THE 1859 SUPER SOLAR STORM THAT CAUSED HAVOC AROUND THE WORLD

Imagine what one would do to us in our technology driven world:


-Bracing the Satellite Infrastructure for a Solar Superstorm-

-A recurrence of the 1859 solar superstorm would be a cosmic Katrina, causing billions of dollars of damage to satellites, power grids and radio communications-


* The solar superstorm of 1859 was the fiercest ever recorded. Auroras filled the sky as far south as the Caribbean, magnetic compasses went haywire and telegraph systems failed.
* Ice cores suggest that such a blast of solar particles happens only once every 500 years, but even the storms every 50 years could fry satellites, jam radios and cause coast-to-coast blackouts.
* The cost of such an event justifies more systematic solar monitoring and beefier protection for satellites and the power grid.


As night was falling across the Americas on Sunday, August 28, 1859, the phantom shapes of the auroras could already be seen overhead. From Maine to the tip of Florida, vivid curtains of light took the skies. Startled Cubans saw the auroras directly overhead; ships’ logs near the equator described crimson lights reaching halfway to the zenith. Many people thought their cities had caught fire. Scientific instruments around the world, patiently recording minute changes in Earth’s magnetism, suddenly shot off scale, and spurious electric currents surged into the world’s telegraph systems. In Baltimore telegraph operators labored from 8 p.m. until 10 a.m. the next day to transmit a mere 400-word press report.

Just before noon the following Thursday, September 1, English astronomer Richard C. Carrington was sketching a curious group of sunspots—curious on account of the dark areas’ enormous size. At 11:18 a.m. he witnessed an intense white light flash from two locations within the sunspot group. He called out in vain to anyone in the observatory to come see the brief five-minute spectacle, but solitary astronomers seldom have an audience to share their excitement. Seventeen hours later in the Americas a second wave of auroras turned night to day as far south as Panama. People could read the newspaper by their crimson and green light. Gold miners in the Rocky Mountains woke up and ate breakfast at 1 a.m., thinking the sun had risen on a cloudy day. Telegraph systems became unusable across Europe and North America.

The news media of the day looked for researchers able to explain the phenomena, but at the time scientists scarcely understood auroral displays at all. Were they meteoritic matter from space, reflected light from polar icebergs or a high-altitude version of lightning? It was the Great Aurora of 1859 itself that ushered in a new paradigm. The October 15 issue of Scientific American noted that ‘‘a connection between the northern lights and forces of electricity and magnetism is now fully established.” Work since then has established that auroral displays ultimately originate in violent events on the sun, which fire off huge clouds of plasma and momentarily disrupt our planet’s magnetic field.

The impact of the 1859 storm was muted only by the infancy of our technological civilization at that time. Were it to happen today, it could severely damage satellites, disable radio communications and cause continent-wide electrical blackouts that would require weeks or longer to recover from. Although a storm of that magnitude is a comfortably rare once-in-500-years event, those with half its intensity hit every 50 years or so. The last one, which occurred on November 13, 1960, led to worldwide geomagnetic disturbances and radio outages. If we make no preparations, by some calculations the direct and indirect costs of another superstorm could equal that of a major hurricane or earthquake.

The Big One
The number of sunspots, along with other signs of solar magnetic activity, waxes and wanes on an 11-year cycle. The current cycle began this past January; over the coming half a decade, solar activity will ramp up from its current lull. During the previous 11 years, 21,000 flares and 13,000 clouds of ionized gas, or plasma, exploded from the sun’s surface. These phenomena, collectively termed solar storms, arise from the relentless churning of solar gases.

In some ways, they are scaled-up versions of terrestrial storms, with the important difference that magnetic fields lace the solar gases that sculpt and energize them. Flares are analogous to lightning storms; they are bursts of energetic particles and intense x-rays resulting from changes in the magnetic field on a relatively small scale by the sun’s standards, spanning thousands of kilometers. So-called coronal mass ejections (CMEs) are analogous to hurricanes; they are giant magnetic bubbles, millions of kilometers across, that hurl billion-ton plasma clouds into space at several million kilometers per hour.

Most of these storms result in nothing more than auroras dancing in the polar skies—the equivalent of a minor afternoon rainstorm on Earth. Occasionally, however, the sun lets loose a gale. No one living today has ever experienced a full-blown superstorm, but telltale signs of them have turned up in some surprising places. In ice-core data from Greenland and Antarctica, Kenneth G. McCracken of the University of Maryland has discovered sudden jumps in the concentration of trapped nitrate gases, which in recent decades appear to correlate with known blasts of solar particles. A nitrate anomaly found for 1859 stands out as the biggest of the past 500 years, with the severity roughly equivalent to the sum of all the major events of the past 40 years.

As violent as it was, the 1859 superstorm does not appear to have been qualitatively different from lesser events. The two of us, along with many other researchers, have reconstructed what happened back then from contemporary historical accounts as well as scaled-up measurements of milder storms in recent decades, which have been studied by modern satellites:

1. The gathering storm. On the sun, the preconditions for the 1859 superstorm involved the appearance of a large, near-equatorial sunspot group around the peak of the sunspot cycle. The sunspots were so large that astronomers such as Carrington could see them with the naked (but suitably protected) eye. At the time of the initial CME released by the storm, this sunspot group was opposite Earth, putting our planet squarely in the bull’s-eye. The sun’s aim need not be so exact, however. By the time a CME reaches Earth’s orbit, it typically has fanned out to a width of some 50 million kilometers, thousands of times wider than our planet.

