Analysis reveals increased shunt resistance with magnetic field in bifacial c-Si cells, indicating effects of illumination geometry.
We analyze the influence of a weak magnetic field (B = 10-4 to 10-3 T) on the shunt resistance Rsh of bifacial polycrystalline-silicon solar cells, focusing on the near short-circuit region where the initial slope of the J-V curves sensitively reveals leakage. The device is modeled using a three-dimensional, grain-column approach. The transport equations are solved with diffusivity and diffusion length allowed to depend on B, while base thickness H (100-400 um) and illumination mode (front, rear, dual) are swept systematically. Joint parameter extraction {J0, n, Rs, Rsh} is performed from the J-V characteristics and interpreted using standard experimental indicators (stability of the photocurrent plateau, low-voltage slope, evolution of the open-circuit voltage). Three key findings emerge. (i) Rsh increases with the carrier-collection velocity and, in general, with B, but the magnitude of this change depends strongly on illumination geometry
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Touré et al. (2025) studied this question.
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