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The protoperithecia assay (PPA) quantifies photoperiodic responses in the fungus Neurospora crassa. Many organisms measure day and night length to coordinate biological processes in a phenomenon known as photoperiodism1,2,3,4,5,6,7,8. In this assay, the development of the female sexual structure, the protoperithecium, serves as a measurable, light-dependent proxy for photoperiodic response. Although photoperiodism is well characterized in plants through night-break experiments3, fewer standardized approaches exist for quantifying photoperiodic responses in non-photosynthetic eukaryotes such as fungi. N. crassa provides a tractable model system for this purpose due to its well-defined genetics and light-responsive developmental pathways. Photoperiod-dependent regulation of reproductive timing has been observed across organisms1,2,3,4,5,6,7,8, supporting the relevance of light-driven physiological responses; however, mechanistic studies in fungi remain limited by the lack of reproducible assays.
Protoperithecia are premature female sexual structures in N. crassa. They arise from ascogonia, which develop coiled trichogynes that fuse with hyphae or conidia of the opposite mating type9. Following fusion, nuclei from the “male” partner enter the protoperithecium. The number of protoperithecia produced is seasonally regulated and strongly light-induced10. Photoperiodic regulation is central to ecology, chronobiology, and fungal physiology because many clock-controlled processes depend on light. Light influences numerous genetic pathways, including photoreceptors, kinases, and light-transduction mechanisms linked to sexual development11. Protoperithecia are well-suited for measuring photoperiodic output because they are easily visualized under a microscope and respond sensitively to light.
Despite the importance of photoperiodism in fungi, few standardized and reproducible assays are available to quantify protoperithecia production under controlled light cycles. A medium-throughput, plate-based assay is valuable because fungi are inexpensive and easily maintained model organisms, enabling systematic analysis of light-induced sexual development and gene function. Most photoperiodism research has focused on plants, whereas equivalent quantitative frameworks for fungal systems remain limited. In other organisms, including insects, light-dependent phenomena such as diapause are well characterized7, but comparable approaches in fungi are lacking. This gap restricts reproducible comparison of photoperiodic responses across strains and experimental conditions.
The PPA builds on a 2004 study that measured protoperithecia production across increasing day lengths, from constant darkness to constant light, in the band (bd) mutant (ras-1bd), which has been used in circadian studies4,12. Photoperiod-dependent changes in protoperithecia production were observed in this background. The present workflow adapts and extends this approach using the reference strain FGSC 2489, which is associated with whole-genome sequencing and knockout resources13,14. The assay quantifies the average number of protoperithecia produced under defined photoperiods over one week as a proxy for photoperiodic response. This approach standardizes culture conditions, imaging, and quantification, enabling reproducible comparison across experimental conditions and strains. Key methodological advances include standardized plate-based culture conditions, defined photoperiod exposure parameters, quadrant-based imaging, and a reproducible quantification workflow.
This protocol quantifies photoperiodic responses in N. crassa by measuring protoperithecia formation following exposure to defined light–dark cycles. For each photoperiodic condition, four biological replicates are used, each consisting of one independently inoculated synthetic crossing (SC) plate. Four images are collected per plate and averaged to generate a single value per biological replicate for statistical analysis. Plates are incubated for seven days under calibrated photoperiods (e.g., 12 h:12 h or 8 h:16 h light–dark cycles).
A data logger is placed inside the growth chamber to continuously record light intensity, temperature, and humidity, thereby verifying stable environmental conditions. Light intensity is maintained above 1,000 lux, as lower levels reduce protoperithecia production. Excessive illumination is avoided to prevent increases in chamber temperature and confounding thermal effects. After incubation, macroconidia are gently removed with a moistened paper towel saturated with 70% ethanol. Four evenly spaced quadrants at the perimeter of each plate are imaged at 40× magnification using a stereo microscope under brightfield illumination. Protoperithecia are counted manually using an image-processing package, and average counts per plate are used for statistical comparisons across photoperiods.