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Merge remote-tracking branch 'origin/sh/#688-rewrite-pv-model' into sh/
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SimonHuette committed Dec 20, 2023
2 parents 66cd6eb + 55f24cd commit e7473d0
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1 change: 1 addition & 0 deletions CHANGELOG.md
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Expand Up @@ -32,6 +32,7 @@ and this project adheres to [Semantic Versioning](https://semver.org/spec/v2.0.0
### Fixed
- Removed a repeated line in the documentation of vn_simona config [#658](https://github.com/ie3-institute/simona/issues/658)
- Removed version number "2.0" from the logo printed to console [#642](https://github.com/ie3-institute/simona/issues/642)
- Fixed PV Model documentation [#684](https://github.com/ie3-institute/simona/issues/684), [#686](https://github.com/ie3-institute/simona/issues/686)

## [3.0.0] - 2023-08-07

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16 changes: 8 additions & 8 deletions docs/readthedocs/models/pv_model.md
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Expand Up @@ -254,7 +254,7 @@ $$
\end{eqnarray*}
$$

Additionally, the condition $$\theta_{g} < 90°$$ must be met (sun must not be behind the surface).
Additionally, the condition $\theta_{g} < 90°$ must be met (the sun must not be behind the surface).

*with*\
**$\omega$** = hour angle\
Expand All @@ -280,7 +280,7 @@ b = (\cos(\phi) \cdot \cos(\delta)) \cdot (\sin(\omega_{2}) - \sin(\omega_{1}))
$$

$$
E_{dir,S} = E_{dir,H} \cdot \frac{a}{b}
E_{beam,S} = E_{beam,H} \cdot \frac{a}{b}
$$

**Please note:** $\frac{1}{180}\pi$ is omitted from these formulas, as we are already working with data in *radians*.
Expand All @@ -292,7 +292,7 @@ $$
**$\omega_1$** = hour angle $\omega$\
**$\omega_2$** = hour angle $\omega$ + 1 hour\
**$\alpha_e$** = surface azimuth angle\
**$E_{dir,H}$** = beam radiation (horizontal surface)
**$E_{beam,H}$** = beam radiation (horizontal surface)

**Reference:**

Expand All @@ -307,7 +307,7 @@ The diffuse radiation is computed using the Perez model, which divides the radia
A cloud index is defined by

$$
\epsilon = \frac{\frac{E_{dif,H} + E_{dir,H}}{E_{dif,H}} + 5.535 \cdot 10^{-6} \cdot \theta_{z}^3}{1 + 5.535 \cdot 10^{-6} \cdot \theta_{z}^3}
\epsilon = \frac{\frac{E_{dif,H} + E_{beam,H}}{E_{dif,H}} + 5.535 \cdot 10^{-6} \cdot \theta_{z}^3}{1 + 5.535 \cdot 10^{-6} \cdot \theta_{z}^3}
$$

Calculating a brightness index
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**$\gamma_{e}$** = slope angle of the surface\
**$I_{0}$** = Extraterrestrial Radiation\
**$m$** = air mass\
**$E_{dir,H}$** = direct radiation (horizontal surface)\
**$E_{beam,H}$** = beam radiation (horizontal surface)\
**$E_{dif,H}$** = diffuse radiation (horizontal surface)

**References:**
Expand All @@ -422,7 +422,7 @@ E_{ref,S} = E_{Ges,H} \cdot \frac{\rho}{2} \cdot (1-
$$

*with*\
**$E_{Ges,H}$** = total horizontal radiation ($E_{dir,H} + E_{dif,H})$\
**$E_{Ges,H}$** = total horizontal radiation ($E_{beam,H} + E_{dif,H})$\
**$\gamma_e$** = slope angle of the surface\
**$\rho$** = albedo

Expand All @@ -437,11 +437,11 @@ $$
Received energy is calculated as the sum of all three types of irradiation.

$$
E_{total} = E_{dir,S} + E_{dif,S} + E_{ref,S}
E_{total} = E_{beam,S} + E_{dif,S} + E_{ref,S}
$$

*with*\
**$E_{dir,S}$** = Beam radiation\
**$E_{beam,S}$** = Beam radiation\
**$E_{dif,S}$** = Diffuse radiation\
**$E_{ref,S}$** = Reflected radiation

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