Using the antenna impedance to estimate soil electrical parameters for the MIST global 21-cm experiment
arXiv:2503.19401 · doi:10.1088/1538-3873/adfa43
Abstract
Radio experiments trying to detect the global ~cm signal from the early Universe are very sensitive to the electrical properties of their environment. For ground-based experiments with the antenna above the soil it is critical to characterize the effect from the soil on the sky observations. This characterization requires estimating the soil's electrical conductivity and relative permittivity in the same frequency range as the observations. Here we present our initial effort to estimate the conductivity and relative permittivity of the soil using the impedance of an antenna mounted at a distance above the surface. In this technique, the antenna used for soil characterization is the same as the antenna used for sky observations. To demonstrate the technique we use the antenna of the MIST global ~cm experiment. We measured the antenna impedance at three sites in the Greater Concepción area, Chile. The measurements were done between and ~MHz, matching the range used by MIST for sky observations. The soil parameters were estimated by fitting the impedance measurements with electromagnetic simulations of the antenna and soil. In this initial effort the soil was modeled as homogeneous. The conductivity at the three sites was found to be between and ~Sm, and the relative permittivity between and . The percent precision of the estimates at probability is, with one exception, better (lower) than . The best-fit simulations have a better than agreement with the measurements relative to the peak values of the resistance and reactance across our frequency range. For MIST, these results represent a successful proof of concept of the use of the antenna impedance for soil characterization, and are expected to significantly improve in future implementations.
Updated to match version published in PASP in August 2025
References in corpus (16)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- 21-cm cosmology
- All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz
- A Ground Plane Artifact that Induces an Absorption Profile in Averaged Spectra from Global 21-cm Measurements - with Possible Application to EDGES
- Results from EDGES High-Band: I. Constraints on Phenomenological Models for the Global cm Signal
- The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28
- Characterization of a Low-Frequency Radio Astronomy Prototype Array in Western Australia
- Mapper of the IGM spin temperature: instrument overview
- Cassiopeia A, Cygnus A, Taurus A, and Virgo A at ultra-low radio frequencies
- Validation of EDGES Low-Band Antenna Beam Model
- The Evolution of Cas A at Low Radio Frequencies
- Antenna beam characterisation for the global 21cm experiment LEDA and its impact on signal model parameter reconstruction
- Spectral index of the Galactic foreground emission in the 50-87 MHz range
- Absolute Calibration of Diffuse Radio Surveys at 45 and 150 MHz
- Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity
- Analytic approximations of scattering effects on beam chromaticity in 21-cm global experiments