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Climate Change classes 1
Preface and Structure
1 Energy from the Sun
Background solar radiation
Experiment solar radiation
Links Sun and Earth
2 The Oceans
3 Albedo
UQ 3 May 07 Cars and ozone
UQ 2 Mar 07 Urban air
Climate change 2007 IPCC special
UQ 1 Nov Dec 06 Particles in air
Special: Oct. 2006 Communication
Nr 10 Sept. 2006 Africa's emissions
Nr 9 July 06 Air traffic
Special: June 06 Climate summit
Nr 8 April 2006 Ozone & N2 cycle
Nr 7 March 2006 Climate modeling
Nr 6 Feb. 2006 acid rain
Nr 5 Jan. 2006 oceanic sulfur
Special: Nov 05 Ozzy Ozone
Nr 4 Oct. 2005 light/satellites
Special: Sept 05 Cyclones
Nr 3 Sept. 2005 methane/energy
Special: July 05 Greenhouse Earth
Nr 2 June 2005 forest/aerosols
No 1 May 2005 vegetation/CO2
     

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Activities

Incoming solar radiation

We can demonstrate by means of a globe, a piece of black cardboard and a spotlight or lamp why solar radiation heats the spherical Earth differently.
  

Material

Required are:

1 globe
1 lamp / spotlight with directional radiation
1 piece of black cardboard, about. 20 x 20 cm
support material (stand)
scissors, spring bow compass
 

Material

Fotos auf dieser Seite: Elmar Uherek

Aufbau

Setup

A round hole is cut into the black cardboard by means of spring bow compass and scissors. The cardboard is fixed between lamp and globe with the help of a stand in a way that the light of the lamp forms a sharp circle or oval on the globe.
   

For the following procedure it is important to keep the distance between lamp, cardboard and globe constant. It has some advantages if the light from the lamp is directional but if the light source is not too much point-shaped. In contrast to a lamp or a spot light with a diverging light cone the sun rays are nearly parallel, since the Sun is far larger than the Earth.
 

Globus angestrahlt

Erddrehung im Sonnenlicht

Simulation of solar radiation in different latitudes

If we shift the lamp and the cardboard in height relative to the globe, the light beam strikes the globe in different areas. We can move it from the equator to the pole. Since the direction of the rays is still the same, their inclination on the globe changes. The closer we are to the pole, the larger the area which is illuminated by the same energy.
  

Animation Erdbeleuchtung

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last updated 19.05.2008 | © ACCENT - Atmospheric Composition Change 2013