Sub-Project 1: Comparison of clouds from the ISCCP simulator with July climatology.
Objectives
This project will require participating models to use the “ISCCP simulator” to produce the “ISCCP clouds”
corresponding to a fixed season. The general climatology of the simulated cloud distribution is to be compared with
the ISCCP climatology. Also some exploration of the simulated cloud regimes in the fixed season case as compared to
the full AMIP2 case would be of interest.
The project will augment the basic analysis of cloud sensitivities with an examination of changes to the ISCCP
cloud types, including analysis in terms of dynamical regimes. In particular the project will perform a detailed
evaluation of the model's simulation of clouds and their representation in different dynamical regimes
for July (the '0K' control experiment) using ISCCP data and reanalyses.
The basic methodology for analysing the ±2K perturbation experiments in terms of climate sensitivity parameters
is described in Cess et al (1990). This will require diagnostic package A. The analysis will be extended to consider cloud amounts in the categories
defined by ISCCP according to cloud top pressure (CTP) and visible optical
depth (tau). CTP-tau histograms of cloud
amounts will be examined in different dynamical regimes, defined primarily in terms of mid-tropospheric vertical
motion using pressure vertical velocity at 500 hPa (diagnostic package B/C).
Sub-Project Leader:
Mark Ringer (Hadley Centre)
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Sub-Project 2: Changes in clear sky radiation.
Objectives
This project should explore the changes in clear sky radiation and its relation with the simulated changes in the
temperature and water vapour profiles (diagnostic package D). Of particular interest may be an exploration of the possible different
behaviour of the models in very dry and very moist areas.
Additional Data Requirements
Time averaged vertical profiles of air temperature, relative humidity and specific humidity.
Sub-Project Leader
Brian Soden (GFDL) and Laura Fowler (CSU)
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Sub-Project 3: Changes in "ISCCP clouds"
Objectives
If different dynamical regimes in the current climate are be taken for proxies for future climate then it is important to
relate the cloud changes seen in a climate change experiment to the shifted dynamical regimes. Thus a careful
investigation of the changes in “ISCCP clouds” is needed. The changes in “ISCCP clouds” will need to be related to
the changes in the cloud radiative forcing in order to explore more fully which aspects of the cloud distribution
contribute most to the cloud feedback. Any consistency found between models would provide valuable information to
assist in model evaluation studies in simulations of the current climate
(diagnostic package E).
Compositing methods will be used to explore the cloud response to a doubling of CO2 in the slab
model experiments as diagnosed from the ISCCP simulator. Methods similar to
Williams et al (2003) (diagnostic package E) and other compositing studies
(e.g. Norris and Weaver, 2001; Bony et al, 1997; Tselioudis et al., 2000;
Jakob and Tselioudis, 2003) (diagnostic package F/G) will be used
to investigate whether any primary relationships associated with the cloud response
can be consistently identified in several models. If any consistency is found,
comparison with composited observations would provide valuable information to assist
in model evaluation. The changes in "ISCCP clouds" will need to be related to changes
in the cloud radiative response in order to explore more fully which aspects of
the cloud distribution contribute most to the cloud feedback.
Sub-Project Leader:
Keith Williams (Hadley Centre)
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Sub-Project 4a: Separation of feedbacks
Objectives
It is understood that there are limitations in using changes in cloud
radiative forcing to estimate cloud feedback (e.g. Zhang et al, 1994; Soden et
al, 2004). This subproject uses the partial radiative perturbation (PRP)
technique of Manabe and Wetherald (1988)
and extended by Colman et al (1997) to calculate the feedback components. This analysis technique can separate out water vapour, lapse rate
and albedo feedbacks from cloud feedbacks and allows a more consistent
intercomparison of models in a spatial context. It is impractical for the
partial derivatives to be calculated centrally, hence participants are
encouraged to save the diagnostics listed in diagnostic
package I and calculate the partial derivatives 'in house'. A draft
document detailing the methodology to do this is available here (Word document).
