Skip to main content

Welcome to a Grasp lesson

Create a free account to keep studying and create your own study path.

Lesson 18

Solar PV: Characteristics and Grid Integration Challenges

Recommended resources

Hello! Welcome to the next lesson in your course on the UK electrical grid.

Introduction

In our last lesson, we delved into the challenges of integrating wind power into the grid, focusing on its non-synchronous nature, the resulting loss of system inertia, and the need for curtailment. We established that connecting generation via power electronics, rather than direct synchronisation, fundamentally changes grid behaviour.

Today, we turn our attention to the UK's other major renewable source: solar power. This lesson will address the learning outcome: Describe the characteristics and grid integration challenges of solar photovoltaic generation.

We will explore:

  1. How solar photovoltaic (PV) panels generate electricity.
  2. The key operational characteristics of solar power, including its variability and efficiency.
  3. The grid integration challenges, many of which it shares with wind power, and some which are unique.

By the end of this lesson, you will understand how solar PV works and how its characteristics create specific challenges for grid operators working to maintain a stable and reliable electricity supply.



1. How Solar Photovoltaic (PV) Generation Works

Before we can discuss the challenges of integrating solar power, we first need to understand its fundamental characteristic: how it converts light into electricity. Unlike the thermal power stations or wind turbines we've discussed, solar PV has no moving parts. The process happens silently at the atomic level.

The following video provides an excellent and clear explanation of the "photovoltaic effect" and the basic construction of a solar panel.

Generate Electricity - How Solar Panels Work!

This video from The Engineering Mindset explains the core principles of solar panel operation, from the photovoltaic effect to the construction of a solar cell.

Please watch the first four minutes of the video (00:00 - 04:11). The first section (00:09 - 01:57) explains the basic photovoltaic effect, where light particles (photons) knock electrons free to create a current. The second section (02:11 - 04:11) details the physical construction of a solar cell, including the silicon layers and conductors.

The key principle is that solar panels produce Direct Current (DC) electricity. As you'll recall from our previous lesson, the grid operates on Alternating Current (AC). This means that, just like modern wind turbines, every solar installation requires a device to convert DC to AC before the power can be used. This device is the inverter, and it is central to all the grid integration challenges we will discuss.



2. Key Operational Characteristics of Solar PV

Now that we know how solar panels work, let's examine their main operational characteristics.

Variability and Predictability

The most obvious characteristic of solar power is that its output depends on sunlight. This means it is inherently variable, changing with:

  • Time of day: Output follows a predictable curve, rising after sunrise, peaking around noon, and falling to zero at sunset.
  • Time of year: Longer summer days mean significantly more energy is produced compared to shorter winter days.
  • Weather: Cloud cover can cause rapid and significant drops in output.

However, it's a common misconception that solar panels require bright, direct sunshine to work.

Solar power: your questions answered

This article from National Grid answers common questions about solar power, including its performance in typical UK weather.

Read the first section, 'Do solar panels need bright sunshine in order to work?'. This clarifies how solar panels perform even on cloudy days.

While the output is variable, it is also predictable to a useful degree. We know the exact times of sunrise and sunset for every day of the year, providing a firm boundary on generation times. Weather forecasts also allow grid operators to predict solar output with increasing accuracy.

Efficiency and Temperature

Solar panel efficiency refers to the percentage of sunlight energy hitting the panel that is converted into electrical energy. Typical commercial panels have efficiencies in the range of 15-20%.

Interestingly, and somewhat counter-intuitively, solar panels are actually less efficient in very hot weather.

Solar power: your questions answered

Let's return to the National Grid article to see how temperature affects performance.

Read the short section titled 'Do solar panels stop working if the weather gets too hot?'.

While the efficiency drop per degree is small, it's an important characteristic. The ideal conditions for a solar panel are a bright, cool, sunny day, which is why they can perform very well in the UK's climate.

Cost

A defining characteristic of modern solar PV is its cost. Thanks to decades of manufacturing improvements and economies of scale, solar power has become one of the cheapest forms of electricity generation in history.

Briefing | Fact Checker

This fact-checker from Solar Energy UK, a trade association, provides context on the cost of solar in the UK.

Read the section under the question 'Is solar expensive?' on page 3. Focus on the trend of falling costs and its comparison to other forms of generation.

