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Discover how much electricity to expect from your solar panels and what affects production with our guide.
In the simplest terms, solar panels convert energy from sunlight into electrical power using photovoltaic (PV) cells. But how much electricity can a solar panel produce?
According to our calculator, a 4.5 kilowatt (kW) system with 12 panels would produce on average 4,100 kilowatt hours (kWh) in a year, enough for a 3 bedroom house.
However, there are a range of factors that can affect how much electricity your solar panels produce, from the efficiency of your system to the angle of your roof. Our guide below takes you through everything you need to know.
In the simplest terms, solar panels convert energy from sunlight into electrical power using photovoltaic (PV) cells.
A PV cell is constructed using semiconductor materials, usually silicon. Sunlight is composed of particles called photons, which strike these cells and displace electrons in the semiconductor material.
The cells’ internal electric field captures and channels the displaced electrons and produces an electric current.
The electric current flows into a solar system component known as an inverter, which turns the direct current (DC) from the solar panel into alternating current (AC) that can power household appliances.
The average home can save more than £1,100 every year with solar panels!
Specific types of measurements are used to gauge solar panels’ output and performance.
Assessments of wattage are at the heart of any discussion about solar panels.
In addition to wattage ratings, we also need a broader metric that measures energy usage over time.
This is where kWh comes into play.
The actual performance of solar panels can vary because of real-world conditions.
To contextualise the potential of solar panels:
Here are 3 examples of how solar power generation differs across the UK for various types and scales of solar systems:
Before we dive into solar panels’ power output and functionality, it’s important to understand the key factors influencing how panels harness the sun’s energy.
You can think of solar irradiance as the sunlight’s brightness or intensity at a specific time and place. Solar irradiance is measured in terms of how much solar energy is received per unit of area, which is usually expressed as W/m^2.
Measuring solar irradiance enables you to understand how much energy a solar panel can capture. In the UK, the average solar irradiance is around 101W/m^2. It ranges from 128.4W/m^2 in the south of England to 71.8 W/m^2 in the northwest of Scotland.
However, this value can spike on particularly sunny days, especially in the summer, when it often ranges between 600 and 800W/m^2.
Solar insolation refers to the total amount of solar energy received at a particular location over a specific period, which is typically expressed as kWh/m^2.
While measuring solar irradiance gives a snapshot of energy output, measuring solar insolation shows the big picture. Annually, insolation in the UK ranges between 750 and 1,100kWh/m^2. This is an average of roughly 2.53kWh/m^2 per day (using the midpoint value of 925kWh/m^2 per year).
Efficiency is the fraction of the incident solar energy (radiant solar energy that hits the Earth) that a solar panel can convert into usable electricity. A solar panel typically has 15 to 22% efficiency.
For instance:
Panel size is a significant determinant of solar energy production.
Geographic location plays a major role in solar energy production. Solar insolation, which is the amount of energy harnessed annually per square metre, greatly varies worldwide.
Latitude is a measure of how far north or south a place is from the Earth’s equator and it plays a significant role in solar intensity.
Near the equator, sunlight beams down almost directly, providing a higher concentration of solar energy. Closer to the North and South Poles, sunlight hits the Earth more obliquely, spreading over a larger area and losing its intensity.
This is why solar panels in tropical regions can produce more energy than those in higher latitudes.
Insolation in London reaches 1,100 kWh/m^2, in New York, it’s 1,300 kWh/m^2, and in the Sahara, it’s a considerably higher 2,800 kWh/m^2. This figure varies widely, even in the UK.
The tilt of the Earth’s axis causes daytime lengths to vary as the Earth orbits the sun. Longer summer days offer more sunlight hours, maximising solar energy potential.
Shorter winter days in high-latitude regions offer drastically reduced sunlight hours and less potential energy. It’s not just about the total hours of daylight, though.
Peak sunlight hours are especially crucial. A summer day might be long but nevertheless have a relatively short period in which solar generation conditions are ideal. For example, London receives 0.52kWh/m2 of solar energy per day in December and 4.74kWh/m2 of solar energy per day in July.
The amount and intensity of sunlight are just one part of the solar energy equation. Local weather conditions and climate are another. They can either boost or hinder solar panel efficiency.
Clouds, fog and precipitation can obstruct sunlight, decreasing solar output. Solar panels still function on cloudy days but have a lower efficiency than they do when the weather is clear and sunny.
