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The sun’s magnetic field, which spans the solar system, is just months away from flipping, observatory measurements show.<\/strong><\/p>\n “This change will have ripple effects throughout the solar system,” solar physicist Todd Hoeksema of Stanford University said\u00a0in a statement<\/a>.<\/p>\n Hoeksema is the director of Stanford’s\u00a0Wilcox Solar Observatory<\/a>, one of just a few observatories around the world that monitors the sun’s polar magnetic fields.<\/p>\n The sun’s magnetic field changes polarity approximately every 11 years during the peak of each solar cycle as the sun’s inner dynamo reorganizes itself.<\/p>\n This next reversal\u2014which will be only the fourth observed since tracking began in 1976\u2014will mark the midpoint of\u00a0Solar Cycle 24<\/a>.<\/p>\n During a magnetic field reversal, “the sun’s polar magnetic fields weaken, go to zero and then emerge again with the opposite polarity,” explained solar physicist Phil Scherrer, also at Stanford, in the statement.<\/p>\n Scientists are already seeing signs of the reversal happening, and this time there’s a twist: Data from Wilcox show that the sun’s two hemispheres are oddly out of sync, with the North Pole already beginning to change and the South Pole racing to catch up.\u00a0That means that for now, at least, the sun effectively has two South Poles.<\/p>\n Soon both poles should be completely reversed. “It looks like we’re no more than three to four months away from a complete field reversal,” Hoeksema said.<\/p>\n The Wilcox Solar Observatory has been observing the sun’s magnetic field since 1975, and its scientists have been converting those numerical measurements into a map that can now be\u00a0viewed online<\/a>.<\/p>\n “What we’re really happy about is we’ve never changed or upgraded [the observatory],” Scherrer said in an interview Wednesday. “It’s the only instrument in the world where you can look back over 40 years and know you’re measuring the same thing. That allows us to compare fields from one cycle to the next.”<\/p>\n What Does a Reversal Mean?<\/strong><\/p>\n A reversal of the sun’s magnetic field will have consequences throughout the solar system since the domain of the sun’s magnetic influence\u2014called the heliosphere\u2014extends far beyond Pluto. Changes to the field’s polarity ripple all the way out to the\u00a0Voyager probes<\/a>, which are racing toward interstellar space.<\/p>\n Playing a central role in solar field reversals is the “current sheet,” a sprawling surface that juts out of the sun’s equator where the sun’s slowly rotating magnetic field induces an electric current.<\/p>\n The current itself is small\u2014only one ten-billionth of an amp per square meter\u2014but there’s a lot of it, and the entire heliosphere is organized around it.<\/p>\n During field reversals, the current sheet becomes very wavy. Scherrer likens the undulations to the seams on a baseball.<\/p>\n As the Earth orbits the sun, our planet dips in and out of the wavy current sheet, and the transitions can stir up stormy\u00a0space weather<\/a>\u00a0around us.<\/p>\n The geometry of the current sheet can also affect Earth’s exposure to cosmic rays, which are high-energy particles accelerated to the speed of light by supernova explosions and other violent events in the galaxy.<\/p>\n Cosmic rays pose a threat to astronauts and space probes, and some researchers say they might also affect the cloudiness and climate of Earth.<\/p>\n The sun’s current sheet functions as a barrier to cosmic rays, preventing them from penetrating into the inner solar system. And a wavy, crinkly current sheet appears to create a better shield against these energetic particles.<\/p>\n Earth’s Flip-Flop Coming<\/strong><\/p>\n The sun isn’t the only body in the solar system with a magnetic field that reverses. Earth has a magnetic field as well, and it has flipped many times over the last billion years.<\/p>\n This isn’t surprising, Scherrer said, because the magnetic fields of both the sun and the Earth are thought to be generated by similar “dynamo” processes that involve rotating and convecting electrically conducting fluids\u2014molten iron in the case of the Earth and hot, ionized gases for the sun.<\/p>\n The difference, however, is that Earth’s magnetic field reversals happen much less frequently\u2014only once every 200,000 to 300,000 years on average, although the actual time can vary widely\u2014and over much longer timescales.<\/p>\n