An important constraint on tropical cloud-climate feedback Dennis L. Hartmann and Kristin Larson Geophysical Res. Lett., 2002.

Slides:



Advertisements
Similar presentations
© Crown copyright 2006Page 1 CFMIP II sensitivity experiments Mark Webb (Met Office Hadley Centre) Johannes Quaas (MPI) Tomoo Ogura (NIES) With thanks.
Advertisements

Weather.
Water Vapor and Lapse Rate Feedbacks Neil Gordon ESP Seminar April 14, 2006.
Investigating the Temperature of Air
Atmospheric Stability
First Law of Thermodynamics The internal energy dU changes when: 1.heat dQ is exchanged between a parcel and its environment 2.work is done by a parcel.
Water Vapor and Cloud Feedbacks Dennis L. Hartmann in collaboration with Mark Zelinka Department of Atmospheric Sciences University of Washington PCC Summer.
Global Warming and Climate Sensitivity Professor Dennis L. Hartmann Department of Atmospheric Sciences University of Washington Seattle, Washington.
Aggregated Convection and the Regulation of Tropical Climate Kerry Emanuel Program in Atmospheres, Oceans, and Climate MIT.
Moist Processes ENVI1400: Lecture 7. ENVI 1400 : Meteorology and Forecasting2 Water in the Atmosphere Almost all the water in the atmosphere is contained.
Climate Sensitivity & Climate Feedback Instructor: Prof. Johnny Luo
Testing the Super-Greenhouse Thermostat with EOS observations Dan Feldman YLY Sunday meeting 10/30/05.
Tropical storms and the First Law of Thermodynamics ATMO 435.
Lesson 2 AOSC 621. Radiative equilibrium Where S is the solar constant. The earth reflects some of this radiation. Let the albedo be ρ, then the energy.
Clouds and climate change
Global Warming & Climate Sensitivity: Climate Feedbacks in the Tropics Professor Dennis L. Hartmann Department of Atmospheric Sciences University of Washington.
Earth-Atmosphere Energy Balance Earth's surface absorbs the 51 units of shortwave and 96 more of longwave energy units from atmospheric gases and clouds.
Lapse Rates and Stability of the Atmosphere
Chapter 6 – Cloud Development and Forms. Cloud Formation Condensation (i.e. clouds,fog) results from:
The Atmosphere. Did you know we are on our 3 atmosphere on Earth? Earth’s original atmosphere was probably just hydrogen and helium, because these were.
Vertical Structure of the Tropical Troposphere (including the TTL) Ian Folkins Department of Physics and Atmospheric Science Dalhousie University.
Climate change and stratosphere-troposphere coupling: Key questions Eugene Cordero, Nathan Gillett, Michael Sigmond, Shigeo Yoden.
Radiation Group 3: Manabe and Wetherald (1975) and Trenberth and Fasullo (2009) – What is the energy balance of the climate system? How is it altered by.
Convective Feedback: Its Role in Climate Formation and Climate Change Igor N. Esau.
2. Climate: “average” weather conditions, but the average doesn’t stay steady. I.e. Ice ages, El Niño, etc. 1. Weather: state of the atmosphere at a given.
ESS 111 – Climate & Global Change
Physics of the Atmosphere II
What Happens When Air Moves Over A Mountain? How do Mountain Ranges Influence Climate? Mr. Walter – Earth Science.
Properties of the Atmosphere
The Atmosphere and is its importance to the Earth.
11.1 Atmospheric Basics atmosphere.
The Atmosphere: Part 3: Unsaturated convection Composition / Structure Radiative transfer Vertical and latitudinal heat transport Atmospheric circulation.
Lab 6: Saturation & Atmospheric Stability
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
1 Clouds Katy Ginger Meteorologist, NCAR. 2 Relationship between changes in air pressure & temperature? As air pressure increases, temperature increases.
Class Outline What is Radiation and Radiative Forcing? –How does radiation differ from convection and conduction? How does radiation from the sun interact.
Humidity Under what conditions do you see the above?
Determination of Tropical Pacific Cloud Structures using AQUA MODIS Data Presented By: Terry Kubar Advisors: Dennis Hartmann and Rob Wood.
CLOUD FORMATION A STUDY IN METEOROLOGY Created by Joshua Toebbe NOHS 2015.
 Students will be able to identify three properties of the atmosphere and how they interact.  Students will be able to explain why atmospheric properties.
Atmosphere: Structure and Temperature Bell Ringers:  How does weather differ from climate?  Why do the seasons occur?  What would happen if carbon.
Cloud-Aerosol-climate feedback
Trends in Tropical Water Vapor ( ): Satellite and GCM Comparison Satellite Observed ---- Model Simulated __ Held and Soden 2006: Robust Responses.
17.1 Atmosphere Characteristics
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
AOS 100: Weather and Climate Instructor: Nick Bassill Class TA: Courtney Obergfell.
A Storm’s Story (So far…) The Sun warms the Earth through radiation. The Earth’s surface warms unevenly. Different types of air masses are created over.
Composition/Characterstics of the Atmosphere 80% Nitrogen, 20% Oxygen- treated as a perfect gas Lower atmosphere extends up to  50 km. Lower atmosphere.
Photo: Pamela R. Cox 2013 Elizabethtown, Kentucky.
The Atmosphere: Structure and Temperature
Climate and Global Change Notes 17-1 Earth’s Radiation & Energy Budget Resulting Seasonal and Daily Temperature Variations Vertical Temperature Variation.
ATMOSPHERE OBJECTIVE 1 1.What are the structural components of the
Composition of the Atmosphere 14 Atmosphere Characteristics  Weather is constantly changing, and it refers to the state of the atmosphere at any given.
Michelle Hughes, Madeleine Flores, Lindsey Morgan, and Joshua Baumbach UNIT 7.
17 Chapter 17 The Atmosphere: Structure and Temperature.
Full calculation of radiative equilibrium. Problems with radiative equilibrium solution Too hot at and near surface Too cold at and near tropopause Lapse.
WEATHER AND CLIMATE Chapter 2. WEATHER AND CLIMATE  Weather-State of constant change. Day to Day  Climate- Placed over a longer period of time.
Chapter 18 Moisture, Clouds, and Precipitation When it comes to understanding atmospheric processes, water vapor is the most important gas in the atmosphere!
18.2 Cloud Formation I. Air Compression and Expansion
What is air pressure and how does it affect us
Lab 2: Vertical Structure of the Atmosphere
Section 2: Properties of the Atmosphere
Seasons and Atmosphere
Dennis L. Hartmann and Kristin Larson
Atmosphere
Dennis L. Hartmann and Kristin Larson
Section 2: Properties of the Atmosphere
Atmospheric Moisture Atmospheric moisture is a very important topic under the theme of climatic system. In this presentation, you can make use of photos.
Global Warming & Climate Sensitivity: Climate Feedbacks in the Tropics
Seasons and Atmosphere
Presentation transcript:

