How a solar installation works – components, mounting, production and vocabulary

Eight minutes to know what we are talking about: the components, the mounting options, what makes output vary, and the vocabulary you will find on quotes.

Panels, inverter, meter: the full circuit

Pick a type of installation: the diagram shows the equipment required and the path electricity takes, from the roof to your sockets.

    kWp and kWh: the number one confusion

    The kWp (kilowatt-peak) measures the size of the system, like engine displacement: 1 kWp is about two panels and 5.5 m² of roof. The kWh measures the energy actually produced or used — what your supplier bills. Between the two sits a single figure: specific yield, the number of kWh one kWp produces where you live in a year. From Helsinki to Valletta it already varies twofold.

    The same panel produces more than twice as much in Malta as in Iceland. That is why solar economics can never be discussed without saying where you live — even within Europe.

    What makes output vary

    For the same specific yield, two roofs are not equal: orientation, tilt and shading make the difference. Move the sliders: the curve shows the power produced through the day, in winter, mid-season and summer, at your latitude.

      In the southern hemisphere, flip it: north produces the most. An east-west split loses about 15 % over the year but spreads output across the day — which raises self-consumption and often makes up for the loss.

      Shade: why so little costs so much

      A panel's cells sit in series: the current is that of the least lit cell. A small shadow therefore throttles a whole group of cells, and on a string inverter the whole panel can get dropped. Move the shadow and watch what is left.

        Classic string (panels in series)
        Micro-inverters or optimisers

        Simplified model: three panels with three bypass diodes each; the shadow is dense at the centre and lighter at the edges.

        Over the year, a chimney on an eight-panel array typically costs 10 %; micro-inverters recover 4 to 12 % depending on the shade (NREL measurements). Winter shadows count for little: the ones to avoid are those from April to September, between 10:00 and 16:00.

        Why tilt and hemisphere matter

        A panel produces most when the rays strike it head-on. But the noon sun is not at the same height at every latitude or season: tilting the panel turns it towards where the sun passes most often. Drag the sliders.

        Left, the view from the ground: the noon sun, the panel and the share of rays it captures, compared with a flat panel. Right, the cause: the Earth's axis, tilted by 23.4°, raises and lowers the sun through the year, all the more the farther you are from the equator.
        • 1The farther from the equator, the lower the sun — and the steeper the panel must be to face it. The ideal tilt over the year is roughly the latitude, a little less to favour summer.
        • 2A compromise, not an absolute. Between 20° and 45° you rarely lose more than 5 % against the ideal: keep your roof's slope. Flat, you lose 10 to 15 % and rain cleans less well.
        • 3In the southern hemisphere everything flips: the noon sun is in the north, panels face north and the most productive month is December. At the equator it crosses from one side to the other with the seasons — a nearly flat panel does best.

        From sunlight to meter: what is lost on the way

        A panel rated 1 kWp almost never delivers 1 kW. Between the nameplate rating and the electricity reaching the meter sit well-known losses, whose sum is called the performance ratio.

        A performance ratio of 80 % is normal on a decent installation, and it is already built into the calculator's figures. A tree or a chimney shading part of the array, however, can cost another 10 to 30 % on its own.

        The vocabulary, one line each

        You have the vocabulary. Now let us see what it means at your place, with your own figures.

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