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  1. “Array Thermal Losses.” PVsyst Website.

  2. Cameron, C.P., Stein, J.S., & Tasca, C.A. “PV Performance Modeling Workshop Summary Report.” May 2011.

  3. “Technology Assessment, Earth Mount SolarTM PV System.” DNV Bankability Report. March 16, 2022.

  4. Faiman, D. “Assessing the outdoor operating temperature of photovoltaic modules.” Progress in Photovoltaics

    16(4): 307-315. 2008.


Earth Mount Solar arrays experience significant heat dissipation — and high levels of overall energy performance — as a result of their installation directly on the ground. This is because the ground acts as a thermal sink, pulling heat from the underside of the modules and cooling the system. This, in turn, leads to improved module efficiency and energy yield. Real-world data gathered at an Earth Mount Solar project site over a span of five months confirmed and quantified the positive impact of ground-driven heat dissipation on the performance of the Earth Mount Solar system.


Furthermore, DNV’s analysis of this same data suggested that anyone using PVsyst to estimate the heat dissipation of an Earth Mount Solar system use an Apparent Uc value of 18.5 W/m2K — this value will deliver reliable (if conversative) performance predictions that fall within the standard range of uncertainty. A PVsyst model using this value will establish a baseline of expected performance for Earth Mount Solar plants.


The results from Bear Mountain — both modeled and real — show that the Earth Mount Solar system has achieved measured thermal performance that is comfortably within accepted industry parameters, with annual per-array energy outcomes that make it competitive with the highest-performing system configurations on the market today.

As noted already, and as evidenced in Figure 6, the Apparent Uc value of 18.5 is a conservative estimate provided by DNV that is intended to serve as a baseline of expected heat dissipation performance in an Earth Mount Solar system. While this estimate already places Earth Mount Solar installations well within the industry’s widely accepted performance norms, the actual heat dissipation (U) value as measured at the Bear Mountain test site significantly exceeded this baseline prediction, with a total U value of 22.8 W/m2K. The difference observed in these values (18.5 and 22.8) is likely explained by the presence of the ground, which acts as a seasonally variable thermal sink that draws heat away from the underside of the Earth Mount Solar array — a phenomenon not able to be modeled by the current version of PVsyst (v7.2), and the full thermal impact of which continues to be studied. For example, our own early test results demonstrate that soil that has been treated with geoenzymes to a depth of six inches — as is common under Earth Mount Solar arrays — can lower the temperature of modules resting on top of that soil by more than 1°C on average.


We will publish a revised version of this white paper as more data confirming or disconfirming these promising preliminary findings become available.

Figure 6 — Heat dissipation values and energy yield of common mounting configurations, including Earth Mount Solar


With a conservatively estimated Apparent Uc value of 18.5W/m2K — based on nearly six months of data collected in five-minute intervals, spanning all hours of each day over parts of three seasons — we can now compare the expected thermal performance and resulting energy yields of Earth Mount Solar systems to more traditional installation types.


We previously provided a table (Figure 1) that showed the heat dissipation and energy yield factors for the main traditional solar installation types in use today. Here, we have repeated that table with the Earth Mount Solar values added. As you can see, when factoring in the thermal dissipation properties of the ground (Ug), Earth Mount Solar compares favorably to other widely used installation types.

The Bear Mountain test data strongly suggests that 18.5 is a reliable (if conservative) Uc estimate for use in PVsyst, and therefore that the baseline energy performance of an Earth Mount Solar installation can be accurately predicted with PVsyst using that value.

Figure 5 — PVsyst-predicted energy vs. actual energy output measured at the grid at Bear Mountain

Based on the robust dataset gathered at the Bear Mountain site, the DNV team conservatively estimated that an Apparent Uc “of 18.5 W/m2K and a convective heat transfer coefficient of 0 W/m2K/m/s are the most relevant values for use with Bear Mountain operational data.”


The use of 18.5 W/m2K as a conservative Apparent Uc value is further validated by the data presented in Figure 5. As you can see, the energy measured at the grid at the Earth Mount Solar site is almost perfectly in line with PVsyst’s modeled power predictions of the same system over the same timeframe, with the real-world energy output in fact slightly outperforming the modeled prediction.

