International Journal of Astronomy and Astrophysics, 2013, 3, 260-273 http://dx.doi.org/10.4236/ijaa.2013.33031 Published Online September 2013 (http://www.scirp.org/journal/ijaa)
Copyright © 2013 SciRes. IJAA
Are Uranus & Neptune Responsible for Solar Grand Minima and Solar Cycle Modulation?
Geoff J. Sharp Moonbeam Close, Narre Warren South, Melbourne, Australia
Email: [email protected]
Received April 7, 2013; revised May 9, 2013; accepted May 16, 2013
Copyright © 2013 Geoff J. Sharp. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
ABSTRACT
Detailed solar Angular Momentum (AM) graphs produced from the Jet Propulsion Laboratory (JPL) DE405 ephemeris display cyclic perturbations that show a very strong correlation with prior solar activity slowdowns. These same AM perturbations also occur simultaneously with known solar path changes about the Solar System Barycentre (SSB). The AM perturbations can be measured and quantified allowing analysis of past solar cycle modulations along with the 11,500 year solar proxy records (14C & 10Be). The detailed AM information also displays a recurring wave of modula- tion that aligns very closely with the observed sunspot record since 1650. The AM perturbation and modulation is a direct product of the outer gas giants (Uranus & Neptune). This information gives the opportunity to predict future grand minima along with normal solar cycle strength with some confidence. A proposed mechanical link between solar activity and planetary influence via a discrepancy found in solar/planet AM along with current AM perturbations indi- cate solar cycle 24 & 25 will be heavily reduced in sunspot activity resembling a similar pattern to solar cycles 5 & 6 during the Dalton Minimum (1790-1830). Keywords: Solar Grand Minimum; Solar Modulation; Angular Momentum; Uranus; Neptune; SSB; Barycentre
1. Introduction
Solar system dynamics have been postulated as the main solar driver for many decades. Jose (1965) [1] was the first to associate a recurring solar system pattern of the 4 outer planets (179 years). Jose suggested this pattern correlates with the modulation of the solar cycle. New research via this study suggests that over the past 6000 years the 179 year cycle cannot be maintained and is closer to a 172 year cycle which aligns with the synodic period of Uranus & Neptune (171.44 years). Later Land- scheidt (2003) [2] progressed the planetary influence theories further by associating quasi-cyclic negative torque readings or “zero crossings” (AM readings going below zero) that can occur near grand minima. It has been found since that the negative readings occur in the gen- eral region of most grand minima but such records are not a reliable method of predicting the timing and strength of grand minima at the solar cycle level.
Other studies detailed the orbit path of the Sun around the Solar System Barycentre (SSB) that showed a bal- anced trefoil pattern during times of “normal” solar cy- cles. Charvàtovà (2000) [3] shows this pattern or path-
way as it moves to a disordered state during times of so- lar slowdown and are a direct result of the Uranus/Nep- tune conjunction of the era.
Theodor Landscheidt’s work has inspired both profes- sional and citizen scientists. For example, Carl Smith (2007) [4] while researching Landscheidt’s work pro- duced an AM graph using the JPL ephemeris (Figure 1). This graph for the first time clearly showed the detailed perturbations of solar AM that also coincide with past solar slowdowns along with the disordered solar path about the SSB. Carl Smith passed away in 2009 and to our knowledge was probably not aware of the hidden detail that was contained in his work, the Perturbed An- gular Momentum curve holding the clue.
The perturbed curves on the solar AM graph (Figure 1) correspond with solar torque perturbations, which also alter the normal balanced solar path around the SSB. The solar velocity is also perturbed on a 172-year cycle (av- erage) and a greater diversion between the orbital AM of the Sun and planets is observed. It is proposed through a spin orbit coupling mechanism resulting in varying solar equatorial rotation rate, the solar dynamo is reduced dur- ing these 172 year intervals.
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1620 1640 1660 1680 1700 1720 1740 1760 1780 1800 1820
1800 1820 1840 1860 1880 1900 1920 1940 1960 1980 2000
1980 2000 2020 2040 2060 2080 2100 2120 2140 2160 2180
-1e+47
0
1e+47
2e+47
3e+47
4e+47
5e+47
-1e+47
0
1e+47
2e+47
3e+47
4e+47
5e+47
-1e+47
0
1e+47
2e+47
3e+47
4e+47
5e+47
Sun-SSB angular momentum
SC5
SC7 SC12 SC20
SC24
LANDSCHEIDT MINIMUM
MINIMUM
MAUNDER MINIMUM DALTON
Figure 1. Detailed Solar Angular Momentum graph showing the perturbations (AMP events) at the green arrows. This graph is a modified example of Carl Smith’s original work that is based on JPL DE405 data. The green arrows and solar grand minima headings have been added. Carl Smith’s [4] original graph is displayed HERE Note: AM units of measure equate to gram-cm^2/sec.
