A concept and design study for a lunar-orbiting radiometer for the global 21-cm cosmic dawn signal, with simulations indicating detection sensitivity for standard models.
Quantifying Ionospheric Effects on Global 21-cm Observations
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abstract
We modelled the two major layer of Earth's ionosphere, the F-layer and the D-layer, by a simplified spatial model with temporal variance to study the chromatic ionospheric effects on global 21-cm observations. From the analyses, we found that the magnitude of the ionospheric disruptions due to ionospheric refraction and absorption can be greater than the expected global 21-cm signal, and the variation of its magnitude can differ, depending on the ionospheric conditions. Within the parameter space adopted in the model, the shape of the global 21-cm signal is distorted after propagating through the ionosphere, while its amplitude is weakened. It is observed that the ionospheric effects do not cancel out over time, and thus should be accounted for in the foreground calibration at each timestep to account for the chromaticity introduced by the ionosphere.
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PRATUSH experiment concept and design overview
A concept and design study for a lunar-orbiting radiometer for the global 21-cm cosmic dawn signal, with simulations indicating detection sensitivity for standard models.