Review Article | Open Access
Gerald E. Marsh, "Interglacials, Milankovitch Cycles, Solar Activity, and Carbon Dioxide", Journal of Climatology, vol. 2014, Article ID 345482, 7 pages, 2014. https://doi.org/10.1155/2014/345482
Interglacials, Milankovitch Cycles, Solar Activity, and Carbon Dioxide
The existing understanding of interglacial periods is that they are initiated by Milankovitch cycles enhanced by rising atmospheric carbon dioxide concentrations. During interglacials, global temperature is also believed to be primarily controlled by carbon dioxide concentrations, modulated by internal processes such as the Pacific Decadal Oscillation and the North Atlantic Oscillation. Recent work challenges the fundamental basis of these conceptions.
The history  of the role of carbon dioxide in climate begins with the work of Tyndall  in 1861 and later in 1896 by Arrhenius . The conception that carbon dioxide controlled climate fell into disfavor for a variety of reasons until it was revived by Callendar  in 1938. It came into full favor after the work of Plass in the mid-1950s. Unlike what was believed then, it is known today that, for Earth’s present climate, water vapor is the principal greenhouse gas with carbon dioxide playing a secondary role.
Climate models nevertheless use carbon dioxide as the principal variable while water vapor is treated as a feedback. This is consistent with, but not mandated by, the assumption that—except for internal processes—the temperature during interglacials is dependent on atmospheric carbon dioxide concentrations. It now appears that this is not the case: interglacials can have far higher global temperatures than at present with no increase in the concentration of this gas.
2. Glacial Terminations and Carbon Dioxide
Even a casual perusal of the data from the Vostok ice core shown in Figure 1 gives an appreciation of how temperature and carbon dioxide concentration change synchronously. (Temperature is given in terms of relative deviations of a ratio of oxygen isotopes from a standard. δ18O means δ18O = /, measured in parts per thousand (). See R. S. Bradley, Paleoclimatology (Harcourt Academic Press, New York, 1999).) The role of carbon dioxide concentration in the initiation of interglacials, during the transition to an interglacial, and its control of temperature during the interglacial is not yet entirely clear.
Between glacial and interglacial periods, the concentration of atmospheric carbon dioxide varies between about 200 and 280 p.p.m.v., being at ~280 p.p.m.v. during interglacials. The details of the source of these variations is still somewhat controversial, but it is clear that carbon dioxide concentrations are coupled and in equilibrium with oceanic changes . The cause of the glacial to interglacial increase in atmospheric carbon dioxide is now thought to be due to changes in ventilation of deep water at the ocean surface around Antarctica and the resulting effect on the global efficiency of the “biological pump” . If this is indeed true, then a perusal of the interglacial carbon dioxide concentrations shown in Figure 1 tells us that the process of increased ventilation coupled with an increasingly productive biological pump appears to be self-limiting during interglacials, rising little above ~280 p.p.m.v., despite warmer temperatures in past interglacials. This will be discussed more extensively below.
The above mechanism for glacial to interglacial variation in carbon dioxide concentration is supported by the observation that the rise in carbon dioxide lags the temperature increase by some 800–1000 years—ruling out the possibility that rising carbon dioxide concentrations were responsible for terminating glacial periods. As a consequence, it is now generally believed that glacial periods are terminated by increased insolation in polar regions due to quasiperiodic variations in the Earth’s orbital parameters. And it is true that paleoclimatic archives show spectral components that match the frequencies of Earth’s orbital modulation. This Milankovitch insolation theory has a number of problems associated with it , and the one to be discussed here is the so called “causality problem”; that is, what came first—increased insolation or the shift to an interglacial. This would seem to be the most serious objection, since if the warming of the Earth preceded the increased insolation, it could not be caused by it. This is not to say that Milankovitch variations in solar insolation do not play a role in changing climate, but they could not be the principal cause of glacial terminations.
