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X-WR-CALNAME;VALUE=TEXT:Special ClimaTea on Zoom
PRODID:-//Harvard events data//EN
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SUMMARY:Special ClimaTea on Zoom
DESCRIPTION:<div class="field field-name-body field-type-text-with-summary field-label-hidden view-mode-full">	<div class="field-items">		<div class="field-item even">			<div class="field field-name-body field-type-text-with-summary field-label-hidden view-mode-full">				<div class="field-items">					<div class="field-item even">						<div class="field field-name-body field-type-text-with-summary field-label-hidden view-mode-full">							<div class="field-items">								<div class="field-item even">									<p>										<strong>Speaker: </strong> <span>Dr. Adeyemi Adebiyi of UCLA</span>									</p>									<p>										<strong>Title: </strong> <em><span>"<strong>How much solar radiation does atmospheric mineral dust absorb?</strong>"</span></em>									</p>									<p>										<strong>Abstract: </strong>Mineral dust particles are critical to the Earth’s climate system because they account for<br>approximately ~25 % of the shortwave radiation scattered and absorbed by all aerosols in the<br>atmosphere. But despite the importance of these radiative effects, the amount of shortwave<br>radiation absorbed by atmospheric dust remains largely unclear. This is because knowledge of<br>dust absorption properties, characterized by the dust aerosol absorption optical depth, primarily<br>depends on the dust size distribution and the complex refractive index, which are difficult to<br>observe from remote-sensing platforms. As a result, climate model simulations and retrieval<br>algorithms rely on certain assumptions about dust properties that have led to significant<br>uncertainties in their estimation of the global dust absorption optical depth. In this talk, I will<br>describe a framework that leverages dozens of in-situ measurements of the dust size distribution<br>and single-scattering albedo to obtain a more accurate constraint on the global dust absorption<br>optical depth. I will show that atmospheric dust is much coarser with significant spatial<br>variability in the imaginary refractive index than represented in climate models. Consequently, I<br>will show that amount of solar radiation absorbs by dust differs substantially from what climate<br>models simulate, which has important implications for the Earth’s energy balance									</p>								</div>							</div>						</div>					</div>				</div>			</div>		</div>	</div></div>
LOCATION:Zoom
STATUS:CONFIRMED
DTSTART:20201117T200000Z
DTEND:20201117T200000Z
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