espere Environmental Science Published for Everyobody Round the Earth
Printer friendly version of this page
Home    Contact    Encyclopaedia    Mobility    International    PDF    magazine    - ? -   
Clouds and Particles
basics
more
1. What happens in clouds?
2. Particles
3. Clouds, particles and climate
- Particles and visibility
- Particles and climate
- Radiation budget
* Worksheet 1
* Worksheet 2
* Worksheet 3
Links
PDF
     
 
clouds and particles

Clouds & Particles

More

The radiation budget

The radiation budget is the balance between the incoming energy from the Sun and outgoing energy from the Earth's surface.   Energy from the Sun can either be directly reflected by the surface of the Earth back into space, reflected back into space by clouds or can be absorbed by the Earth and re-emitted as heat.

 

basicsmore
basicsmore
basicsmore
basicsmore
basicsmore
basicsmore
basicsmore
basicsmore
 

 

Here we look at the global radiation budget and how it affects the Earth's climate.  We focus on the impact of humans today and in the future.

Observations of radiation budget are made using satellites which measure the amount of radiation emited from the Sun and from the Earth.

measurement of radiation from the sun and the earth.

1. Meteor satellite. Source: http://smsc.cnes.fr/SCARAB/Fr/

Incident energy from the Sun

The planet's radiation budget must be in equilibrium so that the Earth doesn't become colder or warmer. Although the climate system is in balance, this balance is dynamic and ever-changing.   Satellites above our atmosphere, directed at the Sun, show that the mean global energy striking the Earth is 340 W m-2.

 

change of insolation - latitude and season

2. Seasons are the result of the revolution of the Earth around the Sun and the tilt of the Earth's axis. A:  21st of June: summer in the Northern Hemisphere and winter in the Southern Hemisphere (opposite to C). D: Spring in the North, autumn in the South (21st of March) (opposite to B). Solar insolation changes with latitude and season.

 

mean value of solar energy in January 2004

3. The monthly mean value of solar energy in January 2004. Data from the polar orbiter NOAA-17. Source: NOAA. Click to enlarge! (20 K).  What is the average value in Europe for January 2004?

Albedo: energy reflected by the Earth

Some of the solar radiation striking the Earth is reflected directly back into space. This fraction is called the albedo. Look at images 4a and 4b to see the average albedo of our planet in January and August. The global annual average albedo is approximately 0.3, so about 30% of the solar radiation entering our atmosphere is reflected back into space.  Polar regions have high albedos because the white ice is highly reflective.

 

planetary average albedo in January

4. a)  Planetary average albedo in January. Data from ERBE, NOAA.
Click to enlarge! (36 K).

planetary average albedo in August

4. b)  Planetary average albedo in August. Data from ERBE, NOAA.
Click to enlarge! (36 K).

The solar energy which is not directly reflected back into space (70%, around 240 W m-) is absorbed by atmosphere and by the Earth's surface.  This process leads to a heating of the surface and emission of infra-red (long wave) radiation.  A proportion of this infra-red radiation is trapped by greenhouse gases in the atmosphere and this natural warming process keeps the mean temperature of our planet at 15 oC.   Some areas of the world absorb more energy than they re-emit and should therefore be getting warmer and warmer.  In other areas the radiation balance is negative and these regions should be getting colder.  This doesn't happen because atmosphere and oceans continuously transport heat from equator to the poles to even up the temperature differences.


global annual mean radiative budget

 

 

5. Global annual mean radiative budget in W m-. Source: LMD/ Scarab. Click to enlarge (22 K)!

How can the radiation budget change?

The amount of energy coming from the Sun can vary.  For example, the tilt of axis about which the Earth rotates can vary.  Contrasts in the amount of solar energy received between latitudes and between seasons are larger when the tilt is larger. Climate changes due to astronomic variations are defined by Milankovitch theory.
The albedo (the amount of energy reflected) changes if there are changes in the amount of ice, water, forest and cloud cover over the Earth.  For example, a colder climate would lead to more polar ice and therefore an increase in mean global albedo.  This would further decrease the global temperature.  This is a positive feedback effect.
The amount of energy kept by the planet changes if the greenhouse effect is modified.

 

 

The radiative budget can change:
1. Naturally as a result of astronomical variations.
2. If the albedo of the Earth changes, either naturally (input of aerosols into the air following volcanic eruption) or because of human activity.   
3. If human activities modify greenhouse gas concentrations and cloud characteristics as this affects the way the planet losses and traps heat.

influences on radiative forcing

6. What affects the radiation balance?
Author: Justine Gourdeau.

 

Much of the research into our climate focuses on the radiation balance.  Understanding the complexity of the controls and feedbacks and how humans modify the fragile equilibrium is a key to predict, and hopefully prevent, future unwanted climate change.

 

About this page...
author: Justine Gourdeau - LaMP, Clermont-Ferrand, France
scientific reviewer: Dr. Maud Leriche and Dr. Frederic Szczap - LaMP, Clermont-Ferrand, France
last published: 2004-05-11

 top

ESPERE / ACCENT

last updated 21.02.2006 14:28:31 | © ESPERE-ENC 2003 - 2013