Figure 2 shows the timing of the termination of the penultimate ice age (Termination II) some 140 thousand years ago. The data shown is from Devils Hole (DH), Vostok, and the δ18O SPECMAP record (The acronym stands for Spectral Mapping Project.). The DH-11 record shows that Termination II occurred at ka; the Vostok record gives ka; and the SPECMAP gives ka . The latter is clearly not consistent with the first two. The reason has to do with the origin of the SPECMAP time scale.
The SPECMAP record was constructed by averaging δ18O data from five deep-sea sediment cores. The result was then correlated with the calculated insolation cycles over the last 800,000 years. This procedure serves well for many purposes, but, as can be seen from Figure 2, sea levels were at or above modern levels before the rise in solar insolation often thought to initiate Termination II. The SPECMAP chronology must therefore be adjusted when comparisons are made with records not being dependent on the SPECMAP timescale.
The above considerations imply that Termination II was not initiated by an increase in carbon dioxide concentration or increased insolation. The question then remains what did initiate Termination II?
A higher time-resolved view of the timing of glacial Termination II is shown in Figure 3 from Kirkby et al. . What these authors found was that “the warming at the end of the penultimate ice age was underway at the minimum of 65°N June insolation, and essentially complete about 8 kyr prior to the insolation maximum.” In this figure, the Visser et al. data and the galactic cosmic ray rate are shifted to an 8 kyr earlier time to correct for the SPECMAP time scale upon which they are based. As discussed above, the SPECMAP timescale is tuned to the insolation cycles.
The galactic cosmic ray flux—using an inverted scale—is also shown in the figure. The most striking feature is that the data strongly imply that Termination II was initiated by a reduction in cosmic ray flux. Such a reduction would lead to a reduction in the amount of low-altitude cloud cover, as discussed below, thereby reducing the Earth’s albedo with a consequent rise in global temperature .
There is another compelling argument that can be given to support this hypothesis. Sime et al.  have found that past interglacial climates were much warmer than previously thought. Their analysis of the data shows that the maximum interglacial temperatures over the past 340 kyr were between 6°C and 10°C above present day values. From Figure 1, it can be seen that past interglacial carbon dioxide concentrations were not higher than those of the current interglacial, and therefore carbon dioxide could not have been responsible for this warming. In fact, the concentration of carbon dioxide that would be needed to produce a 6–10°C rise in temperature above present day values exceeds the maximum (1000 p.p.m.v.) for the range of validity of the usual formula used to calculate the forcing in response to such an increase.
In addition, it should be noted that the fact that carbon dioxide concentrations were not higher during periods of much warmer temperatures confirms the self-limiting nature of the process driving the rise of carbon dioxide concentration during the transition to interglacials; that is, where an increase in the ventilation of deep water at the surface of the Antarctic ocean and the resulting effect on the efficiency of the biological pump cause the glacial to interglacial rise carbon dioxide.
3. Past Interglacials, Albedo Variations, and Cosmic Ray Modulation
If it is assumed that solar irradiance during past interglacials was comparable to today’s value as is assumed in the Milankovitch theory, it would seem that the only factor left—after excluding increases in insolation or carbon dioxide concentrations—that could be responsible for the glacial to interglacial transition is a change in the Earth’s albedo. During glacial periods, the snow and ice cover could not melt without an increase in the energy entering the climate system. This could occur if there was a decrease in albedo caused by a decrease in cloud cover.
The Earth’s albedo is known to be correlated with galactic cosmic-ray flux. This relationship is clearly seen over the eleven-year cycle of the sun as shown in Figure 4, which shows a very strong correlation between galactic cosmic rays, solar irradiance, and low cloud cover. Note that increased lower cloud cover (implying an increased albedo) closely follows cosmic ray intensity.
It is generally understood that the variation in galactic cosmic ray flux is due to changes in the solar wind associated with solar activity. The sun emits electromagnetic radiation and energetic particles known as the solar wind. A rise in solar activity—as measured by the sun spot cycle—affects the solar wind and the interplanetary magnetic field by driving matter and magnetic flux trapped in the plasma of the local interplanetary medium outward, thereby creating what is called the heliosphere and partially shielding this volume, which includes the earth, from galactic cosmic rays—a term used to distinguish them from solar cosmic rays, which have much less energy.
