Solar wind plasma noise correlated between LISA and Taiji can bias stochastic gravitational wave background parameter estimates by up to 19% of Fisher uncertainty under large-scale correlation assumptions.
Smetana, Background for gravitational wave signal at lisa from refractive index of solar wind plasma, Monthly Notices of the Royal Astronomical Society: Letters499, L77 (2020)
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Effects of Solar Wind Plasma Noise on Stochastic Gravitational Wave Background Searches with the LISA-Taiji Network
Solar wind plasma noise correlated between LISA and Taiji can bias stochastic gravitational wave background parameter estimates by up to 19% of Fisher uncertainty under large-scale correlation assumptions.