Title: First light from the Dome C (Antarctica) of a phase knife stellar coronagraph Authors: Geraldine Guerri, Lyu Abe, Jean-Baptiste Daban, Eric Aristidi, Philippe Bendjoya, Jean-Pierre Rivet, Farrokh Vakili
We report on the first daytime on-sky results of a Phase Knife stellar Coronagraph operated in the visible from the French-Italian Concordia station at Dome C of Antarctica. This site has proven in the last few years to offer excellent atmospheric seeing conditions for high spatial resolution observations. The coronagraphic performances obtained from laboratory experiments and numerical models have been compared with those measured from daytime on-sky data recorded on bright single and multiple stars: Canopus (HD 45348), and alpha Centauri (HD 128620J). No correction system was used (adaptive optics or tip-tilt mirror) so that atmospheric turbulence alone defines the image quality, and thus the coronagraphic performances. Moreover, the experiment could not run under optimal operational conditions due to hardware/software problems. Satisfactory results have been obtained: broad band total rejection exceeding 15 were attained in the visible. This first day-time observation campaign yields an experimental feedback on how to improve the instrument to get optimal performances during future night-time observation runs.
During December 2008 and January 2009, scientists from around the world are examining an Antarctic snowfield using a variety of different satellites. The purpose of this exercise is to see how measurements from each satellite differ when viewing the same patch of ground, and then to see how this information can be best used to improve the performance of individual satellites and the data they produce. Ultimately this will lead to improvements in the quality of satellite data that is used in climate studies and improve our ability to mitigate appropriately. The measurements for this intercomparison exercise will be taken over a snowfield in Antarctica known as 'DOME C'. These can only be performed in December and January when the Sun is relatively high in the sky during the southern hemisphere summer.
Title: Submm/FIR astronomy in Antarctica: Potential for a large telescope facility Authors: Vincent Minier (AIME, SAp), V. Minier, L. Olmi, P.-O. Lagage, L. Spinoglio, G.A. Durand, E. Daddi, D. Galilei, H. Gallee, C. Kramer, D. Marrone, E. Pantin, L. Sabbatini, N. Schneider, N. Tothill, L. Valenziano, C. Veyssiere
Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500 micron regime, i.e. for far-infrared (FIR) and submillimetre (submm) astronomy. We present an overview of potential science cases that could be addressed with a large telescope facility at Dome C. This paper also includes a presentation of the current knowledge about the site characterics in terms of atmospheric transmission, stability, sky noise and polar constraints on telescopes. Current and future site testing campaigns are finally described.
Title: Solar Physics and the Solar-Stellar Connection at Dome C Authors: C. Denker (1), K. G. Strassmeier (1) ((1)Astrophysikalisches Institut Potsdam, Germany)
Solar magnetic fields evolve on many time-scales, e.g., the generation, migration, and dissipation of magnetic flux during the 22-year magnetic cycle of the Sun. Active regions develop and decay over periods of weeks. The build-up of magnetic shear in active regions can occur within less than a day. At the shortest time-scales, the magnetic field topology can change rapidly within a few minutes as the result of eruptive events such as flares, filament eruptions, and coronal mass ejections. The unique daytime seeing characteristics at Dome C, i.e., continuous periods of very good to excellent seeing during almost the entire Antarctic summer, allow us to address many of the top science cases related to the evolution of solar magnetic fields. We introduce the Advanced Solar Photometric Imager and Radiation Experiment and present the science cases for synoptic solar observations at Dome C. Furthermore, common science cases concerning the solar-stellar connection are discussed in the context of the proposed International Concordia Explorer Telescope.
The new South Pole Telescope has successfully collected its first light as part of a long-term project to unravel one of the biggest mysteries in cosmology, researchers announced today. The goal of SPT is to learn the nature of mysterious dark energy, an antigravity force that permeates the cosmos and is driving the universe apart at an ever-increasing pace. The telescope does not make conventional images. Instead, it will take advantage of excellent viewing conditions—cold and dry—in Antarctica to detect the cosmic microwave background (CMB) radiation. The CMB is said to be the afterglow of the Big Bang.
First light achieved with the 10-m South Pole Telescope, February 16, 2007. Last night the 10-meter South Pole Telescope with its camera operating at millimeter wavelengths and cooled to 1/4 degree above absolute zero achieved first light. Maps of Jupiter at wavelengths at 2 mm and 3 mm were obtained by scanning the telescope across the planet. These maps showed the telescope, camera and optics are working as designed. First light with the SPT is a major milestone for the project and is a fitting conclusion to a remarkably productive summer season for the South Pole Station. We now look forward to fully characterizing the instrument and beginning cosmological observations.
China plans to build an observatory at the South Pole, setting up 400 telescopes there over the next 10 years in cooperation with the United States, Australia and France. The observatory will be built at Dome A, the highest point on the continent at 4,093 meters above sea level. Dome A is located at latitude 80.22 south and longitude 77.21 east, according to the Chinese Academy of Sciences (CAS).
"The images taken by the telescopes at the South Pole may be almost as good as those of the Hubble Space Telescope" - Ye Shuhua, a CAS academician.
The South Pole has the clearest sky on Earth, allowing scientists to obtain very sharp images of sky phenomena. In scientific parlance, "seeing conditions" are excellent because Antarctica's bitter cold removes the thermal background radiation that reduces the sensitivity of telescopes in warmer climates. China has decided to build a third permanent research station at Dome A, which will support the construction of the observatory. Ye, who is also the director of the China Antarctic Astronomical Centre, which was founded at the end of 2006, said the United States and Australia had built telescopes at Dome C Icecap, which is 3,280 meters above sea level at latitude 74.50 south and longitude 123.00 east.
"The telescopes at Dome A may turn out to be more sensitive than Dome C because the wind is not so strong at Dome A. The cost of the South Pole Observatory is higher than at other sites on Earth, but lower than the cost of a space telescope" - Ye Shuhua.
She said China will cooperate with the United States, Australia and France to build 400 telescopes, each with a diameter of 50 centimetres, in order to explore dark energy and other mysterious substances in the sky.
Beginning in winter 2006, a group of scientists, technicians, and engineers will build the largest telescope ever deployed at the South Pole. Follow their work in a series of Webcasts that track the team's progress as they piece together the 10-meter-diameter telescope. The South Pole Telescope will be an important part of the International Polar Year activities. Once it's completed in January 2007, the telescope will give astronomers a powerful new tool to explore dark energy, the mysterious force that may be causing the universe to accelerate.
Dome A (Dome Argus) is an Antarctic plateau located 1200 kilometres inland. It is thought to be one of the coldest naturally occurring places on Earth, with temperatures believed to reach -90 °C. It is the highest ice feature in Antarctica, comprising a dome or eminence of just over 4,000 m elevation, located near the centre of East Antarctica and approximately midway between the head of Lambert Glacier and the South Pole.
Position: 81°0′S 77°0′E
The name "Dome Argus" was given by the Scott Polar Research Institute from Greek mythology; Argus built the ship in which Jason and the Argonauts travelled.