4.8 • 750 Ratings
🗓️ 30 March 2024
⏱️ 83 minutes
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0:00.0 | Oh, wow, oh, oh, wow, oh, wow, oh, wow. |
0:13.0 | Oh, wow. |
0:15.0 | Oh, James. Hello, you're listening to The Science of Everything podcast, episode 142, the greenhouse effect. |
0:40.8 | I'm your host, James Fodor. |
0:42.7 | So in this episode, we're going to talk about the greenhouse effect and how it acts to warm up the Earth's climate relative to what it otherwise would be. |
0:51.9 | So we'll start with talking about the Earth's energy budget and then introduce the idea of the greenhouse effect and the impact of greenhouse gases have on our atmosphere. |
1:00.0 | We'll talk about the different types of greenhouse gases and their roles in trapping different types of wavelengths of radiation that's submitted from the Earth's surface. |
1:09.0 | We'll talk about the idealized greenhouse |
1:11.5 | model, which is a simple mathematical approach to understand the dynamics a little bit better. |
1:16.1 | We'll then talk about some more of the advanced concepts like radiative transfer models |
1:20.0 | and the sensitivity of the Earth to changes in radiative forcing due to increases in greenhouse gases. |
1:27.0 | Recommended pre-listening is the previous episode. |
1:29.3 | 141 on natural climate change. |
1:32.3 | We're continuing on in that series, so recommend you listen to the previous two |
1:36.3 | in order to have the context for this one. |
1:39.3 | So without further ado, let's get started and introduce the idea of Earth's energy budget. |
1:45.7 | This refers to the different flows of energy to the Earth from the Sun and from the Earth out |
1:50.7 | to space again. |
1:52.2 | So Earth receives energy from the Sun, obviously. |
1:55.9 | The Sun emits radiation mostly in the visible spectrum. |
1:58.6 | It has a surface temperature of about 6,000 Kelvin, and by laws of |
2:03.6 | black body radiation, that means that a body at that temperature will emit mostly in the visible |
... |
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