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2. Discussion—Grand Minima
The AM perturbations shown in Figure 1 are the result of the extra AM from the Uranus/Neptune conjunction. The timing in relation to the Jupiter/Saturn opposition provides the different perturbation shapes that can be measured via the relevant planet angles and categorised into two groups. Perturbations occurring on the down slope are denoted “Type A” and those on the up slope “Type B” (down slope = right hand side of peak).
Type B occurrences coincide with weaker solar slow- downs and are more common before 1000AD and the Medieval Warm Period (MWP). Almost all perturbations throughout the past 6000 years coincide with solar down- turns that vary in intensity.
During the past 750 years strong Type A perturbations are evident on the AM graph (Figure 1). Coinciding with
the strong Type A multiple appearances is one of the greatest sustained periods of grand minima of the Holo- cene (Little Ice Age 1300 - 1870 approx.). The Type A perturbations all have the same planetary configuration, but with slightly differing planet angles (Figure 2).
Type A perturbations have a positive Saturn angle, the higher the Saturn angle the higher the perturbation height on the AM graph. Type B perturbations always display a negative Saturn angle (Figure 2). During each conjunc- tion of Uranus & Neptune, Jupiter & Saturn have multi- ple oppositions. Depending on the planet positions of the era this can result in normally 3 - 4 Angular Momentum Perturbations (AMP) events for each Uranus/Neptune conjunction. The midpoint of these AMP groups displays a 172-year average spacing. The Sporer Minimum (1400 - 1600 approx.) has 2 strong AMP events, and 2 medium AMP events that coincide with one of the longest and
-35° +30°
SATURNSATURN
TYPE B TYPE A
SUN
JUPITER
NEPTUNE
URANUS
15°
Figure 2. Typical planet positions demonstrating strong Types A & B perturbations. The Type A example is taken from near the centre of the Sporer Minimum (1472). Type B events coinciding with less reduction of solar activity compared with Type A events of similar angle (reverse).
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deepest grand minima of the Holocene.
Type A AMP events have a major impact on the inner loop trajectory of the Sun in its orbit around the SSB. The Sun normally follows two distinct loops around the SSB (Figure 3) with each loop lasting approximately ten years. A shallow inner loop is evident when Jupiter & Saturn are in opposition and a much wider loop when Jupiter & Saturn are in conjunction. During strong Type A AMP events the inner loop path is greatly extended
pushing the Sun out of its normal balanced trefoil pattern whereas the normal trefoil pattern returns the Sun to near the SSB on the inner loop path. The AMP event shows the path greatly extended from the SSB, the inner loop is trying to be an outer loop. Type B AMP events affect the outer loop of the Sun’s path, which has the effect of re- ducing the distance travelled away from the SSB. Ac- companying the AMP events is usually a zero crossing (solar AM goes below zero) where Saturn, Uranus &
2029
2013
2015
2005
1991 2031
19892011
2017 2017
Solar inner loop path change from J/S/U/N when ideal type “A” alignment occurs that corresponds with green arrows on Carl’s Graph. 2809
1987
202720032039
2037
2001 2025 2035
19992023
1987 2021
1985
19952019
Large perturbations occur when the disordered inner orbit is higher than the radius of the Sun
J+S opposing
J+S conjunction
Figure 3. The path of the Sun shows the two distinct loops around the SSB (centre point). The extended inner loop begin- ning around 2005 coinciding with a reasonably strong Type A event. Solar cycle 24 is predicted to be the first grand mini- mum cycle. The sunspot records since 1650 suggest that 2 solar cycles can be affected by strong Type A events, there is speculation that the Hale cycle is interrupted and follows a 22-year-period. An animated movie of the path taken can be viewed at http://www.landscheidt.info/images/sim.swf.
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Neptune are in conjunction with Jupiter opposing. This places the Sun right on the SSB, or indeed on the other side of the SSB. The zero crossings can occur either side of an AMP event.
