Showing posts with label 1913. Show all posts
Showing posts with label 1913. Show all posts

Thursday, April 2, 2009

Deep Solar Minimum

Right on time the sunspot cycle is establishing minima. This time it appears to be as deep as last seen in 1913. Otherwise it is essentially good news as business as usual. A number of commentators have made contrarian predictions, but I see no reason to do that. Present evidence supports a rapid rise starting this year culminating in a peak three years hence on schedule. There is no reason to read anything whatsoever into present evidence.

We have seen the first few cycle 24 sunspots, and we can expect that come Christmas we will be seeing plenty more.

A number of commentators have pushed hard to police up the link between this cycle and global temperatures. My sense is that the link is real enough but been one of those factors whose effect is almost within the error range, it is devilishly difficult to separate. The fact that we seem to have decadal cycles in global climatic conditions is very suggestive but a little like trying to measure variable input heat flux in a pot by observing the boiling porridge. And yes, we are the boiling porridge.

The new news is simply that this minima is deeper than any recorded since the minima recorded in 1913. This means that we can compare the weather of the 1913 to 1924 with the weather of the next eleven years and properly determine comparability to perhaps winkle out specific variables not possible or convincing otherwise.

It is a decadal program but it should allow us to propose testable variables and outputs to test against all other sunspot cycles.

Deep Solar Minimum

04.01.2009

April 1, 2009: The sunspot cycle is behaving a little like the stock market. Just when you think it has hit bottom, it goes even lower.

2008 was a bear. There were no sunspots observed on 266 of the year's 366 days (73%). To find a year with more blank suns, you have to go all the way back to 1913, which had 311 spotless days:
plot. Prompted by these numbers, some observers suggested that the solar cycle had hit bottom in 2008.

Maybe not. Sunspot counts for 2009 have dropped even lower. As of March 31st, there were no sunspots on 78 of the year's 90 days (87%).
It adds up to one inescapable conclusion: "We're experiencing a very deep solar minimum," says solar physicist Dean Pesnell of the Goddard Space Flight Center.

"This is the quietest sun we've seen in almost a century," agrees sunspot expert David Hathaway of the Marshall Space Flight Center.

http://solarscience.msfc.nasa.gov/images/ssn_predict_l.gif


Above: The sunspot cycle from 1995 to the present. The jagged curve traces actual sunspot counts. Smooth curves are fits to the data and one forecaster's predictions of future activity. Credit: David Hathaway, NASA/MSFC.


Quiet suns come along every 11 years or so. It's a natural part of the sunspot cycle, discovered by German astronomer Heinrich Schwabe in the mid-1800s. Sunspots are planet-sized islands of magnetism on the surface of the sun; they are sources of solar flares, coronal mass ejections and intense UV radiation. Plotting sunspot counts, Schwabe saw that peaks of solar activity were always followed by valleys of relative calm—a clockwork pattern that has held true for more than 200 years:
plot.

The current solar minimum is part of that pattern. In fact, it's right on time. "We're due for a bit of quiet—and here it is," says Pesnell.

But is it supposed to be this quiet? In 2008, the sun set the following records:

A 50-year low in solar wind pressure: Measurements by the Ulysses spacecraft reveal a 20% drop in solar wind pressure since the mid-1990s—the lowest point since such measurements began in the 1960s. The solar wind helps keep galactic cosmic rays out of the inner solar system. With the solar wind flagging, more cosmic rays are permitted to enter, resulting in increased health hazards for astronauts. Weaker solar wind also means fewer geomagnetic storms and auroras on Earth.

A 12-year low in solar "irradiance": Careful measurements by several NASA spacecraft show that the sun's brightness has dropped by 0.02% at visible wavelengths and a whopping 6% at extreme UV wavelengths since the solar minimum of 1996. These changes are not enough to reverse the course of global warming, but there are some other, noticeable side-effects: Earth's upper atmosphere is heated less by the sun and it is therefore less "puffed up." Satellites in low Earth orbit experience less atmospheric drag, extending their operational lifetimes. That's the good news. Unfortunately, space junk also remains longer in Earth orbit, increasing hazards to spacecraft and satellites.

http://science.nasa.gov/headlines/y2009/images/deepsolarminimum/irradiance.jpg



Above: Space-age measurements of the total solar irradiance (brightness summed across all wavelengths). This plot, which comes from researcher C. Fröhlich, was shown by Dean Pesnell at the Fall 2008 AGU meeting during a lecture entitled "What is Solar Minimum and Why Should We Care?"

