07.12.2012 Aufrufe

Erdfernerkundung - Numerische Physik: Modellierung

Erdfernerkundung - Numerische Physik: Modellierung

Erdfernerkundung - Numerische Physik: Modellierung

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5.5. CAWSES 273<br />

Abbildung 5.40: Ion–pair production due to energetic charged particles during the solar cycle<br />

time, NOx is depleted in the mesosphere by photochemical reactions – its life time in the<br />

stratosphere is much longer and with time it sinks slowly to lower altitudes with its maximum<br />

around the height of the ozone layer.<br />

§ 908 Ozone depletion (bottom panel in Fig. 5.39) is regulated by both species: initially in<br />

the event there is a strong depletion in the mesosphere above 60 km due to the combined<br />

effects of HOx and NOx. The pronounced depletion around 40 km, on the other hand, is<br />

due to NOx as can be inferred from the long time scales. Owing to different temperatures,<br />

the NOx-induced ozone depletion is larger in the stratosphere than in the mesosphere. The<br />

most remarkable effect, however, is the persistent ozone depletion by a few percent right in<br />

the middle of the ozone layer around 25 km lasting for more than a year. Such a persistent<br />

anomaly bears the seed for possible cumulative effects of solar energetic particle events – in<br />

particular during magnetic field reversals where the effects of individual events will be even<br />

larger than in the present day atmosphere.<br />

Ionization through the Solar Cycle<br />

§ 909 The first approach on long–term studies is a view on the solar cycle. Figure 5.40<br />

shows ion–pair production rates from 1988 to 2005, that is almost 2 solar cycles. Times<br />

of high solar activity are clearly visible as times with increased ion–pair production rates<br />

between 1989 and 1992 and again between 2000 and 2005. Solar minimum is around 1996.<br />

The sharp drop in ionization rate at 20 km is ‘instrumental’: the highest energies observed<br />

by the GOES particle detector are 800 MeV protons which stop at that height. At lower<br />

altitudes, ionization expected from higher energies is ignored in this figure – this does not<br />

pose a problem for modeling because the subsequent atmospheric chemistry model is limited<br />

to the stratosphere and mesosphere and thus is not influenced by neglect of tropospheric<br />

ionization. 14<br />

14 Such a limitation for a chemistry module is validated by the fact that the tropopause is a boundary<br />

which strongly inhibits transport of matter and thus almost completely decouples the troposphere from the<br />

atmosphere above.<br />

c○ M.-B. Kallenrode 2. Juli 2008

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