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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Variation of the Mesospheric Ozone above the Arctic caused by solar influence observed<br />

by ground-based millimeterwave radiometry<br />

Palm Mathias, Wieters Nadine, Hoffm<strong>an</strong>n Christoph, Sinnhuber Miriam, Golchert Sven, Notholt<br />

Justus<br />

We present measurements of strato- <strong>an</strong>d mesospheric O3 with a time resolution of 1 hour <strong>an</strong>d<br />

<strong>an</strong> altitude r<strong>an</strong>ge from 25 to 90 km. The instrument is located in the high Arctic at 79N.<br />

Ground based millimeterwave radiometry offers the opportunity to measure O3 at a narrow<br />

<strong>an</strong>d well defined spot in the mesosphere. Because of the slowly moving sun in the high<br />

Arctic, the state of the mesosphere regarding to solar illumination c<strong>an</strong> be assumed to be<br />

const<strong>an</strong>t throughout the measuring time of about 1 hour.<br />

The measurements are compared to the model output of a 3D chemical-tr<strong>an</strong>sport model which<br />

is developed at the IUP. The model is appended using mesospheric chemistry <strong>an</strong>d includes<br />

solar forcing of the atmosphere.<br />

The VMR of O3 strongly depends on the solar illumination. The strongest variation is due to<br />

the equilibrium reaction O3 + nu O + O2, which creates the diurnal variation. There are,<br />

however, other variations which do not follow this scheme <strong>an</strong>d are less well un<strong>der</strong>stood.<br />

The qualitative agreement of the model <strong>an</strong>d the measurement is good, the qu<strong>an</strong>titative<br />

agreement r<strong>an</strong>ges from excellent to rather poor. It is assumed that variation of the O3 content<br />

in the mesosphere due to solar illumination strength is not well represented. Possible sources<br />

for the observed variation <strong>an</strong>d the un<strong>der</strong>lying mech<strong>an</strong>isms are discussed <strong>an</strong>d qu<strong>an</strong>titavely<br />

studied.

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