Wavelet Variability Model

This is a help file for the pvl_WVM MatLab code. It contains links to examples and some FAQs. Click here to Download pvl_WVM Matlab Code

Contents:

What the WVM does
WVM Code Syntax and Required Inputs
Examples
Determining the Cloud Speed
Convert WVM Smoothed Irradiance to Power Output
References
BSD License

What the WVM does

The WVM models the average irradiance over a PV plant footprint. It does this by smoothing the measurements from an irradiance points sensor by different amounts at different timescales. The WVM smoothed irradiance can be used with irradiance to power translation methods to create simulated PV plant power output. To run the WVM, you need measurements from an irradiance point sensor, some information about the PV plant you’d like to simulate (see code syntax section and examples section below), and the cloud speed. See reference [1] for more details.

WVM Code Syntax and Required Inputs

Note you’ll need the PV_Lib toolbox installed on your computer to run the WVM. If you don’t already have it, get the PV_Lib toolbox here.

The WVM syntax is:

smooth_irradiance = pvl_WVM(irr_sensor, plantinfo, cloud_speed)

computes the spatially-smoothed irradiance using the wavelet variability model.

irr_sensor is a struct with variables:
irr_sensor.irr the irradiance measurement
irr_sensor.time the time stamps (Matlab time vector) for irr_sensor.irr
irr_sensor.Lat latitude of the sensor
irr_sensor.Lon longitude of the sensor
irr_sensor.alt altitude of the sensor
irr_sensor.tilt tilt angle of the sensor, 0 = flat (e.g., GHI)
irr_sensor.azimuth azimuth angle of the sensor, 180 = due south
(optional) irr.sensor.clear_sky_irradiance manually enter the clear-sky irradiance (e.g., for an irradiance sensor on a tracking system)
irr_sensor.UTCoffset UTC offset

plantinfo is a struct describing the plant to simulate with variables:

plantinfo.tilt tilt angle of plant modules

plantinfo.azimuth azimuth angle of plant modules

(optional) plantinfo.clear_sky_irrPOA manually enter the clear-sky irradiance in the module POA (e.g., for tracking systems)

plantinfo.type ‘square’,’polygon’, or ‘discrete’

‘square’ square PV plant with specified number of MWs and PV density

‘polygon’ custom PV plant shape (define vetiticies in lat/lon)

‘discrete’ simulate only certain points (e.g., to replicate output of multiple point sensors)

plantinfo.MW MW of PV installed (not necessary for ‘discrete’ type)

plantinfo.PVdensity W PV installed per m2 in plant area (e.g., 41 W/m2 is 1MW per 6 acres) (not necessary for ‘discrete’ type)

plantinfo.Lat (only needed for type ‘polygon’ or ‘discrete’) latitude of polygon verticies or discrete points

plantinfo.Lon (only needed for type ‘polygon’ or ‘discrete’) longitude of polygon verticies or discrete points

cloud_speed is a single value of the daily cloud speed

smooth_irradiance is the WVM smoothed irradiance representing the average irradiance over the plant footprint. It maintains the time stamps of the input irradiance (irr_sensor.time).

Examples

There are three basic ways to model the PV power plant:

Assume a square plant.

WVM example with a square plant.

This is the easiest method and requires only the plant MW rating and the PV density. A PV density of 41 W/m2 corresponds to 1MW per 6 acres, which is a common rule of thumb for PV plants.

Image of Square_Plant

Specify polygon vertices to define plant outline

Polygon WVM example

This setting allows you to simulate a PV plant that is not a square-shape by providing the latitude and longitude of the polygon vertices corresponding to the plant footprint.

Image of Polygon_Plant

Simulate the aggregate output at defined discrete points.

WVM example with discrete inputs.

This setting simulates the average irradiance measured using a network of irradiance point sensors. The WVM output on this setting will not be the average irradiance over the whole footprint, but rather the average of only the discrete locations of the point sensors. The user provides the latitude and longitude of the points to simulate.

Image of Discrete_Plant

Determining the Cloud Speed

The cloud speed is an important input to the WVM, but can be difficult to obtain. The slower the cloud speed, the greater the smoothing will be across the PV plant. Three ways to determine the cloud speed are:

  • Derive cloud speeds from numerical weather forecasts, as described in reference [2].
  • Use a ground network of irradiance sensors, e.g., as described in reference [3]. See the supporting program pvl_WVM_compute_CS_from_sensor_network that can be used to compute the cloud speed if you have an irradiance sensor network.
  • Make an educated guess. Based on [2] and other work, coastal areas such as Hawaii, Puerto Rico, and San Diego typically have slow cloud speeds (e.g., 3-7 m/s), probably due to the typically low-level clouds. Inland areas such as Las Vegas and Albuquerque typically have fast clouds speeds (e.g., 10-30 m/s), likely due to the typically high-level clouds.

Convert WVM Smoothed Irradiance to Power Output

The WVM simulates plant average irradiance, but plant power output is more often of interest. A variety of irradiance to power translation models exist, ranging from:

  • Simple linear models such as
    Power = Irradiance * Plant Area * Module Efficiency * DCtoAC Derate,
    where the DCtoAC Derate can be estimated from the PVWatts derates table (see Table 6). Since the rated capacity of the PV modules is usually more readily known than the module efficiency, this equation can alternatively be written as:
    Power = Irradiance/(1000 W/m2) * Rated Capacity * DCtoAC Derate.
  • Complicated models accounting for temperature, module and inverter technology, etc. Some such models are already included in the PV_Lib toolbox, such as pvl_sapm and pvl_snlinverter.

References

The main WVM references are:

1. Lave, M.; Kleissl, J.; Stein, J.S., “A Wavelet-Based Variability Model (WVM) for Solar PV Power Plants,” Sustainable Energy, IEEE Transactions on , vol.4, no.2, pp.501,509, April 2013, doi: 10.1109/TSTE.2012.2205716

2. Lave, M.; Kleissl, J; “Cloud speed impact on solar variability scaling – Application to the wavelet variability model”, Solar Energy, Volume 91, May 2013, Pages 11-21, ISSN 0038-092X, http://dx.doi.org/10.1016/j.solener.2013.01.023.

3. J.L. Bosch, Y. Zheng, J. Kleissl, Deriving cloud velocity from an array of solar radiation measurements, Solar Energy, Volume 87, January 2013, Pages 196-203, ISSN 0038-092X, http://dx.doi.org/10.1016/j.solener.2012.10.020.
(http://www.sciencedirect.com/science/article/pii/S0038092X12003854)

BSD License

Copyright (c) 2012, The Regents of the University of California

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