Deze website in het Nederlands bekijkenSite en français Zoeken
ContactgegevensTopicsProjecten aan het Belgisch Instituut voor Ruimte-AëronomiePublications

System Earth >> Aerosols

Introduction

In addition to the simple components (e.g. molecular oxygen, ozone, nitrogen) that constitute the Earth’s atmosphere, the atmosphere also contains microscopic particles, of which the composition, form and size are far less known. These small droplets play an important role in the physicochemistry of the stratosphere:

• they change its optical characteristics (absorption and diffusion of light)
• at their surface they can trigger important chemical reactions, in particular the destruction of ozone.

Stratospheric Aerosols and Polar Stratospheric Clouds

The structure of aerosols and their impact on the stratosphere depend on several parameters, including the local temperature. When temperatures are not too low (the threshold temperature depends on the types of particles considered, but is situated around -70° Celsius), these particles appear as fine droplets that are known as stratospheric aerosols.

On the other hand, when temperatures fall below -80° C, as is the case in winter above the poles, these stratospheric particles turn into microscopic ice crystals better known as polar stratospheric clouds. It is the chemical reactions that occur on these clouds that result in the large decrease in ozone during each austral spring over Antarctica (Antarctic ozone hole).

Because of their different physical properties (liquid in one case, solid in the other), aerosols and polar stratospheric clouds have very different physicochemical properties..

Stratospheric aerosols consist of fine particles in gaseous suspension that are mainly terrestrial (volcanic eruptions) of origin, but also anthropogenic (supersonic airplanes), or cosmic (meteorites) of origin.

During a volcanic eruption sulfuric gasses are injected into the stratosphere, where they convert to sulfate aerosols (sub-micron droplets containing about 75 percent sulfuric acid).

Following an eruption a large amount of these particles are formed and a large amount of aerosols fall back to the lower layers of the atmosphere. This explains why the impact of aerosols on incoming solar radiation varies significantly depending on if one is in a period of low or high level volcanic activity.

For example, when the Pinatubo volcano erupted in June 1991, scientists estimated that about 10% of the solar radiation was lost at the Earth’s surface, in comparison to about 0.1% the month before.

Mount St. Helens erupts

  18 May 1980 Mount St Helens erupts (Oregon, USA).

More info :

Stratospheric aerosols (.pdf, 608 KB)
>> Clouds and particles (ESPERE Internet encyclopedia)

 

Link naar de website van het Federaal Wetenschapsbeleid
Link naar de Federale Portaalsite
 
Ecological awareness