IDEAS home Printed from https://ideas.repec.org/a/eee/renene/v246y2025ics0960148125004720.html
   My bibliography  Save this article

Tilt and light-scattering dependent physics-based model for the temporal evolution of soiling loss of solar panels

Author

Listed:
  • Ryyan Khan, M.
  • Didarul Islam, Mohammad
  • Sajjad, Redwan N.

Abstract

Numerical models for solar farms are used to model various loss mechanisms and find designs that are techno-economically viable. Soiling is a prominent concern among these losses. The current soiling models utilize daily soiling loss rates, neglecting factors such as panel tilt and solar angle of incidence (AOI). This results in inaccurate temporal performance prediction. In this paper, we present a time-series model for dust accumulation and the corresponding scattering of sunlight and soiling loss. The effects of ambient dust, dust-surface interaction, and panel tilt are phenomenologically modeled. We then present a physics-based model that incorporates the scattering of direct, diffuse, and albedo lights from the accumulated dust. The model also demonstrates the change of soiling loss on the degree of cloudiness. On cloudy days, for example, the AOI dependency is less prominent as the sunlight is less directional, and the soiling loss is higher. The temporal predictive model has been validated using experimental data collected for various panel tilts and seasons. The modeled daily soiling ratio matches well with the data, achieving RMSE<1.35% and r2>0.965. Such a model with diurnal predictions is important for accurate solar-farm modeling and decoupling degradation analysis from soiling losses.

Suggested Citation

  • Ryyan Khan, M. & Didarul Islam, Mohammad & Sajjad, Redwan N., 2025. "Tilt and light-scattering dependent physics-based model for the temporal evolution of soiling loss of solar panels," Renewable Energy, Elsevier, vol. 246(C).
  • Handle: RePEc:eee:renene:v:246:y:2025:i:c:s0960148125004720
    DOI: 10.1016/j.renene.2025.122810
    as

    Download full text from publisher

    File URL: http://www.sciencedirect.com/science/article/pii/S0960148125004720
    Download Restriction: Full text for ScienceDirect subscribers only

    File URL: https://libkey.io/10.1016/j.renene.2025.122810?utm_source=ideas
    LibKey link: if access is restricted and if your library uses this service, LibKey will redirect you to where you can use your library subscription to access this item
    ---><---

    As the access to this document is restricted, you may want to search for a different version of it.

    Corrections

    All material on this site has been provided by the respective publishers and authors. You can help correct errors and omissions. When requesting a correction, please mention this item's handle: RePEc:eee:renene:v:246:y:2025:i:c:s0960148125004720. See general information about how to correct material in RePEc.

    If you have authored this item and are not yet registered with RePEc, we encourage you to do it here. This allows to link your profile to this item. It also allows you to accept potential citations to this item that we are uncertain about.

    We have no bibliographic references for this item. You can help adding them by using this form .

    If you know of missing items citing this one, you can help us creating those links by adding the relevant references in the same way as above, for each refering item. If you are a registered author of this item, you may also want to check the "citations" tab in your RePEc Author Service profile, as there may be some citations waiting for confirmation.

    For technical questions regarding this item, or to correct its authors, title, abstract, bibliographic or download information, contact: Catherine Liu (email available below). General contact details of provider: http://www.journals.elsevier.com/renewable-energy .

    Please note that corrections may take a couple of weeks to filter through the various RePEc services.

    IDEAS is a RePEc service. RePEc uses bibliographic data supplied by the respective publishers.