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Rooftop solar panels

How Delve estimates the potential for solar power

Updated over a year ago

Solar Yield

Delve estimates solar yield as the average amount of radiation received from direct and diffuse sunlight, measured in kilowatt hours per square meter (kWh/m^2). In addition, Delve converts the solar yield into an estimate of on-site generated energy and associated reduction in operational emissions.

These calculations are based on the orientation of buildings in each design and historical weather data for the local climate and weather.

Solar Panels

Delve generates solar panels assumed to produce 345 Watts with an efficiency of 18%, a DC-to-AC derate factor of 85%, and industry-standard assumptions about other factors. The standard panel size is 78 in by 39 in (1.98m by 0.99m), which corresponds to a commercial-sized solar panel.

We place those solar panels on buildings in accordance with the International Fire Code's Energy Systems requirements. These standards guide solar panel placement, inclusion of interior pathways and a setback from the roof’s edge. In order to maximize efficiency, we only include solar panels that are less than 25% shaded and in an array of at least 4 panels.

Data Sources

Delve combines data from multiple sources to compute the available solar yield and the associated carbon footprint. Details on each source can be found below:

  1. Solar Irradiance Data: The underlying data is Typical Meteorological Year 3 (TMY3) Data sourced from the US Department of Energy. This dataset typifies hourly weather conditions over the period of a year from a 1991-2005 period of record in 1,020 USA locations.

  2. Roofs: Roof surfaces extracted from buildings and evaluated by Delve

How is Solar Yield calculated?

A solar dome is created using data derived from an input EnergyPlus Weather (EPW) data file specific to project location. This data includes information such as Direct Normal Irradiance (DNI) and Diffuse Horizontal Irradiance (DHI) which are used to create solar lookup tables containing each ray angle within the solar dome.

Roof areas on generated buildings are sampled using a 5 by 5 meter grid, and tested for direct line of sight to the solar dome, accounting for overshadowing from adjacent buildings. The total visible exposure can then be summed for the available roof area amount to estimate the total solar radiation over the course of a year.

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