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.
Abbottet al., Upper limits on the isotropic gravitational-wave background from advanced ligo’s and advanced virgo’s third observing run, Physical Review D 104, 022004 (2021)
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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.