When solar activity decreases, with a consequent small decrease in irradiance, the number of galactic cosmic rays entering the Earth’s atmosphere increases as does the amount of low cloud cover. This increase in cloud cover results in an increase in the Earth’s albedo, thereby lowering the average temperature. The sun’s 11-year cycle is therefore not only associated with small changes in irradiance but also with changes in the solar wind, which in turn affect cloud cover by modulating the cosmic ray flux. This, it is argued, constitutes a strong positive feedback needed to explain the significant impact of small changes in solar activity on climate. Long-term changes in cloud albedo would be associated with long-term changes in the intensity of galactic cosmic rays.
The great sensitivity of climate to small changes in solar activity is corroborated by the work of Bond et al., who have shown a strong correlation between the cosmogenic nuclides 14C and 10Be and centennial to millennial changes in proxies for drift ice as measured in deep-sea sediment cores covering the Holocene time period . The production of these nuclides is related to the modulation of galactic cosmic rays, as described above. The increase in the concentration of the drift ice proxies increases with colder climates . These authors conclude that Earth’s climate system is highly sensitive to changes in solar activity.
For cosmic ray driven variations in albedo to be a viable candidate for initiating glacial terminations, cosmic ray variations must show periodicities comparable to those of the glacial/interglacial cycles. The periodicities are shown in Figure 5 taken (a) from Kirkby et al.  and (b) from Schulz and Zeebe . Figure 5(a) is derived from the galactic cosmic ray flux—shown in Figure 6—over the last 220 kyr.
The mechanism for the modulation of cosmic ray flux discussed above was tied to solar activity, but the 41 kyr and 100 kyr cycles seen in Figure 5(a) correspond to the small quasiperiodic changes in the Earth’s orbital parameters underlying the Milankovitch theory. For these same variations, to affect cosmic ray flux, they would have to modulate the geomagnetic field or the shielding due to the heliosphere. Although the existence of these periodicities and the underlying mechanism are still somewhat controversial, the lack of a clear understanding of the underlying theory does not negate the fact that these periodicities do occur in galactic cosmic ray flux.
If cosmic ray driven albedo change is responsible for Termination II and a lower albedo was also responsible for the warmer climate of past interglacials, rather than higher carbon dioxide concentrations, the galactic cosmic ray flux would have had to be lower during past interglacials than it is during the present one. That this appears to be the case is suggested by the record in Figure 6 (note inverted scale).
Reconstructions of solar activity on the temporal scale of Figure 6 are based on records of the cosmogenic radionuclides 14C and 10Be and must be corrected for geomagnetic variations. Using physics-based models , solar activity can now be reconstructed over many millennia. The longer the time period, the greater the uncertainty due to systematic errors.
The appearance of the 100 ky and 41 ky periods in the galactic cosmic ray flux of Figure 5(a) is somewhat surprising. With regard to orbital forcing of the geomagnetic field intensity, Frank  has stated that “Despite some indications from spectral analysis, there is no clear evidence for a significant orbital forcing of the paleointensity signals,” although there were some caveats. In terms of the galactic cosmic ray flux, Kirkby et al.  maintain that “… previous conclusions that orbital frequencies are absent were premature.” An extensive discussion of “Interstellar-Terrestrial Issues” has also been given by Scherer et al. .
Using the fact that the galactic cosmic ray flux incident on the heliosphere boundary is known to have remained close to constant over the last 200 kyr and that there exist independent records of geomagnetic variations over this period, Sharma  was able to use a functional relation reflecting the existing data to give a good estimate of solar activity over this 200 kyr period. The atmospheric production rate of 10Be depends on the geomagnetic field intensity and the solar modulation factor—the energy lost by cosmic ray particles traversing the heliosphere to reach the Earth’s orbit (this is also known as the “heliocentric potential,” an electric potential centered on the sun, which is introduced to simplify calculations by substituting electrostatic repulsion for the interaction of cosmic rays with the solar wind).