A 55-year low in solar radio emissions: After World War II, astronomers began keeping records of the sun's brightness at radio wavelengths. Records of 10.7 cm flux extend back all the way to the early 1950s. Radio telescopes are now recording the dimmest "radio sun" since 1955:
plot. Some researchers believe that the lessening of radio emissions is an indication of weakness in the sun's global magnetic field. No one is certain, however, because the source of these long-monitored radio emissions is not fully understood.

All these lows have sparked a debate about whether the ongoing minimum is "weird", "extreme" or just an overdue "market correction" following a string of unusually intense solar maxima.

"Since the Space Age began in the 1950s, solar activity has been generally high," notes Hathaway. "Five of the ten most intense solar cycles on record have occurred in the last 50 years. We're just not used to this kind of deep calm."

Deep calm was fairly common a hundred years ago. The solar minima of 1901 and 1913, for instance, were even longer than the one we're experiencing now. To match those minima in terms of depth and longevity, the current minimum will have to last at least another year.

In a way, the calm is exciting, says Pesnell. "For the first time in history, we're getting to see what a deep solar minimum is really like." A fleet of spacecraft including the Solar and Heliospheric Observatory (SOHO), the twin STEREO probes, the five THEMIS probes, ACE, Wind, TRACE, AIM, TIMED, Geotail and others are studying the sun and its effects on Earth 24/7 using technology that didn't exist 100 years ago. Their measurements of solar wind, cosmic rays, irradiance and magnetic fields show that solar minimum is much more interesting and profound than anyone expected.

Modern technology cannot, however, predict what comes next. Competing models by dozens of top solar physicists disagree, sometimes sharply, on when this solar minimum will end and how big the next solar maximum will be. Pesnell has surveyed the scientific literature and prepared a "
piano plot" showing the range of predictions. The great uncertainty stems from one simple fact: No one fully understands the underlying physics of the sunspot cycle.

Pesnell believes sunspot counts will pick up again soon, "possibly by the end of the year," to be followed by a solar maximum of below-average intensity in 2012 or 2013.

But like other forecasters, he knows he could be wrong. Bull or bear? Stay tuned for updates.

Tuesday, December 23, 2008

Global Coal Reserves

This piece surprised me because it challenges the integrity of reported reserves by government agencies. He is saying that historically governments have seriously overstated coal reserves and that this process continues.

I beg to differ. Governments will report a resource rather than a reserve. The resource is the total amount of material that might or could be mined regardless of cost. Canada has a 1.7 trillion barrel resource in the tar sands. It has a reserve of 175 billion barrels economically available for now.

Once cost becomes an issue we are talking about reserves. These measure what can be reasonably mined in view of current costs and selling prices. A lot of perfectly good coal will get reclassified as rock.

The one thing that I learned about the mining industry is perfectly good ore reserves turn into rock amazingly often. In fact we are living through one such transition right now.

Double the selling price of coal and I am sure that vast new resources will spring up. Let me put this another way. I have inspected my share of oil drilling logs. Every so often another coal seam will be typically encountered since we normally drill in sedimentary basins. They are all too deep to ever consider mining for the present. None of these are ever even counted as resources.

It is obvious that the USA can double their resource estimate by the simple expedient of measuring deeper. At least it would be more ethical than the resources added by OPEC.
And a note on that. Few understand that the first two discovery wells in a new field plus seismic has proven sufficient to define proven oil reserves. It is very unlikely that later work will significantly increase that figure. In fact the reverse is likely. Those vast new OPEC reserves announced in the eighties did not coincide with new field discoveries. Therefore they are fairy tales.

World Coal Reserves Could Be a Fraction of Previous Estimates

By Alexis Madrigal December 17, 2008 6:29:35 PMCategories: AGU 2008, Clean Tech, Energy, Geology

SAN FRANCISCO — A new calculation of the world's coal reserves is much lower than previous estimates. If validated, the new info could have a massive impact on the fate of the planet's climate.

That's because
coal is responsible for most of the CO2 emissions that drive climate change. If there were actually less coal available for burning, climate modelers would have to rethink their estimates of the level of emissions that humans will produce.

