Discussion Overview
The discussion revolves around the fraction of solar radiation that reaches the Earth, considering the sun as an absolute black body. Participants explore geometric calculations related to the Earth's cross-sectional area and the implications of the Earth's orientation towards the sun.
Discussion Character
- Exploratory
- Technical explanation
- Mathematical reasoning
Main Points Raised
- One participant asks about the portion of solar radiation that hits the Earth, seeking a true value rather than an approximation.
- Another participant suggests that the question can be approached geometrically by comparing the area of the Earth's disc to the surface area of a sphere with the radius of Earth's orbit.
- There is a discussion about whether to consider the full surface area of the Earth or just half, as only one side faces the sun at a time.
- A hypothetical scenario is presented where the Earth is turned to face the sun in different orientations, affecting the amount of energy intercepted.
- A participant expresses realization about the importance of using the area of a flat disc rather than a hemisphere in calculations.
- Another participant provides the currently accepted value for the Solar Constant and discusses its variability based on solar emissivity and the Earth's position in its orbit.
- Climatologists use a value of 342 watts per square meter for studies related to the Earth's heat budget, which is derived from the Earth's surface area compared to its cross-section.
Areas of Agreement / Disagreement
Participants generally agree on the geometric approach to calculating the fraction of solar radiation that reaches the Earth, but there are differing views on whether to consider the full surface area or just the cross-section. The discussion remains unresolved regarding the exact portion of radiation that can be considered as reaching the Earth.
Contextual Notes
The discussion includes assumptions about the sun's black body characteristics and the variability of solar radiation based on the Earth's elliptical orbit. There is also mention of the Solar Constant and its dependence on various factors, which may not be fully resolved in the discussion.