Figure 4 — Time-dependent Uc plotted over five months

Furthermore, DNV observed that the appropriate Uc value “varies seasonally, with drier, warmer weather showing an effective coefficient near 15 W/m2K,” while in cooler weather, when the ground absorbs more heat, the Uc value reached above 25 W/m2K. This observation is represented in Figure 4, which shows the relationship between the Uc value and the time of year, as measured at the Bear Mountain site.

Figure 3 — Full five-month dataset of total heat dissipation at Bear Mountain, color-coded by hour of day

DNV then took the raw information shown in Figure 2 and plotted each data point by the hour of day at which it was recorded. The resulting scatterplot is shown in Figure 3 below, where the relationship between time of day and the value of Uc becomes more apparent.

Figure 2 — Full five-month dataset of total heat dissipation at Bear Mountain

Data Collection at Bear Mountain

In order to demonstrate the extent to which the ground acts as a heat sink upon Earth Mount Solar modules, it was necessary to measure back-of- module temperatures at Bear Mountain at sub-hourly intervals across multiple seasons. This was done with silver, epoxy-mounted resistance temperature detectors, which captured back-of-module temperatures every five minutes from August 6, 2021 through January 22, 2002. When looking at the raw unit regression for the full dataset (Figure 2), we observed 22.8 W/m2K of total power or heat dissipation prior to accounting for the time of day that each data point was recorded.

The Bear Mountain Project Site

In August 2021, Erthos completed the installation of a 200kWac Earth Mount Solar array at Bear Mountain in Bakersfield, California. We have since gathered robust datasets from the Bear Mountain site, which consists of 720 380W solar modules and four 50kWac inverters. We have thoroughly analyzed these datasets, performed further regression calculations to determine the Bear Mountain array’s baseline U-heat dissipation rates and back-of-module temperature fluctuations, and asked DNV to provide an independent, third-party validation of our approach, assumptions, and results, which they did as part of a broader technological assessment report on the Earth Mount Solar system.

Modeling Heat Dissipation in Earth Mount Solar™ PV

These heat dissipation and energy yield values represent the range of thermal performance outcomes considered acceptable in the industry today, as each of these system types is commonly used across the world. In the next section, we share our data from the Earth Mount Solar installation at Bear Mountain and compare the values found there with the values identified above. As you will see, Earth Mount Solar PV compares favorably to these systems and sits comfortably within the industry’s established thermal performance expectations.

Figure 1 — Heat dissipation values and energy yield of common mounting configurations

Heat Dissipation and Energy Yield in Traditional Solar Installations

The typical heat dissipation values for the most common traditional solar installation types are shown in Figure 1 below, not including Earth Mount Solar [4]. To provide for easier comparison of these systems, we have added what we call an “energy yield factor,” which predicts the expected annual energy yield (MWh/year) of a given system type in relation to the expected annual energy yield of flush rooftop PV. A system that has an energy yield factor of 1.13, for example, can be expected to produce 13% more energy over the course of a year than a standard flush rooftop PV system.

Using Apparent Uc as a Substitute for Ug

The PVsyst model includes only two editable U-terms: Uc (the amount of constant heat dissipation) and Uv (the amount of heat dissipation due to wind). It is not possible to manipulate the U-total data within PVsyst. However, to accurately predict heat dissipation and overall thermal performance in an Earth Mount Solar system, we require a third term (“Ug”) that represents the heat-sink effect of theground upon the modules.

Since this term is not currently offered within PVsyst’s model, we employed a workaround, endorsed by DNV in their technological assessment report of the Earth Mount Solar installation at Bear Mountain, that we call Apparent Uc — a substitution of the standalone Uc variable used in PVsyst with a more comprehensive version that combines Uc and Ug. This allows us to better account for the earth’s heat sink effect and quantify its impact on the thermal performance of the modules resting upon it.


DNV agreed with this approach and recommended using a thermal coefficient (or Apparent Uc) of 18.5 W/m2K. This figure was based on their review of the ambient and back-of-module temperature data generated at the site, their recognition of the need for a geothermal coefficient derived from measured soil temperature, and an assumption of no wind dependence (Uv = 0) since the modules sit on the ground. We adopted the DNV recommendation to use 18.5 as our Apparent Uc term, which provided energy modeling outcomes that aligned with (and in fact slightly underperformed) the real-world Bear Mountain data. We highly recommend reading the full DNV report for more details on this specific point, but the general takeaway is this: by using an Apparent Uc value of 18.5 W/m2K in PVsyst, we can generate Earth Mount Solar energy predictions that are “well within the typical uncertainty of standard energy estimates" [3].

