Global Climate: 2.1 Causes of Climate Change Flashcards
Explain the greenhouse effect
- Short-wave radiation from the sun filters through the atmosphere, allowing visible light through.
- This is absorbed by the earth’s surface.
- Long-wave radiation is emitted back towards the atmosphere.
- This is absorbed by greenhouse gases.
- Long-wave radiation is re-emitted back to earth as heat, warming the earth.
Define the word System
A system is a set of interrelated parts and the connections between them. These parts unite to form a complex whole and produce emergent properties.
Define the 3 parts of a system with examples.
Inputs: the elements that go into a system in order for there to be processes, outputs and feedback. E.G. material; water entering the atmosphere or energy; solar radiation.
Processes: act on the inputs and transform them into outputs (e.g. water in the atmosphere becomes rain and returns to the Earth’s surface).
Outputs/feedback: the flows of matter and/or energy that leave a system (e.g. the atmosphere radiates heat into space).
Define open and closed systems.
An open system exchanges matter and energy with its surroundings.
A closed system exchanges energy but not matter with its surroundings.
Define positive and negative feedback loops.
A system output re-enters the system as feedback and becomes a new input.
Response to change = the feedback moves the system in the same direction (positive feedback) or the opposite direction (negative feedback).
Describe this negative feedback loop: clouds
- Global temp. rises.
- More evaporation of water.
- Water vapour forms clouds in atmosphere.
- Albedo increases, reflects more incoming short-wave radiation.
- Global temp. falls. Less evaporation. Less clouds. More incoming radiation.
- Global temp. rises again.
Describe this positive feedback loop: ice caps melting
- Global temp. rises.
- Ice caps melt.
- Soil is exposed, lower albedo, more absorption of heat.
- Global temp. rises more.
4 Benefits of the atmosphere.
- A shield from meteorites
- Protects us from sun’s harmful radiation
- Moderates and stabilises our climate, including temperature
- Supplies O2 and CO2 for producers and consumers.
Structure of the atmosphere + Pressure and Temperature through the atmosphere.
VERTICALLY LAYERED STRUCTURE:
Pressure decreases steadily with height.
Temperature does not change uniformly with altitude.
4 layers of the atmosphere (closest to farthest)
Troposphere - below 10km (0-10km)
Stratosphere - below 50km (10-50km)
Mesosphere - below 80km (50-80km)
Thermosphere - above 80km (80km-1000km)
What happens in the troposphere. (5)
- The Earth’s surface absorbs heat from the sun then heats atmosphere through conduction.
- Winds increase with height.
- Most of the atmospheric mass is found in this layer. (Water vapour, clouds, pollutants).
- Most of our weather occurs here.
- Most organism interaction through the exchange of gases or through the introduction of pollutants.
- The greenhouse effect occurs here.
What happens in the stratosphere. (5)
- Absorbs UV radiation from the sun.
- Winds increase with height.
- Temperature is about –60°C in the lower part of the stratosphere, shielded by the ozone layer.
- Temp. increases with height.
- The air is dry.
What happens in the mesosphere. (2)
- No ozone or other particulates to absorb UV heat, so temp. declines with height (reaching as low as –90°C).
- Strong winds up to around 3000 km/h.
What happens in the thermosphere (2) and inosphere (3).
- Absorbs UV + X-radiation from sun, breaking molecules into atoms (mainly oxygen, nitrogen and helium in the upper thermosphere).
- Temp. increases with height (can reach beyond 2000°C). Heat can cause thermosphere to expand, causing a variation in depth over time (500 to 1000 km).
- Ionosphere is located within the thermosphere + is an area with electrically charged particles.
- Short-wave radiowaves bounce off these ions back to Earth = allows communication over large distances.
- Northern/southern lights occur as electrically charged particles from the sun collide with ions in the ionosphere.
How incoming solar radiation is lost. (with rough figures)
100 units of incoming solar radiation:
- 19 absorbed by atmosphere and clouds
- 51 absorbed by earth’s surface
- 30 reflected and scattered by albedo (surface, clouds)