If is the average production rate of 10Be, the geomagnetic field strength, and the solar modulation factor, the functional relation between the data used by Sharma is where the subscript “0” corresponds to present day values. By setting these equal to unity, the normalized expression simplifies to
Using (2) and a globally stacked record of relative geomagnetic field intensity from marine sediments, as well as a globally stacked, 230Th-normalized 10Be record from deep marine sediments, Sharma was able to calculate the normalized solar modulation factor over the last 200 kyr. (“Stacked” means aligned with respect to important stratigraphic features but without a timescale.) The result is shown in Figure 8.
The 100 kyr periodicity is readily apparent in Figure 8. It is also seen that the δ18O record and solar modulation are coherent and in phase. Sharma concludes from this that “... variations in solar surface magnetic activity cause changes in the Earth’s climate on a 100 ka timescale.”
Variations of solar activity over tens to hundreds of thousands of years do not seem to be a feature of the standard solar model. Ehrlich,  however, has developed a modification of the model based on resonant thermal diffusion waves which shows many of the details of the paleotemperature record over the last 5 million years. This includes the transition from glacial cycles having a 41 kyr period to a ~100 kyr period about 1 Myr ago. While the model has some problems—as noted by the author—the work shows that a reasonable addition to the standard solar model could help explain the long-term paleotemperature record. However, the fact that ice ages did not begin until some 2.75 million years ago, when atmospheric carbon dioxide concentration levels fell to values comparable to today, tells us that solar variations consistent with Ehrlich’s model did not significantly affect climate before this oscillatory phase of climate began .
It has been shown above that low-altitude cloud cover closely follows cosmic ray flux; that the galactic cosmic ray flux has the periodicities of the glacial/interglacial cycles; that a decrease in galactic cosmic ray flux was coincident with Termination II; and that the most likely initiator for Termination II was a consequent decrease in Earth’s albedo.
The temperature of past interglacials was higher than today most likely as a consequence of a lower global albedo due to a decrease in galactic cosmic ray flux reaching the Earth’s atmosphere. In addition, the galactic cosmic ray intensity exhibits a 100 kyr periodicity over the last 200 kyr which is in phase with the glacial terminations of this period. Carbon dioxide appears to play a very limited role in setting interglacial temperature.
Conflict of Interests
The author declares that there is no conflict of interests regarding the publication of this paper.
- An excellent summary of this history is available in the January-February 2010 issue of the American Scientist. This issue reprints portions of Gilbert Plass' 1956 article in the magazine along with two commentaries. See this article for the references to scientific and more popular articles by Plass from the period 1953–1955.
- J. Tyndall, “On the absorption and radiation of heat by gases and vapours; on the physical connection of radiation, absorption, and conduction,” Philosophical Magazine, Series 4, vol. 22, no. 169–194, pp. 273–285, 1861.
- S. Arrhenius, “On the influence of carbonic acid in the air upon the temperature of the ground,” Philosophical Magazine, vol. 4, pp. 237–276, 1896.
- G. S. Callendar, “The artificial production of carbon dioxide and its influence on temperature,” Quarterly Journal of the Royal Meteorological Society, vol. 64, pp. 223–240, 1938.
- W. S. Broecker, “Glacial to interglacial changes in ocean chemistry,” Progress in Oceanography, vol. 11, no. 2, pp. 151–197, 1982.
- D. M. Sigman and E. A. Boyle, “Glacial/interglacial variations in atmospheric carbon dioxide,” Nature, vol. 407, no. 6806, pp. 859–869, 2000.
- D. B. Karner and R. A. Muller, “Paleoclimate: a causality problem for Milankovitch,” Science, vol. 288, no. 5474, pp. 2143–2144, 2000.
- I. J. Winograd, T. B. Coplen, J. M. Landwehr et al., “Continuous 500,000-year climate record from vein calcite in Devils Hole, Nevada,” Science, vol. 258, no. 5080, pp. 255–260, 1992.
