Testing the ACA Phase Correction Scheme using the SMA
Satoki Matsushita (1,2), Yu-Lin Chen (1,3,4) ((1) ASIAA, (2) ALMA,, (3) NTU, (4) Taipei County Yong-Ho Junior High School)

TL;DR
This study tests the ACA phase correction scheme for ALMA using SMA observations, demonstrating effective interpolation but limited extrapolation, with phase fluctuations explained by a frozen phase screen model.
Contribution
It provides observational validation of the ACA phase correction scheme using SMA data, highlighting the effectiveness of interpolation and challenges with extrapolation.
Findings
Interpolation improves phase correction results.
Extrapolation often does not improve phase stability.
Phase fluctuations are consistent with a frozen phase screen model.
Abstract
We conducted the observational tests of a phase correction scheme for the Atacama Compact Array (ACA) of the Atacama Large Millimeter and submillimeter Array (ALMA) using the Submillimeter Array (SMA). Interferometers at millimeter- and submillimeter-wave are highly affected by the refraction induced by water vapor in the troposphere, which results as phase fluctuations. The ACA is planning to compensate the atmospheric phase fluctuations using the phase information of the outermost antennas with interpolating to the inner antennas by creating a phase screen. The interpolation and extrapolation phase correction schemes using phase screens are tested with the SMA to study how effective these schemes are. We produce a plane of a wavefront (phase screen) from the phase information of three antennas for each integration, and this phase screen is used for the interpolation and extrapolation…
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