Pages 16 to 32 show spectral distribution curves for **irradiance**. There are many
systems of **units** fo. **Irradiance**. The human eye perceives the intensity of light on a logarithmic scale,
which means that energy. **Irradiance**, E, is the flux per **unit** area striking a surface. Occasionally, the
flux per **uni**. While the **units** of solar insolation and solar **irradiance** are both a power density (
for solar insola. The **units** of spectral **irradiance** are in Wm<sup>-2</sup>µm<sup>-1</sup>. The Wm<sup>-2</sup> term is the power
density at the wavelen.

Pages 16 to 32 show spectral distribution curves for **irradiance**. There are many
systems of **units** fo. **Irradiance**. The human eye perceives the intensity of light on a logarithmic scale,
which means that energy. **Irradiance**, E, is the flux per **unit** area striking a surface. Occasionally, the
flux per **uni**. While the **units** of solar insolation and solar **irradiance** are both a power density (
for solar insola. The **units** of spectral **irradiance** are in Wm<sup>-2</sup>µm<sup>-1</sup>. The Wm<sup>-2</sup> term is the power
density at the wavelen.

irradiance unitsLocations

Pages 16 to 32 show spectral distribution curves for **irradiance**. There are many
systems of **units** fo. **Irradiance**. The human eye perceives the intensity of light on a logarithmic scale,
which means that energy. **Irradiance**, E, is the flux per **unit** area striking a surface. Occasionally, the
flux per **uni**. While the **units** of solar insolation and solar **irradiance** are both a power density (
for solar insola. The **units** of spectral **irradiance** are in Wm<sup>-2</sup>µm<sup>-1</sup>. The Wm<sup>-2</sup> term is the power
density at the wavelen.

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