We associate solar panels with bright, sunny conditions, but temperature also affects the panels’ efficiency. Extreme heat can reduce a solar panel’s performance. So, in regions such as the Sahara, the impact of impressive solar intensity is partly diminished by the effects of extreme heat. Cooler, sunny days in other parts of the world can offer better conditions for solar panels.
Solar panels’ performance largely depends on their orientation and tilt angle.
Solar panels operate at peak efficiency when they directly face the sun. In the Northern Hemisphere, this translates to a southern orientation. The sun’s journey from the east at dawn to the west at sunset means that panels pointing due south maximise their exposure to sunlight throughout the day. However, even if a roof doesn’t point directly south, the panels on it are far from useless.
Solar panels with southwestern or southeastern orientations achieve around 85 to 90% of the potential energy output of panels with southern orientations.
The tilt or pitch of the solar panels also plays a pivotal role in their energy generation capacity.
An ideal pitch allows the panel to absorb the maximum amount of sunlight, especially during peak hours.
In the UK, a 35-to-40-degree tilt angle is deemed optimal for fixed installations.
Solar tracking systems follow the sun’s movement. They reduce the tilt in summer and increase it in winter to enhance sunlight capture throughout the changing seasons. In London, the optimal summer angle is around 34 degrees, and the optimal winter angle is around 66 degrees.
Solar trackers are advanced systems that automatically adjust the panels’ orientation and tilt throughout the day, ensuring that they always face the sun in the most optimal manner possible.
It’s a common misconception that direct sunlight is the sole contributor to a solar panel’s output. Around half of the UK’s light energy is diffused by clouds or reflected off buildings and the ground. Because the light is diffused, even panels that aren’t perfectly oriented can generate substantial energy.
Solar panel costs, efficiency and lifespan are all factors that affect the overall output.
Here are the most common types of solar panels:
Monocrystalline panels are the most commonly used type of panel for domestic and commercial solar arrays. They are built from a single crystal structure and are considered the benchmark panel technology.
These panels have a sleek appearance and are a uniform shade of black. Their efficiency rates range from 15 to 22 per cent and are generally the more expensive panels to buy.
Polycrystalline panels have multiple crystal structures in each of their cells. The panels are made of silicon fragments that have been melted and poured into moulds. Their efficiency rates typically range from 13 to 18 per cent, so are not generally as efficient as monocrystalline panels.
However, the price point of polycrystalline panels is generally lower, making them an attractive option for property owners who have ample installation space on their roofs or are on tight budgets.
While monocrystalline and polycrystalline panels’ structures are rigid, thin-film panels’ structures are slim and flexible. Thin-film panels can be applied to a broad range of surfaces, including some that are unsuitable for traditional panels.
Thin-film panels’ efficiency rates generally range from 10 to 12 per cent. These panels are a viable alternative when there aren’t space constraints for solar systems or when traditional solar panels can’t be used.
The solar industry has experienced rapid advancements in recent years, which have pushed the boundaries of panel performance. Advanced solar technologies include bifacial solar panels, which capture sunlight on both sides, and solar skins, which blend seamlessly with buildings.
Manufacturers are also developing materials such as perovskite, which offers advantages over silicon.
Recent developments in panel technology that substantially boost electricity production include tandem solar cell designs, which layer different materials to capture a broad spectrum of sunlight.
Advanced manufacturing techniques reduce the space between the cells in a panel, which results in higher power outputs.
Also, innovations in inverter technology and solar tracking systems are optimising the conversion and capture of solar energy and further boosting overall system efficiency.
Upcoming technologies include transparent solar cells, which show promise. They have the potential to transform windows and other surfaces into power generators without obstructing light or views.
Perovskite cells are another upcoming technology. They can absorb light across a broader spectrum than silicon cells. And perovskite cells can be engineered at the molecular level to optimise their light absorption performance.
Solar power is one of the most important forms of renewable energy we can access. Understanding the electricity production capacity of solar panels is crucial for anyone who is considering switching to solar energy.
Irradiance and insolation are fundamental keys to understanding solar energy production. Panel efficiency, size and output ratings govern how much solar energy can actually be captured.
It’s crucial to understand that solar systems involve more than just panels. You must also factor in inverters, batteries and other components.
A 375W solar panel can on average produce 0.94 kWh a day, according to our solar calculator.
If one 375W solar panel can produce around 28.5kWh a month, you would need roughly 35 solar panels to generate 1,000kWh each month.