The Carbon 14 (14C) record for the Holocene is a re- liable solar proxy record. Recent Beryllium 10 (10Be) isotope records derived from ice cores by Steinhilber, Beer, Frolich (2009) [5] confirm the accuracy of the 14C record (Figure 4). During the 11,500 years of the Holo- cene a regular pattern of solar downturns can be observed which vary in intensity. The 14C records used in this report are originally from the INTCAL98 (Stuiver, et al.,
1998b) [6] study and further extended by Solanki et al. (2004) [7] and Usoskin, Solanki & Kovaltsov (2007) [8]. The 14C values are compared with the AMP group cen- tre values (Figure 5). The isotope data show a strong cor- relation with each individual AMP group in timing and strength. Each AMP group centre has the relevant planet angles recorded including the orientation of Uranus/ Neptune (Figure 6). The Figure 6 refers to Figure 5 AM group centres. Most AMP groups are comprised of three to four separate AMP events separated by approx. 40 years.
The planetary angles taken at the AMP events (Figure
70
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20
10
0
-10
-20
-179
5
-165
5
-151
5
-137
5
-123
5
-109
5
-955
-815
-675
-535
-395
-255
-115
25
165
305
445
585
725
865
1005
1145
1285
1425
1565
1705
1845
-14C –Solanki 2005 Years GM Centre – Grand Minima Centre each 172 yr Avg. weighted by J/S angles 10 Be Steinhilber, Beer, Frohlich
= strong Type “A” disturbance
14C vs 10Be with Angular Momentum.
Der
ived
SS
N
Purple line = Angular Momentum Disturbance Strength (inverted)
Figure 4. Comparison of 14C and 10Be isotope records. The purple line is a representation of the AMP group strength (indi- vidual AMP events are summed to form group totals, details follow in later section) with each point representing the AMP centre. A full size image can be viewed at http://www.landscheidt.info/images/solanki_sharp.png. The isotope plots are a graphical comparison of Solanki et al. (2004) [7] & Steinhilber et al. (2009) [5].
80
Maximum Angular Momentum Table.All era’s selected from maximum momentum readingstaken just before or after Grand Minima opportunity except those marked
Sun
spot
num
ber
60
40
20
0 -10000 -9000 -8000 -7000 -6000 -5000 -4000
-3666
-2000 -1000 0 1000 2000
ANGULAR MOMENTUM vs CARBON 14
Usoskin Grand Maxima Line
Sharp Grand Minima Line
Usoskin Grand Minima Line
-3514 -3335 -3155-2989
-3000-2810 -2657 -2478 -2298 -2119 -1940 -1788 -1621 -1442 -1263 -1110 -931 -762 -573 -394 -215 -75 106 284 463 602 781 961 1293 1472 1651 1831
Year-1145-1130
-1105-1085
-1065-1054
-970-950
-885-871
-640 -620
-610 590
-570 -550
-460 -440
-282 -262
-172 155
-135 -115
-25 -5
85 100
185 206
305 321
365 385
480 500
580 600
760780
842859
942960
11181135
13401360
15801600
17621772
19421960
Year
AngMom
4.18 4.47 4.07 4.3 4.0 3.61 4.36 4.33 3.78 3.78 3.4 3.64 3.9 4.2 3.2 4.2 3.2 4.3 4.04 4.07 3.8 4.22 4.41 4.3 3.5 3.64 3.7AngMom
Figure 5. Graphical representation modified from the Usoskin et al. (2007) [8] solar proxy report. Usoskin determined that grand minima occur under 15SSN (derived SSN figures, blue line) that isolates Dalton Minimum type events. By raising the bar (green line) the repeating pattern of grand minima is observed. The middle AMP event per group is shown below the date axis with the peaks in AM shown at the top of the graph. Strong AMP groups coinciding with deep Grand Minima shown below blue line. A full size image can be viewed at http://www.landscheidt.info/images/c14nujs1.jpg.
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Year –3666 –3514 –3335 –3155 –2989 –2810 –2657 –2478 –2298 –2119 –1940
Pos N/L N/L N/L N/L N/L N/L N/L N/L N/L U/L U/L
N/U 8 55 27 10 23 2 45 38 7 5 14
J/S –55 +32 +32 +40 –78 –95 +2 +10 0 –12 –13
Year –1788 –1621 –1442 –1263 –1110 –931 –752 –573 –394 –215 –75 106
Pos N/L N/L N/L Draw N/L N/L N/L Draw U/L U/L N/L N/L
N/U 13 22 13 2 30 30 16 0 17 42 30 13
J/S +85 –35 –34 –45 +58 +62 +35 +18 +9 0 0 –10
Year 284 463 602 781 961 1153 1293 1472 1651 1831 2010
Pos U/L U/L N/L N/L N/L U/L N/L N/L U/L U/L U/L
N/U 3 35 40 30 15 30 48 15 5 20 40
J/S –24 –36 –30 –35 –65 +53 +55 +30 +25 +25 +25
Figure 6. Planet angle tables referring to Figure 5 displaying the middle AMP event per 172 year average period. Pos = rela- tive Uranus/Neptune position i.e. Neptune leading Uranus etc. N/U = angle measured between Neptune & Uranus. J/S = angle measured away from Jupiter/Saturn opposition. 6) providing a statistical measurement that can be com- pared with the AMP events and Figure 1. The depth of the solar downturns shown on the 14C graphs coinciding with the planet angles and observed AMP events, deep troughs aligning with strong Type A events and sustained periods of strong solar activity aligning with periods of weaker Type B events. Type A events can also be weak depending on the planet angles. Type B events occurring before 1000AD are a result of the changing planet angles that move slowly over long periods of time. The overall background shape of the 14C graph coincides with the occurrence and strength of Types A & B events. During times of multiple sustained Type B events, each 172 year cycle group can carry more than 3 events as observed in Figure 7.