This low cost is driving the rapid adoption of solar power across the world and in the UK, which in turn makes understanding its grid integration challenges all the more critical.



3. Grid Integration Challenges

The challenges of integrating solar power stem directly from its characteristics: it is a variable, DC power source that connects to the AC grid via an inverter. This makes it an inverter-based resource (IBR), just like a modern wind turbine.

The following video is an excellent deep-dive into the challenges IBRs pose to a grid designed for traditional power plants.

Connecting Solar to the Grid is Harder Than You Think

This video from Practical Engineering uses a real-world grid disturbance in Texas to explain the complex issues that arise when integrating large amounts of solar power.

First, watch the introduction and the explanation of IBRs (00:00 - 04:43). This will set the scene and reinforce why solar (and wind) are fundamentally different from traditional generators.

Challenge 1: Non-Synchronous Generation and Low Inertia

This is the exact same challenge we identified for wind power.

  • Solar panels are connected via inverters, which electronically create a 50Hz AC waveform.
  • This means they are non-synchronous; there is no large, physical rotating mass synchronised with the grid.
  • As a result, solar PV does not contribute any natural rotational inertia.

As we learned in the last lesson, inertia acts as a shock absorber, slowing down frequency changes during a disturbance. A grid with high solar penetration and low inertia is more fragile, and the grid frequency can change very rapidly, giving operators less time to react to prevent blackouts.

Connecting Solar to the Grid is Harder Than You Think

Now, let's continue with the Practical Engineering video to see how this lack of inertia impacts grid frequency.

Watch the section on frequency response and inertia (09:50 - 13:30). Pay close attention to the graph showing how the rate of frequency drop is much steeper in a low-inertia system.

Challenge 2: The "Duck Curve" and System Ramping

The predictable daily output of solar power creates a unique challenge. As solar generation increases through the morning, it displaces the need for traditional power plants. Then, as the sun sets in the evening, that generation disappears very quickly, just as evening electricity demand is often peaking.

This forces the remaining power plants to ramp up their output extremely quickly to fill the gap. When you plot the shape of the demand that non-solar generators have to meet, it often looks like the silhouette of a duck—this is famously known as the "duck curve". Managing this steep evening ramp is a major daily challenge for grid operators in areas with a lot of solar power.

Challenge 3: Fault Ride-Through

Grid operators need to ensure that power plants don't disconnect from the grid during minor disturbances, as this could turn a small problem into a major one. If a fault causes a brief voltage dip, generators are expected to "ride through" it and continue operating.

However, the inverters used in solar farms are complex electronic devices with their own protective settings. As the Texas event described in the video showed, if these inverters are not programmed correctly, they might all trip offline simultaneously in response to a distant fault, leading to a sudden, massive loss of generation.

Connecting Solar to the Grid is Harder Than You Think

To conclude our look at challenges, let's watch the final key section from the Practical Engineering video on this topic.

Watch the section on 'Fault Ride-Through' (13:30 - 14:57). This explains the 'tug of war' between protecting the solar farm equipment and ensuring the stability of the entire grid.

Ensuring that millions of inverters from different manufacturers all behave in a predictable and helpful way during grid faults is a huge and ongoing engineering challenge.



Conclusion

In this lesson, we have built upon our understanding of renewable integration by focusing on solar PV. We've seen that while it shares fundamental challenges with wind power, it also has its own unique profile.

Key Takeaways:

  • Solar PV generates DC electricity via the photovoltaic effect, requiring an inverter to connect to the AC grid.
  • Its key characteristics are variability (dependent on sun and weather), decreasing efficiency at high temperatures, and very low cost.
  • Like wind, solar is a non-synchronous resource that reduces system inertia, making the grid less resilient to frequency disturbances.
  • Unique solar challenges include managing the steep evening "ramps" caused by the duck curve and ensuring thousands of inverters have the correct fault ride-through capability to prevent cascading failures.

Preview of the Next Lesson:

We have now examined the UK's main sources of renewable and conventional generation. But how does all this electricity get from the power plants to our towns and cities? In the next module, we will begin our exploration of the grid itself. The next lesson will describe the structure of the UK transmission network and voltage levels used (400kV, 275kV, 132kV).