Evaluating the regional consistency of astronomical observing conditions across Dome A
With excellent seeing conditions, ultra-low infrared background noise, high frequency of space debris transits, and continuous polar night coverage, Dome A in Antarctica has become an ideal platform for ground-based astronomy and space situational monitoring. As a crucial observatory site for international deep space, deep Earth, deep sea, and polar exploration, it is very important to evaluate the suitability of Dome A as an observatory site. However, owing to extreme environmental constraints, the evaluation of site conditions is mainly based on single-point measurements, making it challenging to comprehensively evaluate the effective site range and uniformity. This study integrated satellite remote sensing data to develop a cross-comparison framework for diverse indicators across Dome A, to evaluate its spatial uniformity. We find that the area surrounding the Dome A site, defined within a roughly 1° × 1° latitude and longitude range, possesses excellent astronomical observation conditions.
Authors
- Kaiwen Zheng (ORCID: https://orcid.org/0000-0001-6219-8954)
- T. Zhang
- Xiaoyan Li (ORCID: https://orcid.org/0000-0002-0282-5423)
- Jiali Chen
- Peng Jiang (ORCID: https://orcid.org/0000-0002-5387-7952)
- Han Wang (ORCID: https://orcid.org/0009-0008-2794-2520)
- Kun Ma (ORCID: https://orcid.org/0000-0002-9232-4912)
- Shi‐Yi Wang (ORCID: https://orcid.org/0000-0002-3294-5784)
- H Song
Publication Details
- Journal
- Astronomical Techniques and Instrument
- Published
- 2025-09-03
- DOI
- https://doi.org/10.3724/ati2025061
- Primary Topic
- Adaptive optics and wavefront sensing
- Type
- article
- Field-Weighted Citation Impact
- 0.00