Figure 7 shows each individual AMP event making up each AMP group, the strength of each disturbance coin- ciding with the relevant planet angles. Type A events with a J/S angle around +30 degree and N/U angle of 15 degree providing the strongest downturns, Type B&A events with a J/S angle near zero degree or 180 degree providing the weakest downturn. Weak AMP events co- incide with the Medieval Warm Period 950AD-1250AD (Figure 8).
The Sporer Minimum (Figure 9) displayed the longest period of solar inactivity across the Little Ice Age coin- ciding with 3 strong Type A events and 1 Type B event. The last two AMP events during the Maunder Minimum being stronger than the initial AMP event occurring
around 1610. Also see Figures 1 and 8.
3. Determining AMP Strength
The purple line shown on Figure 4 is a representation of the AMP strength of the era that follows the general trend of solar activity. The method used (Figure 10) is a preliminary method using visual observation of each dis- turbance of the graph period. Figure 1 displays the dif- ferent types of AMP events that cycle in groups every 172 years (average). These disturbances always line up with periods of solar downturn.
The Solanki/Steinhilber [5,7] data shows regular solar downturns that vary in intensity, by observing the shapes of the AMP events that align with these downturns we are able to see a pattern that is repeatable.
There are rare occasions of strong Type A AMP events that do not cause solar activity reduction or perhaps not as low as expected, when not meeting the Wilson Test described in Wilson et al. (2008) [9] (Figure 11). This test states that for an AMP event to fully utilize the dis- turbance, the Jupiter/Saturn opposition or conjunction must happen before cycle maximum (to achieve a cycle with less than 80SSN). This has been tested over the sunspot record but is not available for accurate testing beyond this point as the cycle maximum date is not known. 1830 and –530 are probable examples of this phenomena, during 1830 the Jupiter/Saturn conjunction occurred before cycle maximum. AMP events need to occur well before cycle maximum to achieve full impact.
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30
20
10
0
-10
-20
-179
5 -1
705
-161
5 -1
525
-143
5 -1
345
-125
5
-985
-8
95
-805
-7
15
-625
-265
-85 5
14C vs Angular Momentum D
eriv
ed S
SN
-116
5 -1
075
-535
-4
45
-355
-175
95
185
275
365
455
545
635
725
815
905
995
1085
11
75
1265
13
55
1445
1535
16
25
1715
1805
18
95
Years
14C Solanki
STRENGTH STRONG WEAK WEAK GAINING RELAPSE VERY STRONG STRONG WEAKENING
Hi Ang Mom
Type A Type B
WEAK
Figure 7. Individual AMP events plotted directly onto the Solanki data [7]. As each conjunction of Uranus & Neptune has a varying Jupiter/Saturn position, the strength of each individual AMP event along with the AMP group total changes over the millennia. This can be represented as the AM power curve of the Holocene. A full size image can be viewed at http:// www.landscheidt.info/images/solanki_sharp_detail.jpg. The spreadsheet with original Solanki data [7] with AMP events is available at http://www.landscheidt.info/images/solanki_sharp.xls.
Sun-SSB angular momentum
1620 1640
5.00E+47
4.00E+47
3.00E+47
2.00E+47
1.00E+47
0.00E+00
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Mom
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ng M
om
Ang
Mom
1580 1600 1540 1560152015001480 1460 1440
Type A Type B Years
14601440 1420 140013801360134013201300 1280 1260
1280 1260 1240 122012001180116011401120 1100 1080
1100 1080 1060 104010201000980960940 920 900
Ang
Mom
Figure 8. Solar AM graph depicting the period from 900AD - 1640AD. The change in Type A dominance shown after 1100AD. The MWP possibly being the only period during the Holocene not to be affected by the recurring 172 years AMP pattern. This is a time of transition moving from very weak Type B occurrence to a strengthening Type A dominance. The AMP events at 930 & 970 are midway between Types A & B. Note: AM units of measure equate to gram-cm^2/sec.
