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Add aod and clearsky_index to glossary, link terms in spectrum.rst
#2663
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@@ -19,7 +19,16 @@ There is a convention on consistent variable names throughout the library: | |||||||||||||||||||||
| albedo | ||||||||||||||||||||||
| Ratio of reflected solar irradiance to global horizontal irradiance | ||||||||||||||||||||||
| [unitless] | ||||||||||||||||||||||
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| aod | ||||||||||||||||||||||
| aod500 | ||||||||||||||||||||||
| aerosol optical depth. Measure of aerosols (e.g., smoke | ||||||||||||||||||||||
| particles, desert dust) distributed within a column of air from the | ||||||||||||||||||||||
| instrument (Earth's surface) to the top of the atmosphere. The AOD | ||||||||||||||||||||||
| value indicates the level of extinction of sunlight in this column, and | ||||||||||||||||||||||
| when followed by a number (e.g. AOD500), indicates the extinction at | ||||||||||||||||||||||
| this wavelength (500nm). [unitless] | ||||||||||||||||||||||
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| aoi | ||||||||||||||||||||||
| Angle of incidence. Angle between the surface normal vector and the | ||||||||||||||||||||||
| vector pointing towards the sun's center. [°] | ||||||||||||||||||||||
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@@ -33,17 +42,21 @@ There is a convention on consistent variable names throughout the library: | |||||||||||||||||||||
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| apparent_zenith | ||||||||||||||||||||||
| Refraction-corrected solar zenith angle. The solar | ||||||||||||||||||||||
| zenith angle describes the position of the sun relative to the vertical and is | ||||||||||||||||||||||
| defined as the angle between a vector pointed straight up and a vector pointed | ||||||||||||||||||||||
| at the sun, from the observer. [°] | ||||||||||||||||||||||
| zenith angle describes the position of the sun relative to the vertical | ||||||||||||||||||||||
| and is defined as the angle between a vector pointed straight up and a | ||||||||||||||||||||||
| vector pointed at the sun, from the observer. [°] | ||||||||||||||||||||||
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| apparent_elevation | ||||||||||||||||||||||
| Refraction-corrected solar elevation angle. This is the complement of | ||||||||||||||||||||||
| :term:`apparent_zenith` (90 - apparent_zenith). [°] | ||||||||||||||||||||||
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| bhi | ||||||||||||||||||||||
| Beam/direct horizontal irradiance | ||||||||||||||||||||||
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| clearsky_index | ||||||||||||||||||||||
| clearsky index. Ratio of actual global irradiance to modeled clearsky | ||||||||||||||||||||||
| global irradiance | ||||||||||||||||||||||
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There was a problem hiding this comment. Choose a reason for hiding this commentThe reason will be displayed to describe this comment to others. Learn more. +1 for "An admonition to distinguish it from clearness index" |
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| dhi | ||||||||||||||||||||||
| Diffuse horizontal irradiance | ||||||||||||||||||||||
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@@ -95,10 +108,12 @@ There is a convention on consistent variable names throughout the library: | |||||||||||||||||||||
| Sandia Array Performance Model IV curve parameters | ||||||||||||||||||||||
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| latitude | ||||||||||||||||||||||
| Latitude in decimal degrees. Positive north of equator, negative to south. | ||||||||||||||||||||||
| Latitude in decimal degrees. Positive north of equator, negative to | ||||||||||||||||||||||
| south. | ||||||||||||||||||||||
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| longitude | ||||||||||||||||||||||
| Longitude in decimal degrees. Positive east of prime meridian, negative to west. | ||||||||||||||||||||||
| Longitude in decimal degrees. Positive east of prime meridian, negative | ||||||||||||||||||||||
| to west. | ||||||||||||||||||||||
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| pac, ac | ||||||||||||||||||||||
| AC power | ||||||||||||||||||||||
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@@ -149,15 +164,16 @@ There is a convention on consistent variable names throughout the library: | |||||||||||||||||||||
| Diode saturation current | ||||||||||||||||||||||
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| solar_azimuth | ||||||||||||||||||||||
| Azimuth angle of the sun in degrees East of North. The solar azimuth angle | ||||||||||||||||||||||
| describes the sun’s position along the horizon relative to the observer. | ||||||||||||||||||||||
| The pvlib-python convention is defined as degrees East of North, so | ||||||||||||||||||||||
| North = 0°, East = 90°, South = 180°, West = 270°. | ||||||||||||||||||||||
| Azimuth angle of the sun in degrees East of North. The solar azimuth | ||||||||||||||||||||||
| angle describes the sun’s position along the horizon relative to the | ||||||||||||||||||||||
| observer. The pvlib-python convention is defined as degrees East of | ||||||||||||||||||||||
| North, so North = 0°, East = 90°, South = 180°, West = 270°. | ||||||||||||||||||||||
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Suggested change
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| solar_zenith | ||||||||||||||||||||||
| Zenith angle of the sun in degrees. This is the angle between is between a | ||||||||||||||||||||||
| vector pointed straight up and a vector pointed at the sun, from the observer. | ||||||||||||||||||||||
| This is the complement of solar elevation (90 - elevation). [°] | ||||||||||||||||||||||
| Zenith angle of the sun in degrees. This is the angle between is | ||||||||||||||||||||||
| between a vector pointed straight up and a vector pointed at the sun, | ||||||||||||||||||||||
| from the observer. This is the complement of solar elevation | ||||||||||||||||||||||
| 90 - elevation). [°] | ||||||||||||||||||||||
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Suggested change
Since we're editing this definition. |
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| spectra | ||||||||||||||||||||||
| spectra_components | ||||||||||||||||||||||
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@@ -167,16 +183,17 @@ There is a convention on consistent variable names throughout the library: | |||||||||||||||||||||
| is composed of direct and diffuse components. | ||||||||||||||||||||||
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| surface_azimuth | ||||||||||||||||||||||
| Azimuth angle of the surface in degrees East of North. This angle describes the | ||||||||||||||||||||||
| horizontal projection of the normal vector from the surface. The pvlib-python | ||||||||||||||||||||||
| convention is defined as degrees East (clockwise) of North, so North = 0°, | ||||||||||||||||||||||
| East = 90°, South = 180°, West = 270°. | ||||||||||||||||||||||
| Azimuth angle of the surface in degrees East of North. This angle | ||||||||||||||||||||||
| describes the horizontal projection of the normal vector from the | ||||||||||||||||||||||
| surface. The pvlib-python convention is defined as degrees East | ||||||||||||||||||||||
| (clockwise) of North, so North = 0°, East = 90°, South = 180°, | ||||||||||||||||||||||
| West = 270°. | ||||||||||||||||||||||
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| surface_tilt | ||||||||||||||||||||||
| Tilt from horizontal [°]. The surface tilt angle | ||||||||||||||||||||||
| is defined as degrees from the horizontal | ||||||||||||||||||||||
| such that a surface facing up would have a surface tilt of 0°, and one facing | ||||||||||||||||||||||
| the horizon would be 90°. [°] | ||||||||||||||||||||||
| such that a surface facing up would have a surface tilt of 0°, and one | ||||||||||||||||||||||
| facing the horizon would be 90°. [°] | ||||||||||||||||||||||
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| temp_air | ||||||||||||||||||||||
| Temperature of the air | ||||||||||||||||||||||
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Is it described by these equations? https://en.wikipedia.org/wiki/Optical_depth#Spectral_optical_depth
I have trouble finding PV specific information on a mathematical relationship. At least that is the only missing piece for me.