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X-WR-CALNAME;VALUE=TEXT:Harvard Climate Seminar
PRODID:-//Harvard events data//EN
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UID:event_533756_0
SUMMARY:Harvard Climate Seminar
DESCRIPTION:<div><em><strong>"From the Troposphere to the Stratosphere:  Physical and Chemical Details Linking Chemistry and Radiative Forcing"</strong></em></div><p><strong></strong>by <a href="http://www.seas.harvard.edu/directory/keutsch" data-url="http://www.seas.harvard.edu/directory/keutsch">Frank Keutsch (Harvard/SEAS)</a></p><p><drupal-media data-entity-type="media" data-entity-uuid="a8b20a4c-6b11-4bd8-89a8-8067d8a34af9" data-view-mode="hwp_large"></drupal-media></p><p><strong>Abstract:</strong></p><p>Tropospheric ozone and secondary aerosol affect climate and are known to harm human health and ecosystems. The processing rate of gas-phase reactive carbon compounds is directly coupled to formation of ozone and secondary organic aerosol in the troposphere. I will discuss how well novel bottom-up and top-down observations of the reactive carbon budget agree within the context of anthropogenic influence and the ability to predict amounts of ozone and aerosol.</p><p>Solar radiation management (SRM), a geoengineering approach to modify Earth’s climate on a global level, has been receiving growing attention. Although most work has focused on introduction of sulfate aerosol into the stratosphere to reduce solar radiation at the surface, a number of other materials have also been considered. To date, the detailed chemical and physical properties of these materials have mostly been treated in a simplified manner. As an example of the role physicochemical detail plays in understanding consequences of SRM, I will discuss the implications of a more detailed treatment of titania (TiO<sub>2</sub>), including the role of different titania polymorphs.</p>
LOCATION:Haller Hall (Geology Museum 102)
STATUS:CONFIRMED
DTSTART:20151118T210000Z
DTEND:20151118T220000Z
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