Intercontinental network control platform and robotic observation for Chinese Antarctic telescopes

Lingzhe Xu

doi:10.1117/12.925629

24 September 2012 Intercontinental network control platform and robotic observation for Chinese Antarctic telescopes

Lingzhe Xu

Proceedings Volume 8451, Software and Cyberinfrastructure for Astronomy II; 845114 (2012) https://doi.org/10.1117/12.925629
Event: SPIE Astronomical Telescopes + Instrumentation, 2012, Amsterdam, Netherlands

Abstract

The Chinese astronomical exploration in Antarctic region has been initialized and stepped forward. The R&D roadmap in this regard identifies each progressive step. For the past several years China has set up Kunlun station at Antarctic Dome-A, and Chinese Small Telescope ARray (CSTAR) has already been up and running regularly. In addition, Antarctic Schmidt Telescopes (AST3_1) was transported to the area in the year of 2011 and has recently been placed in service for some time and followed with telescopes in larger size predictably more to come. Antarctic region is one of a few best sites left on the Earth for astronomical telescope observation, yet with worst fundamental living conditions for human survival and activities. To meet such a tough challenge it is essential to establish an efficient and reliable means of remote access for telescope routine observation. This paper outlines the remote communication for CSTAR and AST3_1, and further proposes an intercontinental network control platform for Chinese Antarctic telescope array with remote full-automatic control and robotic observation and management. A number of technical issues for telescope access such as the unattended operation, the bandwidth based on iridium satellite transmission as well as the means of reliable and secure communication among other things are all reviewed and further analyzed.

Citation Download Citation

Lingzhe Xu "Intercontinental network control platform and robotic observation for Chinese Antarctic telescopes", Proc. SPIE 8451, Software and Cyberinfrastructure for Astronomy II, 845114 (24 September 2012); https://doi.org/10.1117/12.925629

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