Sub-Project Leader:
Robert Colman (BMRC)
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Sub-Project 4b: Analysis of large sclae feedback mechanisms
Objectives
The aim of this sub-project is to use the standard diagnostics from
diagnostic package H to decompose the global mean cloud
radiative response into contributions from familiar (or unfamiliar mechanisms)
e.g. mid-latitude phase change, decrease in tropical cloud amount, deepening
of tropical troposphere, changes in subtropical cloud water content, etc.
This is to be achieved by extending the regional Boer & Yu (2003) analysis to
include use of the ISCCP simulator diagnostics.
A secondary aim of the sub-project is to assess various simple models which
can be used to interpret changes in cloud radiative forcing in terms of the
radiative perturbation diagnostics applied in Project4a.
The applicability of another (simpler) method following Gregory et al (2003)
will also be tested across the range
of models with data obtained from the models during their approach to
equilibrium (diagnostic package J).
Sub-Project Leader:
Mark Webb (Hadley Centre)
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Sub-Project 5: Instantaneous CO2 radiative Forcing.
Objectives
This sub-project requests modelling groups to diagnose radiative forcing,
using the instantaneous change double radiation call approach in the 2xCO2
slab experiment. The forcing should be diagnosed at TOA, surface and 200mb,
and split into SW and LW, up and down, clear-sky and all sky net fluxes (diagnostic package K). At
a bare minimum at-least-5-year means of the geographical distribution should
be provided. This should be linked to the WCRP (GEWEX Radiation Panel)
Intercomparison of Radiation codes in Climate Models (ICRCCM).
Participants are also encouraged also to calculate the surface, TOA and
200mb "Hansen"/"relaxed" forcing (double CO2 but
keep SST constant; Hansen et al, 1997).
Sub-Project Leader:
Bill Collins (NCAR)
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Sub-Project 6: Changes in Surface Energy Balance.
Objectives
The intercomparison paper of Randall et al., 1992 (using additional model output from the Cess et al 1990
experiments) concluded that the major differences in the responses of models in the component of the surface energy
budget to a 4K warming were due to:
Differences in the simulated hydrologic cycles
Parametrisation of long wave radiation (especially the water vapour continuum)
Cumulus convection.
In contrast cloud-radiation effects were found to have only a secondary importance.
In both Cess et al 1990 and Randall et al 1992 the conclusions reached are consistent with
problems and uncertainties with moist processes.
It was further argued that the wide range of model sensitivities that were found would not be narrowed through simply
increasing model resolution but that improvements in the model physics would be needed.
While there have been many improvements to models since 1992, it is not self-evident that the differences in model
response at the surface to a 4K SST perturbation have reduced especially since there remain many deficiencies in the
representation of the hydrologic cycle in climate models.
Additional Data Required
To be agreed by participants but no doubt water vapour and temperature profiles will be required. Daily data may also
be required in order (possibly) to determine the main sources of model
differences (diagnostic package L).
Sub-Project Leader:
Volunteer Needed
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Sub-Project 7: Relating model metrics to climate
sensitivity
Objectives
One of the major shortcomings of all climate prediction assessments has
been the inability to objectively and unambiguously relate the errors in
model simulations (as judged by comparisons to observations) to uncertainty
in climate sensitivity. One of the problems immediately obvious (and why this
has not been accomplished to date) is that climate model error metrics vary
with a) model variable b) spatial scale c) time scale d) single variable
errors versus multiple correlated variable errors. The fundamental nonlinear
nature of the climate system guarantees that this function is unlikely to be
simple. To date attempts have been ad-hoc and have varied widely depending
on physical feedback mechanism, variable, time and space scale.
This sub-project forms part of a more general approach to relate model metrics
to climate sensitivity. Initially, the approach will
utilise a parameter perturbation ensemble based on one GCM, however a critical
extension will be to use the multi-model ensemble of CFMIP. Required
diagnostics will be identified as the approach develops, however diagnostic packages E, F and Z are likely to be required.
Sub-Project Leaders:
David Sexton (Hadley Centre)
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