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The Scientific Basis for a Satellite Mission to Retrieve Ccn Concentrations and Their Impacts on Convective Clouds : Volume 5, Issue 1 (10/02/2012)

By Rosenfeld, D.

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Book Id: WPLBN0003975023
Format Type: PDF Article :
File Size: Pages 38
Reproduction Date: 2015

Title: The Scientific Basis for a Satellite Mission to Retrieve Ccn Concentrations and Their Impacts on Convective Clouds : Volume 5, Issue 1 (10/02/2012)  
Author: Rosenfeld, D.
Volume: Vol. 5, Issue 1
Language: English
Subject: Science, Atmospheric, Measurement
Collections: Periodicals: Journal and Magazine Collection (Contemporary), Copernicus GmbH
Publication Date:
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications


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Rennó, N. O., Freud, E., Andreae, M. O., Williams, E., Rosenfeld, D., & Pöschl, U. (2012). The Scientific Basis for a Satellite Mission to Retrieve Ccn Concentrations and Their Impacts on Convective Clouds : Volume 5, Issue 1 (10/02/2012). Retrieved from

Description: Institute of Earth Sciences, The Hebrew University of Jerusalem, Jerusalem 91904, Israel. The cloud -mediated radiative forcing is widely recognized as the main source of uncertainty in our knowledge of the anthropogenic climate forcing and in our understanding of climate sensitivity. Current outstanding challenges are (1) global measurements of cloud condensation nuclei (CCN) in the cloudy boundary layer from space, and, (2) disentangling the effects of aerosols from the thermodynamic and meteorological effects on the clouds. Here we present a new concept for a way to overcome these two challenges, using relatively simple passive satellite measurements in the visible and IR. The idea is to use the clouds themselves as natural CCN chambers by retrieving simultaneously the number of activated aerosols at cloud base, Na, and the cloud base updraft speed. The Na is obtained by analyzing the distribution of cloud drop effective radius in convective elements as a function distance above cloud base. The cloud base updraft velocities are estimated by double stereoscopic viewing and tracking of the evolution of cloud surface features just above cloud base. In order to resolve the vertical dimension of the clouds, the field of view will be 100 m for the microphysical retrievals, and 50 m for the stereoscopic measurements. The viewing geometry will be 30 degrees off nadir eastward, with the Sun in the back at 30 degrees off zenith westward, which requires a Sun synchronous orbit at 14:00 LST. Having measured simultaneously the thermodynamic environment, the vertical motions of the clouds, their microstructure and the CCN concentration will allow separating the dynamic from the CCN effects. This concept is being applied in the proposed satellite mission named Clouds, Hazards and Aerosols Survey for Earth Researchers (CHASER).

The scientific basis for a satellite mission to retrieve CCN concentrations and their impacts on convective clouds

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