MLS and CALIOP Cloud Ice Measurements in the Upper Troposphere: A Constraint from Microwave on Cloud Microphysics
Artikel i vetenskaplig tidskrift, 2014

This study examines the consistency and microphysics assumptions among satellite ice water content (IWC) retrievals in the upper troposphere with collocated A-Train radiances from Microwave Limb Sounder (MLS) and lidar backscatters from Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP). For the cases in which IWC values are small (<10 mg m(-3)), the cloud ice retrievals are constrained by both MLS 240- and 640-GHz radiances and CALIOP 532-nm backscatter (532). From the observed relationships between MLS cloud-induced radiance T-cir and the CALIOP backscatter integrated (532) along the MLS line of sight, an empirical linear relation between cloud ice and the lidar backscatter is found: IWC/(532) = 0.58 +/- 0.11. This lidar cloud ice relation is required to satisfy the cloud ice emission signals simultaneously observed at microwave frequencies, in which ice permittivity is relatively well known. This empirical relationship also produces IWC values that agree well with the CALIOP, version 3.0, retrieval at values <10 mg m(-3). Because the microphysics assumption is critical in satellite cloud ice retrievals, the agreement found in the IWC-(532) relationships increase fidelity of the assumptions used by the lidar and microwave techniques for upper-tropospheric clouds.

Clouds

MODEL

DISTRIBUTIONS

EXTINCTION

SATELLITE-OBSERVATIONS

WATER-CONTENT

ODIN-SMR

CALIPSO

A-TRAIN

RETRIEVAL

RADIATIVE-TRANSFER

Författare

D. L. Wu

NASA Goddard Space Flight Center

A. Lambert

Jet Propulsion Laboratory, California Institute of Technology

W.G. Read

Jet Propulsion Laboratory, California Institute of Technology

Patrick Eriksson

Chalmers, Rymd- och geovetenskap, Global miljömätteknik och modellering

J. Gong

Universities Space Research Association

Journal of Applied Meteorology and Climatology

1558-8424 (ISSN)

Vol. 53 1 157-165

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1175/jamc-d-13-041.1

Mer information

Skapat

2017-10-07