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# Incident power density: correctly measuring panel performance

In our previous introduction article about Ohm’s Law, the importance of knowing the source resistance Rs to measure the degree of a module’s miserliness was explained. It is one of the two important variables which control how much maximum power the panel will transfer to a load.

In continuation of Ohm’s Law and miserly solar modules, in this article we explore the core importance of heavenly impact factors on a module’s miserliness and how to measure the related performance parameters.

## The importance of load resistance

Basically, from an engineering perspective we are not so much talking about what a PV module will offer, but what it will give. It also determines how much resistance such a lucky load should represent in order to obtain maximum power from the module.

That is because of a very popular theorem in electrical engineering: the so-called maximum power transfer theorem.

This theorem basically states that in order to get the maximum power out of a source, the resistance of the load must be identical to the internal source resistance.

## Incident power densitiy – heavenly intervention

Apart from the source resistance, the second controlling parameter is the open circuit voltage (Voc). This is the terminal voltage of the module when no current is being drawn from it.

It is important to remember that these two parameters Rs and Voc are variables that depend not only on the module technology and construction but also on the ambient light level, angle, tilt and the orientation of the module with respect to the sun.

Hence, each is valid only for a specified incident power density.

Why should the module output properties like Voc and Rs depend on the incident power density? That is because the module virtually only provides an ‘arena’ for the sunlight photons to play.

Photons of the correct energy create electron-hole pairs from the silicon atoms in the panel. Electrons are minority carriers in the p-region. Some of these manage to escape recombination and breach the junction. The field in the deletion region pushes the electrons to the n-side where they are the majority carriers.

Similarly, some holes from the n-region are pushed across to p-region. This charge accumulation creates a potential difference across the terminals.

That is why it is not the module’s raw technical specifications alone that determine its performance properties. Module properties are strongly controlled by the density of solar power incident on the module’s area.

This is not the only mode of seemingly ‘heavenly intervention’. Even minor shading of a cell in the module also changes these parameters and strongly affects the performance of the cell string and as such the whole module.

Multimeter – used to measure Amps

## Measuring Voc and Rs

So how do we measure Voc and Rs, these two core parameters of solar modules (and of course other electrical systems, small and large)?

Measuring Voc is simple. All you need is a voltmeter. Unless you want to measure it under a specific set of conditions, simply position the module to face the sun and connect the voltmeter across the terminals of the module taking due note of the polarity. The voltage read on the meter is the open circuit voltage Voc of the panel under the prevalent conditions.

Of course you know that while measuring, you should of course not block the sun from the module. Theoretically, even your presence close to the ray path can affect the result due to scattering from the clothes you wear.

Evaluating Rs is trickier. Theoretically, Rs and Isc could be measured by short circuiting the panel terminals through an ammeter (of course, with a low internal resistance).

However, a short circuit condition must be avoided unless prior knowledge is available about it being a safe condition. In the case of solar modules, luckily, short circuiting the module output will normally not damage it. But in case of most circuits, short circuiting the output can have tragic results.

The other alternative is to apply a variable load resistance, and note when the voltage reduces to half of the open circuit value. At this moment, the load resistance and the source resistance are sharing the total open circuit voltage equally. Hence, your load resistance is equal to the source resistance.

Needless to say, both Voc and Rs must be measured under the same lighting conditions.  For this reason, formal testing on commercial level is done in specialized labs which can produce standard illumination conditions, and have sophisticated measurement equipment.

## Comment Section

2 thoughts on “Incident power density: correctly measuring panel performance

### By Magzoub on 14 November 2015

Thankful me best Solar information team .
How can that internal resistance measuring of the module be a whight for the pannel quality and performance?
Thank

### By Niclas on 18 November 2015

Hi Magzoub, thank you for your kind feedback. The internal series resistance is an important performance parameter impacting voltage and current. If you look at an I-V curve you can regard it as the factor that – when increasing – moves the curve away from the optimal maximum power point (the intersection of Vmp and Imp), thus effectively reducing the fill factor (squareness of the I-V curve).

Niclas is co-founder of the Sinovoltaics Group and Quality Director at 3rd party PV Quality Assurance company Kisun Solar. He is based in Shanghai and has been living and working in Asia for 9 years, including Mainland China, Taiwan, India and Iran. Niclas is PV quality specialist with extensive experience with manufacturers in Asia and has before worked on clean energy projects at UNIDO and Grameen Shakti. Connect with Niclas on LinkedIn