Feature Article: Macro and Asset Allocation Implications of Environmental Trends and Uncertainties
Context
We first wrote about the potential relationships between the evolution of environmental uncertainties and future asset class valuations in 2006 (“Climate Change and Asset Allocation”), shortly after the Stern Review (“The Economics of Climate Change”) was published by the UK Treasury. Thirteen years later, this column will review key macro trends and uncertainties related to the environment, alternative scenarios their interactions could produce, and the implications for asset class valuation and portfolio allocation.
Before delving in, it is critical that we place environmental issues in their proper, and much broader context.
In “The Natural Science Underlying Big History”, the astrophysicist Eric Chaisson concludes that, “A wealth of observational data supports the hypothesis that increasingly complex systems evolve unceasingly, uncaringly, and unpredictably from big bang to humankind. These are global history greatly extended, big history with a scientific basis, and natural history broadly portrayed across ∼14 billion years of time…”
“Quantitative models and experimental tests imply that a remarkable simplicity underlies the emergence and growth of complexity for a wide spectrum of known and diverse systems. Energy is a principal facilitator of the rising complexity of ordered systems within the expanding Universe; energy flows are as central to life and society as they are to stars and galaxies…Rising energy expenditure per capita has been a hallmark in the origin, development, and evolution of humankind…In particular, energy rate density [energy flow per unit of time per unit of mass or area] is an objective metric suitable to gauge relative degrees of complexity among a hierarchy of widely assorted physical, biological, and cultural systems observed throughout the material Universe. Operationally, those systems capable of utilizing optimum amounts of energy tend to survive, and those that cannot are non-randomly eliminated…”
In sum, environmental issues are inextricably bound up in the larger context of energy issues, which are deeply embedded in fundamental technological, economic, national security, social, and political dynamics.
Starting Points
According to NASA, crude global temperature records have only been available since around 1880. And since even today temperature sensors are not evenly distributed around the globe, even today’s global average temperature data remain somewhat noisy estimates. Yet even taking that into account, the evidence indicates that average global temperature has been increasing, at an accelerating rate.
NASA estimates that between 1880 and 2018, average global temperature increased by 0.8 degrees Celsius, or 1.4 degrees Fahrenheit. Moreover, two thirds of this increase has occurred since 1975.
Two hypothesis have been suggested to explain this increase. The first is solar cycles, the most recent of which is coming to its end. It is speculated that the next cycle may be a multicycle minimum (e.g., with low sunspot activity), which, all else being equal, could reduce average global temperatures by 0.3 degrees Celsius.
While solar cycles clearly had an impact, their impact is not sufficient to fully account for the observed rise in average temperature. For example, examination of extremely old ice cores, and other paleohistory techniques, have demonstrated an association throughout the earth’s history of increases in atmospheric and ocean CO2 levels (e.g., due to volcanic activity) with increases in temperatures. However, the operation of the earth’s climate system is extremely complex, with multiple feedback loops and non-linearities at work. Put differently, modeling the world climate system is extremely challenging, and all conclusions contain a degree of uncertainty (which the International Panel on Climate Change – the IPCC – is now expressing systematically).
The inability of solar cycles to fully explain the observed temperature change, and the findings from studies of the earth’s history led to the second hypothesis, that human actions have also had a substantial impact. In particular, this hypothesis has strongly focused on the burning of fossil fuels as a major contributor to the significant increase in carbon dioxide (CO2) and other so-called “greenhouse gases” in the earth’s atmosphere. Specifically, from a pre-industrial age estimated level of 280 parts per million, atmospheric CO2 had reached 407 ppm by 2018. Again, this has been increasing at an accelerating rate, from about 1.0 ppm per year in 1969, to 2.0ppm by 2005, and 2.5ppm most recently. This has been caused not only by accelerating production of CO2 and other GHG emissions, but also a slowdown in the rate at which oceans absorb CO2 from the atmosphere (and in the process become more acidic).
This “anthropogenic” hypothesis has led to calls for restricting CO2 and other GHG emissions, largely by reducing the burning of fossil fuels to generate energy. Most recently, the IPCC has urged policymakers to limit the observed rise in temperature to 1.5 degrees Celsius above the pre-industrial level.
Critical Uncertainties
First, what are the most important potential macro impacts if GHG emissions and average global temperature levels continue to increase?
Extreme heat days are 4.0c hotter rather than 3.0c hotter, and associated reductions in human morbidity and mortality from extreme heat;
Higher frequency and severity of drought in some regions and extreme precipitation events in others;
Potentially lower climate-driven global migration flows;
A reduction of .1 meter (4 inches) in average sea level rise versus the .26 - .77 meter rise (10” to 30”) predicted if average temperatures increase by 2.0 degrees Celsius;
Reduced intensity of wildfires;
Less permafrost thawing;
Reduced spread of invasive species and vector born diseases from hot climates (e.g., malaria and dengue fever);
Reduced increase in ocean acidity and an estimated reduction of 2% rather than 4% in the aggregate annual fisheries catch; and
A lower reduction in global crop yield declines (forecast at 2% - 6% per decade at a 2 degree increase).
Second,to what extent are we theoretically able to reduce GHG emissions and limit the increase in average global temperature?