- #106
Saul
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As I said, there is a massive cosmogenic isotope change that is concurrent with a massive 1000 year abrupt cooling event which paleo climatologists have called the "Younger Dryas" cooling event.http://cio.eldoc.ub.rug.nl/FILES/root/2000/QuatIntRenssen/2000QuatIntRenssen.pdf
There is evidence is the sun is moving to a complete solar magnetic cycle interruption, not a slow down.
The magnetic field strength of newly formed sunspots has been linearly decreasing with time. It is believed sunspots are created at interface of the convection zone and the radiative zone (the tachocline). The sunspot requires a minimum field strength of around 1500 gauss to avoid being torn to pieces as it moves up to the surface of the sun through the turbulent convection zone.
Sunspots from the previous cycle are believed to move back down to tachocline to form the seeds for the next cycle, which explains why there is some periodicity between every second cycle. (The period of the convection motion motion is 22 years.). An interesting and unanswered question is how does the solar magnetic cycle re-start after being interrupted?
http://www.leif.org/EOS/2009EO300001.pdf
Reduced solar activity as a trigger for the start of the Younger Dryas?
The Younger Dryas (YD, 12.9-11.6 ka cal BP, Alley et al., 1993) was a cold event that interrupted the general warming trend during the last deglaciation. The YD was not unique, as it represents the last of a number of events during the Late Pleistocene, all characterised by rapid and intensive cooling in the North Atlantic region (e.g., Bond et al., 1993; Anderson, 1997). During these events, icebergs were common in the N Atlantic Ocean, as evidenced by ice-rafted sediments found in ocean cores. The most prominent of these episodes with ice rafting are known as Heinrich events (e.g., Bond et al., 1992, 1993; Andrews, 1998). A Heinrich-like event (H-0) was simultaneous with the YD (Andrews et al., 1995). Moreover, the YD seems to be part of a millennial-scale cycle of cool climatic events that extends into the Holocene (Denton and KarleHn, 1973; Harvey, 1980; Magny and Ru!aldi, 1995; O'Brien et al., 1995; Bond et al., 1997). Based on analysis of the 14C record from tree rings, Stuiver and Braziunas (1993) suggested that solar variability could be an important factor a!ecting climate variations during the Holocene (see also Magny, 1993, 1995a), possibly operating together with oceanic forcing.
Evidence for solar variations in the geological past may be inferred from cosmogenic isotope records (Hoyt and Schatten, 1997). The two most important of these isotopes are carbon-14 (14C) and beryllium-10 (10Be),... Estimates for the increase in 14C at the start of the YD all demonstrate a strong and rapid rise: 40-70 %/% within 300 years (Goslar et al., 1995), 30-60 %/% in 70 years (BjoK rck et al., 1996), 50-80%/% in 200 years (Hughen et al., 1998) and 70%/% in 200 years (Hajdas et al., 1998). This change is apparently the largest increase of atmospheric 14C known from late glacial and Holocene records (Goslar et al., 1995). Hajdas et al. (1998) used this sharp increase of atmospheric 14C at the onset of the YD as a tool for time correlation between sites.
There is evidence is the sun is moving to a complete solar magnetic cycle interruption, not a slow down.
The magnetic field strength of newly formed sunspots has been linearly decreasing with time. It is believed sunspots are created at interface of the convection zone and the radiative zone (the tachocline). The sunspot requires a minimum field strength of around 1500 gauss to avoid being torn to pieces as it moves up to the surface of the sun through the turbulent convection zone.
Sunspots from the previous cycle are believed to move back down to tachocline to form the seeds for the next cycle, which explains why there is some periodicity between every second cycle. (The period of the convection motion motion is 22 years.). An interesting and unanswered question is how does the solar magnetic cycle re-start after being interrupted?
http://www.leif.org/EOS/2009EO300001.pdf
Are Sunspots Different During This Solar Minimum?
But something is unusual about the current sunspot cycle. The current solar minimum has been unusually long, and with more than 670 days without sunspots through June 2009, the number of spotless days has not been equaled since 1933 (see http:// users . telenet .be/ j . janssens/ Spotless/ Spotless .html). The solar wind is reported to be in a uniquely low energy state since space measurements began nearly 40 years ago [Fisk and Zhao, 2009].
The same data were later published [Penn and Livingston, 2006], and the observations showed that the magnetic field strength in sunspots were decreasing with time, independent of the sunspot cycle. A simple linear extrapolation of those data suggested that sunspots might completely vanish by 2015.
Yet although the Sun’s magnetic polarity has reversed and the new solar cycle has been detected, most of the new cycle’s spots have been tiny “pores” without penumbrae (see Figure 1); in fact, nearly all of these features are seen only on flux magnetograms and are difficult to detect on whitelight images.
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