Solar irradiance changes and phytoplankton productivity in Earth's ocean following astrophysical ionizing radiation events
Patrick J. Neale (SERC), Brian C. Thomas (Washburn Univ.)

TL;DR
This study predicts that astrophysical ionizing radiation events cause minor decreases in marine phytoplankton productivity due to changes in spectral irradiance, with effects varying by water depth and spectral response.
Contribution
It introduces a spectral model of phytoplankton photosynthesis response to ionizing radiation events, integrating remote sensing data to predict productivity changes in Earth's oceans.
Findings
Productivity declined by up to 2-3% overall after simulated events.
Decreases were larger (5-7%) when considering only the surface mixed layer.
Decreased utilizable PAR at depth due to NO2 haze was a key factor.
Abstract
Two atmospheric responses to simulated astrophysical ionizing radiation events significant to life on Earth are production of odd-nitrogen species, especially NO2, and subsequent depletion of stratospheric ozone. Ozone depletion increases incident short-wavelength ultraviolet radiation (UVB, 280-315 nm) and longer ( > 600 nm) wavelengths of photosynthetically available radiation (PAR, 400 -700 nm). On the other hand, the NO2 haze decreases atmospheric transmission in the long-wavelength UVA (315-400 nm) and short wavelength PAR. Here we use the results of previous simulations of incident spectral irradiance following an ionizing radiation event to predict changes in Terran productivity focusing on photosynthesis of marine phytoplankton. The prediction is based on a spectral model of photosynthetic response developed for the dominant genera in central regions of the ocean (Synechococcus…
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