2. First blast. The superstorm released not one but two CMEs. The first may have taken the customary 40 to 60 hours to arrive. The magnetometer data from 1859 suggest that the magnetic field in the ejected plasma probably had a helical shape. When it first hit Earth, the field was pointing north. In this orientation, the field reinforced Earth’s own magnetic field, which minimized its effects. The CME did compress Earth’s magnetosphere—the region of near-Earth space where our planet’s magnetic field dominates the sun’s—and registered at magnetometer stations on the ground as what solar scientists call a sudden storm commencement. Otherwise it went unnoticed. As plasma continued to stream past Earth, however, its field slowly spun around. After 15 hours, it opposed rather than reinforced Earth’s field, bringing our planet’s north-pointing and the plasma cloud’s south-pointing field lines into contact. The field lines then reconnected into a simpler shape, releasing huge amounts of stored energy. That is when the telegraph disruptions and auroral displays commenced. Within a day or two the plasma passed by Earth, and our planet’s geomagnetic field returned to normal.

3. X-ray flare. The largest CMEs typically coincide with one or more intense flares, and the 1859 superstorm was no exception. The visible flare observed by Carrington and others on September 1 implied temperatures of nearly 50 million kelvins. Accordingly, it probably emitted not only visible light but also x-rays and gamma rays. It was the most brilliant solar flare ever recorded, bespeaking enormous energies released into the solar atmosphere. The radiation hit Earth after the light travel time of eight and a half minutes, long before the second CME. Had shortwave radios existed, they would have been rendered useless by energy deposition in the ionosphere, the high-altitude layer of ionized gas that reflects radio waves. The x-ray energy also heated the upper atmosphere and caused it to bloat out by tens or hundreds of kilometers.

4. Second blast. Before the ambient solar-wind plasma had time to fill in the cavity formed by the passage of the first CME, the sun fired off a second CME. With little material to impede it, the CME reached Earth within 17 hours. This time the CME field pointed south as it hit, and the geomagnetic mayhem was immediate. Such was its violence that it compressed Earth’s magnetosphere (which usually extends about 60,000 kilometers) to 7,000 kilometers or perhaps even into the upper stratosphere itself. The Van Allen radiation belts that encircle our planet were temporarily eliminated, and huge numbers of protons and electrons were dumped into the upper atmosphere. These particles may have accounted for the intense red auroras seen in much of
the world.

5. Energetic protons. The solar flare and the intense CMEs also accelerated protons to energies of 30 million electron volts or higher. Across the Arctic, where Earth’s magnetic field affords the least protection, these particles penetrated to an altitude of 50 kilometers and deposited additional energy in the ionosphere. According to Brian C. Thomas of Washburn University, the proton shower from the 1859 superstorm reduced stratospheric ozone by 5 percent. The layer took four years to recover. The most powerful protons, with energies above one billion electron volts, reacted with the nuclei of nitrogen and oxygen atoms in the air, spawning neutrons and creating the nitrate abundance anomalies. A rain of neutrons reached the ground in what is now called a ground level event, but no human technology was available to detect this onslaught. Fortunately, it was not hazardous to health.

6. Massive electric currents. As the auroras spread from the usual high latitudes to low latitudes, the accompanying ionospheric and auroral electric currents induced intense, continent-spanning currents in the ground. These currents found their way into telegraph circuitry. The multiampere, high-voltage discharges caused near electrocutions and were reported to have burned down several telegraph stations.

Toasted Satellites
When a large geomagnetic storm happens again, the most obvious victims will be satellites. Even under ordinary conditions, cosmic-ray particles erode solar panels and reduce power generation by about 2 percent annually. Incoming particles also interfere with satellite electronics. Many communications satellites, such as Anik E1 and E2 in 1994 and Telstar 401 in 1997, have been compromised or lost in this way. A large solar storm can cause one to three years’ worth of satellite lifetime loss in a matter of hours and produce hundreds of glitches, ranging from errant but harmless commands to destructive electrostatic discharges.

To see how communications satellites might fare, we simulated 1,000 ways a superstorm might unfold, with intensities that varied from the worst storm of the Space Age (which occurred on October 20, 1989) to that of the 1859 superstorm. We found that the storms would not only degrade solar panels as expected but also lead to the significant loss of transponder revenue. The total cost would often exceed $20 billion. We assumed that satellite owners and designers would have mitigated the effects by maintaining plenty of spare transponder capacity and a 10 percent power margin at the time of their satellite’s launch. Under less optimistic assumptions, the losses would approach $70 billion, which is comparable to a year’s worth of revenue for all communications satellites. Even this figure does not include the collateral economic losses to the customers of the satellites.

Fortunately, geosynchronous communications satellites are remarkably robust against once-a-decade events, and their life spans have grown from barely five years in 1980 to nearly 17 years today. For solar panels, engineers have switched from silicon to gallium arsenide to increase power production and reduce mass. This move has also provided increased resistance to cosmic-ray damage. Moreover, satellite operators receive advanced storm warnings from the National Oceanic and Atmospheric Administration’s Space Weather Prediction Center, which allows them to avoid complex satellite maneuvers or other changes during the time when a storm may arrive. These strategies would doubtless soften the blow of a major storm. To further harden satellites, engineers could thicken the shielding, lower the solar panel voltages to lessen the risk of runaway electrostatic discharges, add extra backup systems and make the software more robust to data corruption.

It is harder to guard against other superstorm effects. X-ray energy deposition would cause the atmosphere to expand, enhancing the drag forces on military and commercial imaging and communications satellites that orbit below 600 kilometers in altitude. Japan’s Advanced Satellite for Cosmology and Astrophysics experienced just such conditions during the infamous Bastille Day storm on July 14, 2000, which set in motion a sequence of attitude and power losses that ultimately led to its premature reentry a few months later. During a superstorm, low-orbiting satellites would be at considerable risk of burning up in the atmosphere within weeks or months of the event.



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[link to www.scientificamerican.com]