October 23, 2003:
Newly uncovered scientific data of recorded history’s most massive space storm is helping a NASA scientist investigate its intensity and the probability that what occurred on Earth and in the heavens almost a century-and-a-half ago could happen again.
What happened in 1859 was a combination of several events that occurred on the Sun at the same time. If they took place separately they would be somewhat notable events. But together they caused the most potent disruption of Earth’s ionosphere in recorded history. “What they generated was the perfect space storm,” says Bruce Tsurutani, a plasma physicist at NASA’s Jet Propulsion Laboratory.
To begin to understand the perfect space storm you must first begin to understand the gargantuan numbers with which plasma physicists like Tsurutani work every day. At over 1.4 million kilometers (869,919 miles) wide, the Sun contains 99.86 percent of the mass of the entire solar system: well over a million Earths could fit inside its bulk. The total energy radiated by the Sun averages 383 billion trillion kilowatts, the equivalent of the energy generated by 100 billion tons of TNT exploding each and every second.
But the energy released by the Sun is not always constant. Close inspection of the Sun’s surface reveals a turbulent tangle of magnetic fields and boiling arc-shaped clouds of hot plasma dappled by dark, roving sunspots.
Once in a while–exactly when scientists still cannot predict–an event occurs on the surface of the Sun that releases a tremendous amount of energy in the form of a solar flare or a coronal mass ejection, an explosive burst of very hot, electrified gases with a mass that can surpass that of Mount Everest.
What transpired during the dog days of summer 1859, across the 150 million-kilometer (about 93 million-mile) chasm of interplanetary space that separates the Sun and Earth, was this: on August 28, solar observers noted the development of numerous sunspots on the Sun’s surface. Sunspots are localized regions of extremely intense magnetic fields. These magnetic fields intertwine, and the resulting magnetic energy can generate a sudden, violent release of energy called a solar flare. From August 28 to September 2 several solar flares were observed. Then, on September 1, the Sun released a mammoth solar flare. For almost an entire minute the amount of sunlight the Sun produced at the region of the flare actually doubled.
“With the flare came this explosive release of a massive cloud of magnetically charged plasma called a coronal mass ejection,” said Tsurutani. “Not all coronal mass ejections head toward Earth. Those that do usually take three to four days to get here. This one took all of 17 hours and 40 minutes,” he noted.
Not only was this coronal mass ejection an extremely fast mover, the magnetic fields contained within it were extremely intense and in direct opposition with Earth’s magnetic fields. That meant the coronal mass ejection of September 1, 1859, overwhelmed Earth’s own magnetic field, allowing charged particles to penetrate into Earth’s upper atmosphere. The end game to such a stellar event is one heck of a light show and more — including potential disruptions of electrical grids and communications systems.
We have to understand some indicators before the coming of superstorms , to anticipate what will happen in 2012.