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  • Irish Chronicles Document Links Between Volcanoes and Weather
    A study of over 40,000 written entries in Irish Annals and ice core measurements shows a strong corr...Read more

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    Irish Chronicles Document Links Between Volcanoes and Weather

    A study of over 40,000 written entries in Irish Annals and ice core measurements shows a strong correlation between the occurrence of volcanic eruptions and extreme cold weather in Ireland over a 1200 year period. Data analyzed in this study cover the period from 431 to 1649, during which time up to 48 volcanic eruptions are identified in Greenland ice core records through deposition of volcanic sulfate in annual layers of ice. You can find the study (open access), published on 6 June 2013 in IOP Publishing's journal Environmental Research Letters, at http://iopscience.iop.org/1748-9326/8/2/024035/article. Find out more about how volcanoes can influence climate.
  • EF-5 Tornado in El Reno, Oklahoma Widest Ever Recorded in US
    The EF-5 tornado that hit El Reno, Oklahoma on May 31st was the widest ever recorded in the US, acco...Read more

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    EF-5 Tornado in El Reno, Oklahoma Widest Ever Recorded in US

    The EF-5 tornado that hit El Reno, Oklahoma on May 31st was the widest ever recorded in the US, according to the National Weather Service in Norman Oklahoma. The tornado, which remained on the ground for 40 minutes and reached 2.6 miles across (4.2 km), took the lives of 18 people including storm chasers Tim Samaras, Paul Samaras and Carl Young. For more information on the tornado, visit http://ow.ly/i/2hfDG.
  • Atmospheric CO2 Level Tops 400 ppm
    During the week of May 13th, the CO2 level at the Mauna Loa Observatory in Hawaii topped 400 ppm rep...Read more

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    Atmospheric CO2 Level Tops 400 ppm

    During the week of May 13th, the CO2 level at the Mauna Loa Observatory in Hawaii topped 400 ppm repeatedly. Daily levels of CO2 can vary due to weather, and there are seasonal trends as well. The level of atmospheric greenhouse gases continues to increase, now over 120 ppm since the Industrial Revolution began. For more on the Keeling Curve, see http://keelingcurve.ucsd.edu/. Find out more about greenhouse gases and warming.
Streamers in the Sun's corona during a solar eclipse. In the top image, taken in 1994 near solar min, the streamers are mostly absent from the Sun's poles. In the bottom image, taken near solar max in 1980, streamers sprout from all solar latitudes.
Click on image for full size
Images courtesy of UCAR's High Altitude Observatory and Rhodes College.

The Solar Polar Atmosphere

At certain times in the sunspot cycle, the Sun's atmosphere and the solar wind behave very differently near the Sun's poles as compared to equatorial regions on the Sun.

Scientists call the relatively "quiet" phase of each sunspot cycle "solar min". Around solar min, images of the Sun's upper atmosphere (the corona) show striking differences between the polar corona and the equatorial corona. Images taken during a solar eclipse or by a special instrument called a coronagraph show dense structures called streamers extending outward through the corona at low latitudes. However, near the Sun's poles the streamers are less prominent or absent altogether.

The solar wind, the Sun's "extended atmosphere", also displays distinct polar and equatorial regimes around each solar min. The solar wind emanating from polar regions races away from the Sun at speeds of 700 km/sec (435 miles/second) or faster. The solar wind flowing outward from equatorial regions is much slower, moving about half as quickly as the fast polar wind. The fast solar wind escapes the Sun through coronal holes which form around open magnetic field lines near the poles.

During the active phase of the solar cycle, called "solar max", the number of sunspots increases and the Sun's magnetic field becomes complex and chaotic. Eclipse photos and coronagraphs show streamers bursting forth in a haphazard fashion from all latitudes on the Sun at solar max. Likewise, the Sun's scrambled magnetic field at solar max produces many more fluctuations in solar wind speed with latitude... unlike the clear equatorial vs. polar distinction found at solar min.

Much of our knowledge of the Sun's poles and the high-latitude solar wind was gathered by the Ulysses spacecraft. Ulysses is the only mission so far to "fly over" the poles of the Sun.

Last modified June 11, 2009 by Randy Russell.

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