Alaska Science
      Quiet time on the sun stalls
      aurora viewing 
      By NED ROZELL
       
      November 30, 2009 
      Monday PM 
       
      It's a slow season for aurora watchers, due to an extra-long
      quiet period on the great aurora generator-and all-around giver
      of life-the sun. 
        
      "For two years we've been in an unusual, very low, extended
      solar minimum," said Dirk Lummerzheim, an aurora forecaster
      at the Geophysical Institute at the University of Alaska Fairbanks.
      "That has an effect on aurora because aurora activity follows
      solar activity. The aurora hasn't been too exciting lately." 
       
       
      Poul Jensen of Fairbanks
      took this photo near Old Murphy Dome Road on an exceptional aurora
      night from Oct. 29-30, 2009. 
      Photograph by Poul Jensen
       
      Like the booms and busts of snowshoe hares, the numbers of both
      solar flares and sunspots (dark splotches on the sun) peak about
      every 11 years. On the other side of that peak is a crash, and
      the sun has bottomed out in sporadic activity since early 2008.
      The sun has gone more than two years without spewing a significant
      solar flare, and sunspot counts have also been very low. And
      sunspots are not great aurora indicators anyway. 
        
      "There's a statistical connection, but the appearance of
      a sunspot doesn't guarantee aurora," said Roger Smith, a
      space physicist and director of the Geophysical Institute. "It
      isn't the sunspots that cause aurora; it's irregularities in
      the solar wind that liberate energy for these beautiful optical
      displays." 
        
      Syun-Ichi Akasofu, an expert on the aurora and former director
      of both the Geophysical Institute and the International Arctic
      Research Center, agrees that people place too much emphasis on
      the connection between sunspots and aurora activity. He says
      the presence of another irregularity on the surface of the sun-a
      large, cool area called a coronal hole-often generates nice aurora
      for those in the north as emissions from the hole rotate toward
      Earth every 27 days or so. 
        
      According to Akasofu, we see more of the coronal hole type of
      aurora than people in the Lower 48. He says: "The stream
      from a coronal hole is weaker than a blast wave (caused by a
      solar flare.) Sightings of this type of aurora are confined to
      high latitudes, like Alaska. In Iowa, you won't see them." 
        
      Aurora sightings have been scarce in southern Alaska this year,
      and forecasts have been tepid at http://www.gedds.alaska.edu/AuroraForecast/. 
        
      "In Anchorage, it's very difficult to see aurora,"
      Lummerzheim says. "In Fairbanks, it's not too bad. If you
      go to the Brooks Range, you get regular aurora, but we don't
      have that big (solar) storm that pushes the aurora 
      south." 
        
      If you want to see aurora right now, at any cost, catch a flight
      to Barrow or Kaktovik, Lummerzheim says. 
        
      "On the northern coast of Alaska, we have aurora every day,"
      he says. "It may be boring aurora, a weak green glow just
      over the horizon, but it's there."  
        
      But what goes down must go up, right? In the case of that awesome
      nuclear reactor in the sky, scientists look to the past activity
      as a possible predictor of what is to come. Except for a mysterious
      70-year period without sunspots in the 17th century, solar cycles
      have lasted from about nine to 14 years from trough to trough,
      and the last bottoming out of solar activity was 13 years ago,
      in 1996. 
        
      "We don't understand the physics of the sun enough to make
      confident predictions," Lummerzheim says. "But the
      general consensus is that we're getting into the end of the minimum,
      and we expect (solar activity, and, perhaps, aurora sightings)
      to go up as winter progresses." 
        
       
        
      This column is provided
      as a public service by the Geophysical Institute, 
      University of Alaska Fairbanks, in cooperation with the UAF research
      community.  
      Ned Rozell is a science writer at the institute. 
 
      
        
      
          
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