The new model, created by Dave Rutledge, chair of Caltech's engineering and applied sciences division, suggests that humans will only pull up a total — including all past mining — of 662 billion tons of coal out of the Earth. The best previous estimate, from the World Energy Council, says that the world has almost 850 billion tons of coal still left to be mined.

"Every estimate of the ultimate coal resource has been larger," said ecologist Ken Caldeira of Stanford University, who was not involved with the new study. "But if there's much less coal than we think, that's good news for climate."

The carbon dioxide emitted when humans burn coal to create usable energy is primarily responsible for global warming. Leading scientists think that the stability of Earth's climate will be dictated by how the world uses — or doesn't use — its coal resources. And the thinking has been that the world has more than enough coal to wreak catastrophic damage to the climate system, absent major societal or governmental changes.

So the new estimate, which opens the slim possibility that humankind could do nothing to mitigate carbon dioxide emissions and still escape some of the impacts of climate change, comes as quite a shock.

Rutledge argues that governments are terrible at estimating their own fossil fuel reserves. He developed his new model by looking back at historical examples of fossil fuel exhaustion. For example, British coal production fell precipitously form its 1913 peak. American oil production famously peaked in 1970, as controversially predicted by King Hubbert. Both countries had heartily overestimated their reserves.

It was from manipulating the data from the previous peaks that Rutledge developed his new model, based on fitting curves to the cumulative production of a region. He says that they provide much more stable estimates than other techniques and are much more accurate than those made by individual countries.

"The record of geological estimates made by governments for their fossil fuel estimates is really horrible," Rutledge said during a press conference at the American Geological Union annual meeting. "And the estimates tend to be quite high. They over-predict future coal production."

More specifically, Rutledge says that big surveys of natural resources underestimate the difficulty and expense of getting to the coal reserves of the world. And that's assuming that the countries have at least tried to offer a real estimate to the international community. China, for example, has only submitted two estimates of its coal reserves to the World Energy Council — and they were wildly different.

"The Chinese are interested in producing coal, not figuring out how much they have," Rutledge said. "That much is obvious."

The National Research Council's Committee on Coal Research, Technology, and Resource Assessments to Inform Energy Policy actually agrees with many of Rutledge's criticisms, while continuing to maintain far sunnier estimates of the recoverable stocks of American coal.

"Present estimates of coal reserves are based upon methods that have not been reviewed or revised since their inception in 1974, and much of the input data were compiled in the early 1970’s,"
the committee wrote in a 2007 report. "Recent programs to assess reserves in limited areas using updated methods indicate that only a small fraction of previously estimated reserves are actually mineable reserves.”

And don't look to technology to bail out coal miners. Mechanization has actually decreased the world's recoverable reserves, because huge mining machines aren't quite as good at digging out coal as human beings are.

With Rutledge's new numbers, the world could burn all the coal (and other fossil fuels) it can get to, and the atmospheric concentration of CO2 would only end up around 460 parts per million, which is predicted to cause a 2-degree-Celsius rise in global temperatures.

For many scientists, that's too much warming. A growing coalition is calling for limiting the CO2 in the atmosphere to 350 parts per million, down from the 380 ppm of today, but it's a far cry from some of the more devastating scenarios devised by the Intergovernmental Panel on Climate Change.

"Coal emissions really need to be phased out proactively — we can't just wait for them to run out — by the year 2030," said Pushker Kharecha, a scientist at NASA's Goddard Institute for Space Studies. "There is more than enough coal to keep CO2 well above 350 ppm well beyond this century."

The Intergovernmental Panel on Climate Change uses economic models that assume that the world will not run out of coal. Some IPCC scenarios show 3.4 billion tons of coal being burned just through 2100.
That's more than five times what Rutledge thinks will be possible — and a good deal higher than the WEC's estimate for recoverable coal reserves, too.

On the other hand, if the world were really to encounter a swift and steep decline in accessible coal resources, it's unclear how humans could retain our current levels of transportation, industry and general energy-usage.

So, even if coal were to run out and the most dangerous climate change averted, the imperative to develop non–fossil-fuel energy sources would remain.

"Peak Oil and peak gas and peak coal could really go either way for the climate," Kharecha said. "It all depends
on choices for subsequent energy sources."