An important constraint on tropical cloud-climate feedback Dennis L. Hartmann and Kristin Larson Geophysical Res. Lett., 2002

The emission temperature of tropical anvil clouds doesn’t depend on SST, thus it will remain constant during climate change. Positive feedback Main result: This is relevant for climate change, because LW radiative effects of tropical convection are dominated by convective anvil clouds.

In the tropics: the heat balance is between convective heating and radiative cooling The most active convection is constrained to the altitude where radiative cooling is efficient Observations show a peak of probability of optically thick cloud tops (i.e. anvils) at 200 hPa and that clear- sky cooling rate decreases rapidly above 200 hPa The radiative cooling is balanced by adiabatic heating (subsidence). The rapid decrease in clear-sky cooling is accompanied by a strong convergence of mass at 200 hPa, which is balanced by a strong divergence of mass from the convective regions

Hypothesis: Even if SST increases, the emission temperature of anvil clouds remains the same.

The temperature at which tropical convection detrains and convective anvil tops occur is constrained by the Clausius-Clapeyron relationship. This is because anvil tops occurs where cooling rate declines rapidly, and this happens when water vapor emission becomes inefficient. Low water vapor emissivity is due to low saturation vapor pressure, which is related principally to the air temperature through C-C, rather than to pressure. Physical explanation:

Test of hypothesis with model: 3D Radiative-Convective model in which they specify SST and solve for equilibrium climate of the troposphere as a function of SST Convective (non-convective) regions of the models are defined to be those with ice visible optical depths > (<)0.1

Results (I): Clear-sky cooling decreases rapidly with height way before tropopause. As T drops < 200 K, emission from water vapor becomes inefficient. As SST goes up, the pressure at which rapid cooling occurs goes down (height goes up). This is because the troposphere warms up more than surface, so that the pressure (height) where T drops < 200 K gets lower (higher).

cooling rate drops off const 200 hPa high clouds anvils max/min vertical vel.

Results (II): The T where cooling rate drops is about const. compared to the T at fixed p = 200 hPa.

Ideas for CRG -> Fall 2012: 1.ENSO (mechanisms, teleconnections, prediction, asymmetry, climate change…) 2.IPCC/Anthropogenic climate change 3.Aerosols radiative impacts on climate 4.TCs and climate variability 5.Models uncertainty 6.Decadal variability/predictability 7.Stochastic climate models/Noise 8.ITCZs, single or not 9.Teleconnections 10.Stratocumulus clouds 11.Subtropical highs (already done?) 12.Simple climate models