This story entered on 20th Sep, 2012 01:45:06 PM PST
At the bottom of the world, fifty people are looking forward to seeing the sun peek above the horizon
on or around September 22 – the first time they have seen the sun in six months. NOAA ESRL/
GMD personnel LTJG Heather Moe and Johan Booth spent the Antarctic winter working at NOAA’s
Atmospheric Research Observatory located at the geographic South Pole. The Amundsen-Scott South
Pole Station, one of three United States research stations in Antarctica, only experiences one sunrise
and sunset per year due to its location at 90˚S latitude. Although the sun officially sets on March
23 and rises on September 22, the actual sunrise and set times vary due to refraction of light on the
horizon from atmospheric conditions: the sun typically rises and dips below the horizon several times
before fully setting or rising. The station is completely isolated during the winter months because frigid
temperatures make it impossible for aircraft to land. This past winter South Pole was especially cold:
the crew experienced a low temperature of -105.5⁰ F (-76.2⁰ C) in July and spent several other days
below -100⁰ F. To view the South Pole sunrise, please go the live NOAA/ESRL web camera at:
http://www.esrl.noaa.gov/obop/spo/livecamera.html
Sunrise over the Antarctic continent also signifies the onset of the yearly ozone hole formation. NOAA
staff at the South Pole launches ozonesonde instruments on large balloons to ascertain the vertical
profile of ozone in the Antarctic stratosphere. As the balloon carrying the instrument ascends through
the atmosphere, the ozonesonde collects information about ozone and standard meteorological
quantities such as pressure, temperature and humidity. The balloon can typically ascend to altitudes
of about 115,000 feet (35 km) before it bursts. Polar ozonesonde profiles provide a detailed vertical
measurement of ozone that can be made during dark periods when satellite ozone observations are
limited due to the lack of sunlight over Antarctica during the austral winter. Antarctic ozone depletion
occurs primarily between the altitudes of 12 and 20 kilometers, a region where polar stratospheric
clouds, necessary for the chlorine-catalyzed chemical ozone destruction process, readily form. Progress
of the 2012 ozone hole can be followed at the website:
http://esrl.noaa.gov/gmd/dv/spo_oz/
Background: A wide range of baseline atmospheric measurements have been acquired at South Pole
by NOAA/ESRL and its predecessor organizations since the International Geophysical Year (IGY), 1957.
South Pole’s atmospheric carbon dioxide greenhouse gas record pre-dates the better-known Mauna
Loa carbon dioxide curve by one year, making it the longest carbon dioxide sampling record on earth. In
addition to monitoring greenhouse gases, the winter crew also measures atmospheric particulates, solar
radiation, and ozone-depleting gases. Each year NOAA releases over 40 ozonesondes on high-altitude
balloons to study the stratospheric ozone layer and to document the onset and severity of the annual
Antarctic “Ozone Hole”; the continuous NOAA ozonesonde record dates back to 1986.
Significance: Continuous long term records of atmospheric parameters measured at the South Pole,
where the mantra is “the cleanest air on earth”, have documented a wide range of changes in the
composition, chemistry, and radiative balance of the atmosphere over the Antarctic continent since the inception of the measurements in 1957. Many of these changes are related to mankind’s combustion of
fossil fuels and from the release of industrial and household chemicals into the atmosphere.
http://www.esrl.noaa.gov/dv/spo_oz/movies/index.html
Contact information
Name: Brian Vasel
Tel: (303) 497-6823
Brian.Vasel@noaa.gov