- J. Kirkby, A. Mangini, and R. A. Muller, “The glacial cycles and cosmic rays,” Tech. Rep. CERN-PH-EP/2004-027, http://arxiv.org/abs/physics/0407005.
- K. S. Carslaw, R. G. Harrison, and J. Kirkby, “For a discussion of the phenomenology behind galactic cosmic ray intensity and cloud formation,” Science, vol. 298, p. 1732, 2002.
- L. C. Sime, E. W. Wolff, K. I. C. Oliver, and J. C. Tindall, “Evidence for warmer interglacials in East Antarctic ice cores,” Nature, vol. 462, no. 7271, pp. 342–345, 2009.
- G. Bond, B. Kromer, J. Beer et al., “Persistent solar influence on north atlantic climate during the Holocene,” Science, vol. 294, no. 5549, pp. 2130–2136, 2001.
- G. Bond, W. Showers, M. Cheseby et al., “A pervasive millennial-scale cycle in North Atlantic Holocene and glacial climates,” Science, vol. 278, no. 5341, pp. 1257–1266, 1997.
- K. G. Schulz and R. E. Zeebe, “Pleistocene glacial terminations triggered by synchronous changes in Southern and Northern Hemisphere insolation: the insolation canon hypothesis,” Earth and Planetary Science Letters, vol. 249, no. 3-4, pp. 326–336, 2006.
- I. G. Usoskin, “A history of solar activity over millennia,” Living Reviews in Solar Physics, vol. 5, no. 3, 2008.
- M. Frank, “Comparison of cosmogenic radionuclide production and geomagnetic field intensity over the last 200 000 years,” Philosophical Transactions of the Royal Society A, vol. 358, no. 1768, pp. 1089–1107, 2000.
- K. Scherer, H. Fichtner, T. Borrmann et al., “Interstellar-terrestrial relations: variable cosmic environments, the dynamic heliosphere , and their imprints on terrestrial archives and climate,” Space Science Reviews, vol. 127, no. 1–4, pp. 327–465, 2006.
- M. Sharma, “Variations in solar magnetic activity during the last 200 000 years: is there a Sun-climate connection?” Earth and Planetary Science Letters, vol. 199, no. 3-4, pp. 459–472, 2002.
- J. Masarik and J. Beer, “Simulation of particle fluxes and cosmogenic nuclide production in the Earth's atmosphere,” Journal of Geophysical Research D, vol. 104, no. 10, pp. 12099–12111, 1999.
- R. Ehrlich, “Solar resonant diffusion waves as a driver of terrestrial climate change,” Journal of Atmospheric and Solar-Terrestrial Physics, vol. 69, pp. 759–766, 2007.
- G. E. Marsh, “Climate stability and policy: a synthesis,” Energy & Environment, vol. 22, no. 8, pp. 1085–1090, 2008.
- J. R. Petit, J. Jouzel, D. Raynaud et al., “Climate and atmospheric history of the past 420,000 years from the Vostok ice core, Antarctica,” Nature, vol. 399, no. 6735, pp. 429–436, 1999.
- M. Christl, C. Strobl, and A. Mangini, “Beryllium-10 in deep-sea sediments: a tracer for the Earth's magnetic field intensity during the last 200,000 years,” Quaternary Science Reviews, vol. 22, no. 5–7, pp. 725–739, 2003.
- G. M. Henderson and N. C. Slowey, “Evidence from U-Th dating against Northern Hemisphere forcing of the penultimate deglaciation,” Nature, vol. 404, no. 6773, pp. 61–66, 2000.
- C. D. Gallup, H. Cheng, F. W. Taylor, and R. L. Edwards, “Direct determination of the timing of sea level change during Termination II,” Science, vol. 295, pp. 310–313, 2002.
- K. Visser, R. Thunell, and L. Stott, “Magnitude and timing of temperature change in the Indo-Pacific warm pool during deglaciation,” Nature, vol. 421, no. 6919, pp. 152–155, 2003.
Copyright © 2014 Gerald E. Marsh. 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.