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Exploring Climate Change and Energy Dynamics
Oct 19, 2024
Climate Change and Energy Transfer
Introduction
Presented by Rosh
Focus on three main processes governing global climate
Climate has historically been unstable, with dramatic changes
Understanding Climate vs. Weather
Climate
: Long-term average of weather
Weather
: Results from energy transfer within the atmosphere
Rain: Water vapor cools, condenses, releases energy
Wind: Hot air rises, cooler air fills in
Global climate change is a shift in total energy in the system
Source of Energy
Sun
: Main source of energy, fusing 600 million tonnes of hydrogen per second
Surface temperature: 5800 Kelvin
Energy primarily emitted as visible light and ultraviolet radiation
Earth emits mostly infrared radiation (heat)
Dynamic Equilibrium
Climate moves towards stable state when energy leaving equals energy coming in
Energy Leaves Earth
:
Reflection (high albedo surfaces like ice, clouds)
Absorption and re-emission as heat (low albedo surfaces like oceans, forests)
Greenhouse Effect
Greenhouse gases absorb and re-emit heat
Reduces energy escaping to space
Atmosphere warms up until it radiates enough heat to maintain equilibrium
Radiative Forcing and Feedbacks
Radiative Forcing
: Any change in energy balance
Can trigger feedbacks that alter energy balance
Types of Forcings:
Solar
: Solar cycles
Albedo
: Volcanic dust, asteroid impacts, tectonic movements
Greenhouse Gases
: Volcanic activity, weathering, combustion
Conclusion
Climate change results from changes in:
Energy from the sun
Albedo
Greenhouse effect
Upcoming content will cover current forcings affecting modern climate
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