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1000
=TypeB AMP
1200 1400 1600 1800 2000 Year AD
20
10
0
-10
-20
Dalton Minimum
MaunderMinimumSpörer
Minimum
Wolf Minimum
Medieval Maximun
Oort Minimum
=Type A AMP
weak weak
Modern Maximun
Solar Activity Events in 14C
δ14C
(pe
rmil
le)
Figure 9. Carbon 14 graph (Wikipedia) with the AMP events overlaid.
4
Type “B”
Type “A”
2 1 .5
3 2 1
Year Count Conv
1830 5 11
1651 9 15
1472 7 3
1293 7 3
1153 2 23
961 4 15
781 4 15
602 6 7
463 5 11
284 3 19
106 2 23
-75 2 23
-215 3 19
-394 8 -1
-573 8 -1
-752 10 -9
-931 4 15
-1110 4 15
Count
Conversion
2
23
3
19
4
15
5
11
6
7
7
3
8
-1
9
-5
10
-9
Figure 10. Charts showing the AMP strength quantification method. Each count unit corresponding with 4 units of Usoskin [8] derived SSN units. Future quantification methods involving accurate planet angles would provide more detail.
By matching the AMP event shapes on the AM graphs with solar downturn strength each disturbance can be quantified. AMP events that align with deep grand min- ima (on a constant basis throughout history) get the high- est score and also show the same shape or perturbation.
4. Discussion—Solar Cycle Modulation
Solar cycle strength depicted by SSN (smoothed sunspot
number) follows a recurring wave of power that follows the overall AM values. The AM wave displays a peak at the Uranus/Neptune conjunction and the corresponding trough at the Uranus/Neptune opposition, Scafetta (2009, 2010) [10] also recognized this trend in his work dealing with the celestial origin of climate oscillations. The SSN record of the past 400 years when matched with this wave shows a strong correlation. The AMP events that
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1620 1640 1660 1680 1700 1720 1740 1760 1780 1800 1820
1800 1820 1840 1860 1880 1900 1920 1940 1960 1980 2000
1980 2000 2020 2040 2060 2080 2100 2120 2140 2160 2180-1e+47
0
1e+47
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-1e+47
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Sun-SSB angular momentum
Figure 11. Wilson’s Test. Black dots are Jupiter/Saturn together, Blue dots Jupiter/Saturn opposed, and Red dots are solar cycle maxima, reduced solar activity occurs when a black or blue dot occurs in between cycle minimum and before cycle maximum. 1830 & 1790 does not pass the test. The yellow circles comply with Wilson’s Test. Note: AM units of measure equate to gram-cm^2/sec. always occur at different intensities and length near the AM maximum interrupt the correlation and work as a separate process. The AM sine wave is also seen as a
background solar engine that affects cycle modulation (SSN) but not the length of the cycle. Other processes determine the length of each solar cycle.
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The Damon Minimum (1856-1913) is sometimes de- scribed as a grand minimum and is most likely an exam- ple of a low sunspot cycle/s affected by low AM at the time of the Uranus/Neptune opposition and not a true grand minimum. AMP events are not observed during these intervals with only low AM recorded. The AMP event is thought to create a “phase catastrophe” situation that perhaps is responsible for reported monopolar solar pole readings of the Maunder Minimum by Callebaut et al., (2007) [11]. The monopolar position is effectively providing the majority of sunspot activity to a single so- lar hemisphere. The monopolar position being described as a prolonged period where the solar poles have the same polarity as a result of only one pole reversing po- larity during the Hale cycle. These events need to be ac- commodated when comparing the AM modulation versus the sunspot cycle modulation. The monopolar distur- bance to the normal Hale cycle could explain the occur- rence of twin low cycles paired during grand minima even though the second cycle is not perturbed. The poles require the extra cycle to maintain the normal synchro- nised state. The key point being that low cycles can be a result of low AM without experiencing “phase catastro- phe” conditions. Grand minima occur during the higher part of the AM wave.
The AM graphs show a sine wave of AM modulation (around 10 years), the low points are considered as im- portant as the high points. While a direct mechanical link between AM modulation and solar cycle modulation re- mains theoretical there is a direct example of some physi- cal connection. The solar velocity (Figure 12) around the SSB is absolutely linked to the AM sine wave that pro- vides a roughly decadal acceleration/deceleration phase.
