This paper discusses the methodology for processing measurements of solar terahertz radiation fluxes and solar flares that will be recorded in the upcoming Solntse-Terahertz experiment using equipment installed onboard the International Space Station (ISS). Possible distortions of measurement results due to the registration of spurious emissions that are not included in the passband of the installation channel, as well as methods for restoring the “primary” radiation spectrum, are discussed.
Logachev et al. (Thu,) studied this question.