunspot minimum," Knowledge, 17 : 173-176.
    • Spörer (1887) "Ueber die Periodicität der Sonnenflecken seit dem Jahre 1618, vornehmlich in Bezug auf die heliographische Breite derselben, und Hinweis auf eine erhebliche Störung dieser Periodicität während eines langen Zeitraumes" (On the periodicity of sunspots since the year 1618, especially with respect to the heliographic latitude of the same, and reference to a significant disturbance of this periodicity during a long period), Vierteljahrsschrift der Astronomischen Gesellschaft (Leipzig), 22 : 323-329.
    • G. Spoerer (February 1889) "Sur les différences que présentent l'hémisphère nord et l'hémisphère sud du Soleil" (On the differences that the northern hemisphere and southern hemisphere of the sun present), Bulletin Astronomique, 6 : 60-63.
  4. ^
  5. ^ John E. Beckman and Terence J. Mahoney. "The Maunder Minimum and Climate Change: Have Historical Records Aided Current Research?". Astronomical Society of the Pacific. 
  6. ^ Lockwood, M. et al. (July 2014). "Centennial variations in sunspot number, open solar flux and streamer belt width: 2. Comparison with the geomagnetic data". J. Geophys. Res. 119 (7): 5183–5192.   PDF Copy
  7. ^ "Hadley Centre Central England Temperature (HadCET) dataset". 
  8. ^ "Climate Change 2013, The Physical Science Basis, WG1, 5th Assessment Report, IPCC". 
  9. ^ Lockwood, M. et al. (February 2010). "Are cold winters in Europe associated with low solar activity?". Env. Res. Lett. 5 (2): 024001.   PDF Copy
  10. ^ Woollings, T.G. et al. (October 2010). "Enhanced signature of solar variability in Eurasian winter climate". Geophys. Res. Lett. 37 (20): L20805.  
  11. ^ Harder, J.A. et al. (April 2009). "Trends in solar spectral irradiance variability in the visible and infrared". Geophys. Res. Lett. 36 (7): L07801.  
  12. ^ Ineson, S. et al. (October 2011). "Solar forcing of winter climate variability in the Northern Hemisphere". Nature Geoscience 4: 753–757.  
  13. ^ Niles' Weekly Register, Volume 15, Supplement, History of the Weather
  14. ^ Whitehouse, David (December 17, 2003). "Stradivarius 'sound' due to Sun".  
  15. ^ Usoskin I.G. (2008). "A History of Solar Activity over Millennia". Living Reviews in Solar Physics 5 (3).   PDF Copy
  16. ^ Lockwood M. et al. (June 1999). "A doubling of the sun's coronal magnetic field during the last 100 years". Nature 399.   PDF Copy
  17. ^ Lockwood M. (2013). "Reconstruction and Prediction of Variations in the Open Solar Magnetic Flux and Interplanetary Conditions". Living Reviews in Solar Physics 10 (4).   PDF Copy
  18. ^ Celia Martin-Puertas, Katja Matthes, Achim Brauer, Raimund Muscheler, Felicitas Hansen, Christof Petrick, Ala Aldahan, Göran Possnert & Bas van Geel (April 2, 2012). "Regional atmospheric circulation shifts induced by a grand solar minimum".  
  19. ^ Vaquero JM, Sánchez-Bajo F, Gallego MC (2002). "A Measure of the Solar Rotation During the Maunder Minimum". Solar Physics 207 (2): 219.  
  20. ^ Schröder, Wilfried (1992). "On the existence of the 11-year cycle in solar and auroral activity before and during the Maunder Minimum". Journal of Geomagnetism and Geoelectricity 44 (2): 119–28.  
  21. ^ Legrand, JP; Le Goff, M; Mazaudier, C; Schröder, W (1992). "Solar and auroral activities during the seventeenth century". Acta Geodaetica et Geophysica Hungarica 27 (2–4): 251–282. 
  22. ^ Nevanlinna, H. (1995). "Auroral observations in Finland - Visual sightings during the 18th and 19th centuries". Journal of Geomagnetism and Geoelectricity 47 (10): 953–960.   PDF Copy
  23. ^ Vázquez, M., et al. (2014). "Long-term Spatial and Temporal Variations of Aurora Borealis Events in the Period 1700 – 1905". Solar Physics 289 (5): 1843–1861.   PDF Copy
  24. ^ Beer, J. et al. (1988). "An Active Sun Throughout the Maunder Minimum". Solar Physics 181 (1): 237–249.   PDF Copy
  25. ^ Owens, M.J.. et al. (2012). "Heliospheric modulation of galactic cosmic rays during grand solar minima: Past and future variations". Geophys. Res. Lett. 39 (19): L19102.   PDF Copy
  26. ^ Schröder, Wilfried (2005). Case studies on the Spörer, Maunder, and Dalton minima. Beiträge zur Geschichte der Geophysik und Kosmischen Physik 6. Potsdam: AKGGP, Science Edition. 

Further reading

External links

  •, further links and resources, updated 2014
  • Climate History Network, network of historical climatologists, updated 2014
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