To visualise the importance of the low points in rela- tion to the high points of the AM graph, a centre point needs to be determined and the values recorded under that centre point are inverted. This provides a true read- ing of the AM strength (Figures 13 and 14). For the past 400 years an AM reading of 2E + 47 (gram-cm^2/sec) was used from Carl Smith’s data as the centre point.
5. Angular Momentum Data Formula
The original Carl Smith AM data [4] is referenced and validated by independent analysis carried out by G. E. Pease using JPL DE405 coordinates and the following standard AM formula:
2 2 2
L M yz zy zx xz xy yx
M is the Mass of the Sun in kilograms. x, y, z, xdot, ydot, zdot must be converted from kilometres and km/sec to metres and metres/sec to get m^2ks units. The equa- tion yields the absolute value of L, using the instantane- ous cross products of the body’s position and velocity vectors (Figure 15).
6. Proposed Mechanical Link via Spin Orbit Coupling
A spin orbit coupling mechanism has been discussed by Wilson et al. (2008) [9] which translates into a varying solar equatorial rotation speed, enabling changes to the solar dynamo and the meridional flows. Solar equatorial rotation rate changes have been recorded by Javaraiah (2003) [12] based on sunspot movement records.
Total Angular Momentum is the combination of orbital
Sol
ar A
M (
gram
-cm
2 /sec
)
1600
5.50E-03
Solar Velocity km/s vs Angular Momentum
1636
1649
1661
1673
1685
1697
1709
1722
1734
1746
1758
1782
1795
1807
1819
1831
1843
1855
1868
1880
1892
5.00E+46
1.00E+47
1.50E+47
2.00E+47
2.50E+47
3.00E+47
3.50E+47
4.00E+47
4.50E+47
5.00E+47
0.0085
0.0095
0.0105
0.0115
0.0125
0.0135
0.0145
0.0155
0.0165
0.0175
Sol
ar V
el (
km/s
)
Solar AM
Solar velocity km/s
1770
1624
1612
1904
1916
1928
1941
1953
1965
1977
1989
2001
2014
2026
= 172 year AMP event centres
Figure 12. Solar AM values matched with solar velocity. The red dots displaying the 172-year centre of the AMP groups. Note the repeating pattern of change in velocity. Data source: Jet Propulsion Laboratory.
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4.90E+47
1600
4.40E+47
3.90E+47
3.40E+47
2.90E+47
2.40E+47
1.90E+47
ANGULAR MOMENTUM STRENGTH (2.0e+47 centre) Geoff Sharp April 2009 www.landscheidt.info
Neptune/Uranus opposing Neptune/Uranus opposing
= grand minimum affected cycle = grand minimum producing cycle (possible)
1611
1623
1634
1646
1657
1669
1680
1692
1703
1715
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1738
1749
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1887
1899
1910
1922
1933
1945
1956
1968
1979
1991
2002
2013
2025
2036
Figure 13. Manipulated Solar AM graph using Carl Smith’s original data [4] with all points on Figure 1 below 2E + 47 in- verted. High and low AM extremes on Figure 1 are considered of equal importance, with high and low AM corresponding with strong solar cycles (outside of AMP events). High AM is linked with larger outer loop paths and lower AM linked with tighter inner loop paths towards the SSB as seen in Figure 3.
4.90E+47
1600
4.40E+47
3.90E+47
3.40E+47
2.90E+47
2.40E+47
1.90E+47
ANGULAR MOMENTUM STRENGTH (2.0e+47 centre) Geoff Sharp April 2009 www.landscheidt.info
Neptune/Uranus opposing Neptune/Uranus opposing
sunspot cycles
= grand minimum affected cycle = grand minimum producing cycle (possible)
angular momentum
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1968
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1991
2002
2013
2025
2036
Figure 14. The values of Figure 13 are compared with the SIDC Smoothed Sunspot Number (SSN) values (overlaid graphi- cally). Once allowing for AMP events and the coinciding low solar amplitude, the derived AM strength follows the SIDC sunspot record.
1700
4.5E+40 4.0E+40
3.5E+40 3.0E+40
2.5E+40 2.0E+40
1.5E+40 1.0E+40
5.0E+40
0.0E+40
1710 1720 1730 1740 1750 1760 1770 1780 1790 1800 1810 1820 1830 1840 1850 1860 1870 1880 1890 1900 1910 1920 1930 1940 1950 1960 1970 1980 1990 2000 2010
Solar Orbital Angular Momentum (kg-m2/s) Msun*sqrt((YZdot-ZYdot)2+(ZXdot-XZdot)2+(XYdot-YXdot)2)
Figure 15. G. E. Pease AM graph depicting the same AMP events and timing as the Smith AM graph. The G. E. Pease graph using JPL DE405 xyz coordinate data and the above formula to produce the same AM outcomes as Figure 1.
