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Using the paleo-cosmic ray record to compare the solar activity during the sunspot minimum of 2006- 2009 with those during the Spoerer, Maunder, and Dalton.

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Presentation on theme: "Using the paleo-cosmic ray record to compare the solar activity during the sunspot minimum of 2006- 2009 with those during the Spoerer, Maunder, and Dalton."— Presentation transcript:

1 Using the paleo-cosmic ray record to compare the solar activity during the sunspot minimum of 2006- 2009 with those during the Spoerer, Maunder, and Dalton Grand Minima Ken McCracken IPST, University of Maryland. jellore@hinet.net.au NESSC, Boston, 17April, 2014 U. New Hampshire, 14 April, 2014

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3 McCracken and Beer, 2014

4 GALACTIC COSMIC RADIATION SPALLATION OF ATMOSPHERIC A, N and O. TIME 1O Be ICE CORE THE PALEO- COSMIC RADIATION RECORD TREE RINGS 14 C DIFFERENT ATMOSPHERIC AND SEQUESTRATION PROCESSES 5730 y 1.5x10 6 y 36 Cl > 120 investigator years of data

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6 COSMOGENIC NUCLIDE PRODUCTION DURING THE PAST 10,000 YEARS TWO INDEPENDENT MEASUREMENTS OF THE PAST Beer et al, ICRC 2007

7 Steinhilber et al, PNAS (USA), 2012 M

8 PALEO-COSMIC RAYS - A PROXY FOR SPACE CLIMATE High PCR(“Maunder”)Low PCR (“Modern”) Low sunspot cyclesHigh sunspot cycles Low solar activity High solar activity Low HMFHigh HMF High radiation environ’tLow radiation environ’t

9 OTHER SEQUENCES OF GRAND MINIMA- AND >1000 YR LONG INTERVALS BETWEEN M S M M S M M D D D

10 McCracken and Beer, JGR, 2014 Dye 3 and North GRIP Annual Data

11 THE MAUNDER MINIMUM – UP CLOSE. McCracken and Beer, JGR, 2014

12 COSMIC RAYS- A COSMIC MAGNETOMETER After Caballero - Lopez et al, 2004

13 Modulation Potential (Observed) Φ = k. V P. B 2 (t) / ˂ (ΔB) 2 ˃ Helio-magnetic field (inferred) B(t) = B 0. {Φ(t)/ Φ 0 } 1/α

14 The HMF (Omni-2) near Earth, 1975-2009 B max B min B max / B min = (1.31-1.63) Average = 1.52

15 COMPARING THE SOLAR DYNAMO DURING MAUNDER MINIMUM WITH THE PRESENT MODERN MAUNDER B max / B min 1.31-1.63 1.30-1.85 Average 1.521.54 CONCLUSION- A remarkable similarity- the solar dynamo apparently worked then like now with much weaker magnetic fields.

16 Name Duration Rise Cycles Peak NM(%) Min.HMF(nT) Spoerer 1440-1540 4 111.3 2.4 Maunder 1645-1715 5 117.0 <2.0 Dalton 1790-1830 2 110.9 2.6 Gleissberg 1880-1910 104.5 3.8 Extended Minimum 2006-9 102.8 3.9 Modern epoch Minima 1954-96 97.7 5.4 Comparison of key features of the Minima

17 COMPARISON OF EXTENDED SUNSPOT MINIMUM 2006-9 AND GRAND MINIMA, 1400-1850 AD. - The cosmic ray intensity during 2006-9 was well below those in the Spoerer and Maunder Minimum, while approaching that in the Gleissberg Minimum. - The cosmic ray intensity increased over 4 to 5 solar cycles at the commencement of the Grand Minima. - The next solar minimum 2019 will determine whether the Sun is going into another Grand Minimum. -The solar dynamo operated during the Maunder Minimum as it does today

18 THANK YOU

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21 Steinhilber et al, PNAS (USA), 2012 M

22 THE SEQUENCE OF GRAND MINIMA- 950-2000 AD - OUR CALIBRATION ERA. In “Grand Minimum” ~40% of time! Space Era Level


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