Here, Uc is the amount of heat dissipation constant to the module, Uv is the amount of heat dissipation due to wind, and vwind is the wind velocity.

These equations aren’t perfect. As noted on PVsyst’s website, “The determination of the parameters Uc and Uv is indeed a big question. We have some reliable measured data for free mounted arrays, but there is a severe lack of information when the modules are integrated” [1].

The same lack of information applies to modules installed directly on the ground, which introduces heat transfer dynamics that are quite different from those seen in building-integrated systems: whereas the roof or wall of a building is insulative, blocking the free flow of air around the module as well as trapping heat, the earth acts as a heat sink, drawing heat away from the underside of the Earth Mount Solar array and cooling the system.


Because PVsyst uses only two heat dissipation terms, it is unable to natively account for this radiative heat transfer from an Earth Mount Solar array to the underlying earth. According to a report published by Sandia National Laboratories, failure to model the heat dissipation of modules “relative to their mounting configuration” can lead to heat dissipation predictions that are off by 10% or more [2].


These shortcomings are understandable. Until recently, it has not been common or practical to install modules directly on the ground. As a result, there has been no industry need for equations that accurately capture the heat dissipation properties of such systems.


That has now changed with the introduction of Earth Mount Solar. While we fully expect future versions of PVsyst to better account for radiative factors, especially given the transformative potential of solar arrays installed directly on the ground, we needed a revised model in the meantime that enables more accurate heat dissipation and energy yield predictions in such systems. As a solution, we have utilized what we call Apparent Uc — a concept explained in more detail in the following section.

Here, Tcell is the module operating temperature, Tamb represents ambient temperature, α (or Alpha) is the absorption coefficient of solar radiation, Ginc is the amount of radiance hitting the PV plane, and ηmod is the efficiency of the module according to operating conditions.


To calculate the U-value, which represents the overall heat dissipation factor, PVsyst uses the following equation:

Standard Heat Dissipation Modeling

In order to accurately predict the performance of photovoltaic (PV) power plants, it is necessary to first understand how the solar modules in your specific project will dissipate heat during operation. It is not enough to understand the thermal performance of solar modules generally. There are numerous factors — including installation method, module construction, wind patterns, and others — that affect how much heat is dissipated by a module, and the impact of each of these factors on thermal performance can be different from project to project.


Because of its widespread acceptance and use within the solar industry, we chose to use PVsyst to model the thermal performance of the Earth Mount Solar installation at the Bear Mountain site in Kern County, California. This approach allows for the most accurate baseline comparisons to be made between Earth Mount Solar systems and the most common traditional system types in use today.

The PVsyst model of heat transfer is as follows:

Modeling the Thermal Performance of Solar Modules


PVsyst is a simulation software program that enables the user to model the expected thermal performance of their solar installation in order to accurately estimate production. It is the most widely used such program in the industry today. However, it was developed with elevated fixed-tilt and tracker systems in mind and therefore does not sufficiently consider the ground-based, heat-sink effect that the soil imparts on the thermal performance of Earth Mount Solar™ systems, which are installed directly on the ground.


This paper details a solution to this problem — a concept called Apparent
 — that enables users of PVsyst to accurately represent this missing geothermic variable and better predict the expected energy production values of an Earth Mount Solar system. This solution was endorsed by DNV, an independent third-party engineering firm that conducted a thorough technological assessment of Earth Mount Solar, including close analysis of real-world data generated at an Earth Mount Solar project site over a period of five months. This analysis led DNV to recommend an Apparent Uc value for PVsyst of 18.5 W/m2K.


Using DNV’s recommended Apparent Uc value of 18.5, PVsyst modeling showed that Earth Mount Solar arrays perform comfortably within accepted industry parameters for heat dissipation and overall energy performance.

Modeling Heat Dissipation in Earth Mount Solar™ PV

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