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AM and spin AM. The laws of AM conservation allow a “trade off” between orbital AM and spin AM. Each body in the solar system has its own orbital AM that can be calculated using the standard formula:
2 2 2
L M yz zy zx xz xy yx
If there is a discrepancy between solar orbital AM and planet/body orbital AM the laws of AM conservation would allow changes to a body’s spin AM. This could re- sult in a varying solar equatorial rotation rate.
To perform this task all the solar system planets and the asteroids Ceres, Juno, Vesta, Pallas, Eugenia, Siwa & Chiron have been included to arrive at a total planet AM. Data coordinates were taken from the JPL DE405 ephe- meris.
To compare planet AM with solar AM the inertial frame should be the same. The JPL DE405 heliocentric planetary coordinates are referred to the solar system ba- rycentric inertial frame rather than the heliocentric iner- tial frame, which required a transformation of our com- puted planetary angular momenta to the heliocentric in- ertial frame. The planet AM was calculated using helio-centric coordinates, the solar data was calculated using the SSB as the axis point (barycentric), then the solar AM is subtracted from the planet AM to achieve the same inertial frame.
The following graph (Figure 16) displays a divergence between solar and planet orbital AM. A future study will be performed with G.E. Pease further outlining this pro- cedure. Extending this graph back over the whole Little Ice Age may prove interesting, possibly showing us an- other method of identifying solar slow down by studying the planetary AM and its relationship with solar AM.
Some big questions remain.
7. Conclusions and Predictions
The correlation of the inverted AM values with the ex- isting sunspot record, along with the quantification of AMP events provides a platform for future sunspot pre- diction out to 3000AD. Cycles 24 & 25 are predicted to be less than 50SSN using the Layman’s Sunspot Count (based on the SIDC values but ignoring specks rated lower than 23 pixels). Solar cycle 20 was the first stage of the current AMP group that failed to generate a full grand minimum. This stems from the very weak AMP event caused by the late timing of the Uranus/Neptune conjunction and the failed Wilson’s Test. The current AMP group does not display a third event that is ex- tremely rare and hence will allow a modest recovery during solar cycle 26 (Figure 17). Looking out further, the next 1000 years do not show any major chances for deep grand minima that should provide stable conditions for future generations, not withstanding the possible en- try into the next ice age (Figure 18).
Solar cycle 24 will need to reach maximum after March 2011 to comply with the Wilsons Test.
Further information on the Layman’s Sunspot Count can be found at: http://www.landscheidt.info/?q=node/50.
8. Acknowledgements
Special thanks go to G. E. Pease for confirming Carl Smith’s AM data and for the advice and input on inertial frames.
The author would also like to thank Nicola Scafetta for providing advice and the initial peer review.
Sol
ar A
M
5.00E+40
4.50E+40
4.00E+40
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3.00E+40
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Sun AM Planet AM
Sun AM vs Planet AM
3.13281870E+43
3.13281770E+43
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3.13281470E+43
3.13281370E+43
3.13281270E+43
3.13281170E+43
Pla
net A
M
1900- Jan-01
1913- Sep-10
1906- Nov-06
1920- Jul-10
1927-May-20
1934- Mar-24
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1947- Dec-01
1954-Oct-05
1961-Aug-09
1968-Jun-13
1975-Apr-18
1982-Feb-20
1988-Dec-25
1995-Oct-30
2002-Sep-03
2009-Jul-08
2016- May-12
2023- Mar-17
2041- Jan-26
2036- Nov-23
Year
Geoff Sharp, Gerry Nov 2009 www.landscheidt.info
Figure 16. Differences in orbital AM become clear when viewed in the correct inertial frame. Note the near constancy (smaller range of deviation from top to bottom) of the Planet AM after subtracting the solar AM. The Planet AM is now con- stant to six significant figures, whereas it was only constant to three significant figures before the inertial frame transforma- tion. We believe the residual variations in the seventh and higher significant digits may be the result of spin orbit coupling between the planetary orbits and solar rotation.
