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The tearing and reconnecting of magnetic field lines in the area surrounding sunspots triggers the explosions known as solar flares. The explosions rip electrons from the hydrogen gas in the Sun's corona and create hot, electrified gas called plasma. The plasma rises into the solar atmosphere along the solar magnetic field lines, forming fiery loops and arches. Plasma in the flares is heated to many millions of degrees Celsius.
The solar flares send enormous amounts of radiation racing towards Earth's atmosphere at the speed of light. They release radiation across the entire electromagnetic spectrum, from radio waves at the long-wavelength end to X-rays and gamma-rays at the short end. The radiation can disrupt electromagnetic signals used for satellite, radio, TV, and other broadcasts.
A strong solar storm like the one on July 14 may also spit out a long stream of particles called a coronal mass ejection, or CME. The electrified gas particles burst into space from the Sun's corona in a fierce solar wind at speeds that can exceed 2 million miles (3.2 million kilometers) per hour. A CME can carry as much as 10 billion tons of solar material into space.
Down to Earth
The weather in space can greatly affect Earth. Geomagnetic storms can trigger power blackouts and satellite failures. During the last solar cycle peak in 1989, millions of people lost electricity across Canada and the Northeast. In 1998, 45 million people lost their telephone pager service after solar wind particles caused the failure of a communications satellite.
NASA scientists must carefully check the
space weather forecast before scheduling astronaut space walks. An astronaut's radiation exposure is quadrupled during strong geomagnetic storms.
Air travelers flying at high altitudes in the polar regions, where Earth's magnetic fields are strongest, get a dose of radiation equal to that of a brief chest X-ray. Fortunately, the magnetic field acts as a shield to protect Earthlings on the surface from significant radiation exposure.
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The graph below shows how a solar explosion on June 6 affected the solar wind on June 8, as measured by a NASA satellite orbiting Earth. The solar wind speed is shown on the y-axis in kilometers per second, and time is shown on the x-axis. (The time is calculated on a 24-hour cycle, so 9 = 9am and 21 = 9pm.)
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