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4.90E+47
1780
4.40E+47
3.90E+47
3.40E+47
2.90E+47
2.40E+47
1.90E+47
1791
1802
1813
1824
1835
1846
1857
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19
68
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01
2012
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2034
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2056
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2078
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2100
2111
2122
2133
2144
2155
2166
2177
2188
2199
= grand minimum affected cycle = grand minimum producing cycle (possible)
Angular Momentum
Angular Momentum & Past/Future Solar Activity Geoff Sharp June 2009 www.landscheidt.info
Neptune/Uranus opposing Neptune/Uranus opposing
Past Solar Activity Predicted Solar Activity
Figure 17. 200-year solar cycle prediction. The trough in the sunspot record coinciding with the opposition of Uranus & Nep- tune in past records and is expected to remain the same. Solar proxy records do not show high solar activity during times of low AM (Figures 5 & 7). The length of each future solar cycle remains unknown and predicted solar cycles should be taken as a guide with the overall trend being important. AM timing does not seem to be related to solar cycle timing. Predictions are based on overall AM strength.
70
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14C vs Angular Momentum
Der
ived
SS
N
14C
GM Centre
2795
Geoff Sharp Sept 2009 www.landscheidt.info
MWP
wolf
Maunder
Landscheidt
Great Warming Plateau
Sporer
Dalton
Figure 18. Earth’s future climate based on the projected solar activity using the same method as described in the chapter headed “Determining AMP Strength”. Deep grand minima are not expected. GM centre refers to the central AMP event oc- curring each 172 years on average, all AMP events in that group are totalled.
The SIM diagram (Figure 3) produced with software made available by Carsten Arnholm.
The data and main concepts were first published online 6
November 2008 at http://landscheidt.wordpress.com/2008/ 11/06/are-neptune-and-uranus-the-major-players-in-solar-grand-minima/. This document is a summary of many articles published at http://landscheidt.wordpress.com and http:// www.landscheidt.info.
REFERENCES [1] P. Jose, “Sun’s Motion and Sunspots,” Astronomical Jour-
nal, Vol. 70, 1965, pp. 193-200. doi:10.1086/109714
[2] T. Landscheidt, “New Little Ice Age Instead of Global Warming,” Energy and Environment, Vol. 14, No. 2-3, 2003, pp. 327-350.
[3] I. Charvàtovà, “Can Origin of the 2400-Year Cycle of Solar Activity Be Caused by Solar Inertial Motion?” Geo- physical Institute AS CR, Bocnõ II, Czech Republic, 2000.
[4] C. Smith, “Angular Momentum Graph,” 2007. http://landscheidt.wordpress.com/2007/06/01/dr-landscheidts-solar-cycle-24-prediction http://landscheidt.wordpress.com/6000-year-ephemeris
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diance during the Holocene,” Geophysical Research Let- ters, Vol. 36, No. 19, 2009, p. L19704. doi:10.1029/2009GL040142
[6] M. Stuiver, P. J. Reimer, E. Bard, J. W. Beck, G. S. Burr, K. A. Hughen, B. Kromer, G. McCormac, J. van der Plicht and M. Spurk, “INTCAL98 Radiocarbon Age Cali- bration, 24,000#0 cal BP,” Radiocarbon, Vol. 40, 1998, p. 1041#83.
[7] S. K. Solanki, I. G. Usoskin, B. Kromer, M. Schussler and J. Beer, “Unusual Activity of the Sun during Recent Decades Compared to the Previous 11,000 Years,” Na- ture, Vol. 431, No. 7012, 2004, pp. 1084-1087. ftp://ftp.ncdc.noaa.gov/pub/data/paleo/climate_forcing/solar_variability/solanki2004-ssn.txt
[8] I. Usoskin, S. Solanki and G. Kovaltsov, “Grand Minima and Maxima of Solar Activity: New Observational Con- straints,” Astronomy & Astrophysics Manuscript No. 7704, 2007.
[9] I. Wilson, B. Carter and I. A. Waite, “Does a Spin-Orbit
Coupling between the Sun and the Jovian Planets Govern the Solar Cycle?” Publications of the Astronomical Soci- ety of Australia, Vol. 25, No. 2, 2008, pp. 85-93. http://www.publish.csiro.au/?act=view_file&file_id=AS06018.pdf doi:10.1071/AS06018
[10] N. Scafetta, “Empirical Evidence for a Celestial Origin of the Climate Oscillations and Its Implications,” Journal of Atmospheric and Solar-Terrestrial Physics, Vol. 72, No. 13, 2010, pp. 951-970. http://yosemite.epa.gov/ee/epa/eed.nsf/vwpsw/360796B06E48EA0485257601005982A1#video doi:10.1016/j.jastp.2010.04.015
[11] D. Callebaut, V. Makarov and A. Tlatov, “Monopolar Structure of the Sun in between Polar Reversals and in Maunder Minimum,” Advances in Space Research, Vol. 40, No. 12, 2007, pp. 1917-1920.
[12] J. Javaraiah, SoPh, Vol. 212, 2003, p. 23.
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